TESLA Born
N.GENESIS
Three-Body
URRAS Moon
LE GUIN*
Matrix '99
Nikola Tesla was a Serbian‑American engineer, futurist, and inventor born on 10 July 1856 in Smiljan, then part of the Austrian Empire, and he died on 7 January 1943 in New York City. He is best known for his contributions to the design of the modern alternating current (AC) electricity supply system and for pioneering work in electromagnetism and electrical engineering. Tesla studied engineering and physics in the 1870s without receiving a degree, and he gained practical experience in the early 1880s working in telephony and at Continental Edison in the emerging electric power industry. In 1884, he emigrated to the United States and became a naturalized citizen, briefly working for the Edison Machine Works in New York before striking out on his own to develop his inventions and ideas. With partners to finance and market his work, he set up laboratories and companies in New York that produced a range of electrical and mechanical devices. His AC induction motor and related polyphase AC patents, licensed by Westinghouse Electric in 1888, earned him considerable recognition and became the cornerstone of the polyphase system marketed across the expanding electrical grid. Tesla’s work encompassed a broad array of technologies and concepts. He developed the rotating magnetic field, which forms the basis of most alternating current machinery, and invented the Tesla coil, an induction coil capable of generating high‑voltage, high‑frequency currents, widely used in radio technology and other applications.
Nikola Tesla was a Serbian‑American engineer, futurist, and inventor born on 10 July 1856 in Smiljan, then part of the Austrian Empire, and he died on 7 January 1943 in New York City. He is best known for his contributions to the design of the modern alternating current (AC) electricity supply system and for pioneering work in electromagnetism and electrical engineering. Tesla studied engineering and physics in the 1870s without receiving a degree, and he gained practical experience in the early 1880s working in telephony and at Continental Edison in the emerging electric power industry. In 1884, he emigrated to the United States and became a naturalized citizen, briefly working for the Edison Machine Works in New York before striking out on his own to develop his inventions and ideas. With partners to finance and market his work, he set up laboratories and companies in New York that produced a range of electrical and mechanical devices. His AC induction motor and related polyphase AC patents, licensed by Westinghouse Electric in 1888, earned him considerable recognition and became the cornerstone of the polyphase system marketed across the expanding electrical grid. Tesla’s work encompassed a broad array of technologies and concepts. He developed the rotating magnetic field, which forms the basis of most alternating current machinery, and invented the Tesla coil, an induction coil capable of generating high‑voltage, high‑frequency currents, widely used in radio technology and other applications.
Nikola Tesla was a Serbian‑American engineer, futurist, and inventor born on 10 July 1856 in Smiljan, then part of the Austrian Empire, and he died on 7 January 1943 in New York City. He is best known for his contributions to the design of the modern alternating current (AC) electricity supply system and for pioneering work in electromagnetism and electrical engineering. Tesla studied engineering and physics in the 1870s without receiving a degree, and he gained practical experience in the early 1880s working in telephony and at Continental Edison in the emerging electric power industry. In 1884, he emigrated to the United States and became a naturalized citizen, briefly working for the Edison Machine Works in New York before striking out on his own to develop his inventions and ideas. With partners to finance and market his work, he set up laboratories and companies in New York that produced a range of electrical and mechanical devices. His AC induction motor and related polyphase AC patents, licensed by Westinghouse Electric in 1888, earned him considerable recognition and became the cornerstone of the polyphase system marketed across the expanding electrical grid. Tesla’s work encompassed a broad array of technologies and concepts. He developed the rotating magnetic field, which forms the basis of most alternating current machinery, and invented the Tesla coil, an induction coil capable of generating high‑voltage, high‑frequency currents, widely used in radio technology and other applications.
Nikola Tesla was a Serbian‑American engineer, futurist, and inventor born on 10 July 1856 in Smiljan, then part of the Austrian Empire, and he died on 7 January 1943 in New York City. He is best known for his contributions to the design of the modern alternating current (AC) electricity supply system and for pioneering work in electromagnetism and electrical engineering. Tesla studied engineering and physics in the 1870s without receiving a degree, and he gained practical experience in the early 1880s working in telephony and at Continental Edison in the emerging electric power industry. In 1884, he emigrated to the United States and became a naturalized citizen, briefly working for the Edison Machine Works in New York before striking out on his own to develop his inventions and ideas. With partners to finance and market his work, he set up laboratories and companies in New York that produced a range of electrical and mechanical devices. His AC induction motor and related polyphase AC patents, licensed by Westinghouse Electric in 1888, earned him considerable recognition and became the cornerstone of the polyphase system marketed across the expanding electrical grid. Tesla’s work encompassed a broad array of technologies and concepts. He developed the rotating magnetic field, which forms the basis of most alternating current machinery, and invented the Tesla coil, an induction coil capable of generating high‑voltage, high‑frequency currents, widely used in radio technology and other applications.
(AC) Power
FERROMAG.
Quantum—No
Neo Choice
MINITEL80
Hard Disk
He investigated the wireless transmission of power and information and conducted experiments with high‑frequency currents, resonance phenomena, and lighting systems. Tesla also explored early demonstrations of shadowgraphs similar to X‑rays and experimented with electrical resonance and the transmission of energy without wires. His inventive mind led him to envision global networks for communication and energy distribution, although many of his most ambitious projects, such as wireless power transmission on a worldwide scale, were never fully realized due to financial and technical obstacles. Tesla’s career included intense experimentation, public demonstrations, and patent battles, and he received both acclaim and financial instability throughout his life. He gave exhibitions in his laboratory in which he lit lamps by allowing electricity to flow through his body to allay fears of alternating currents, and his AC power system was used to light the World’s Columbian Exposition in Chicago in 1893, contributing to Westinghouse’s success in installing power machinery at Niagara Falls by 1896. In later years, Tesla pursued projects such as terrestrial stationary waves and wireless world broadcasting towers, but many of these ventures were abandoned due to lack of funds or support. Although he faced setbacks, including the loss of potential Nobel Prizes and financial difficulties, he remained dedicated to research and innovation. After his death, his papers, notes, and inventions were preserved, and he has since been recognized as one of the most influential figures in the history of electrical engineering, with his legacy continuing to shape modern technology.
He investigated the wireless transmission of power and information and conducted experiments with high‑frequency currents, resonance phenomena, and lighting systems. Tesla also explored early demonstrations of shadowgraphs similar to X‑rays and experimented with electrical resonance and the transmission of energy without wires. His inventive mind led him to envision global networks for communication and energy distribution, although many of his most ambitious projects, such as wireless power transmission on a worldwide scale, were never fully realized due to financial and technical obstacles. Tesla’s career included intense experimentation, public demonstrations, and patent battles, and he received both acclaim and financial instability throughout his life. He gave exhibitions in his laboratory in which he lit lamps by allowing electricity to flow through his body to allay fears of alternating currents, and his AC power system was used to light the World’s Columbian Exposition in Chicago in 1893, contributing to Westinghouse’s success in installing power machinery at Niagara Falls by 1896. In later years, Tesla pursued projects such as terrestrial stationary waves and wireless world broadcasting towers, but many of these ventures were abandoned due to lack of funds or support. Although he faced setbacks, including the loss of potential Nobel Prizes and financial difficulties, he remained dedicated to research and innovation. After his death, his papers, notes, and inventions were preserved, and he has since been recognized as one of the most influential figures in the history of electrical engineering, with his legacy continuing to shape modern technology.
He investigated the wireless transmission of power and information and conducted experiments with high‑frequency currents, resonance phenomena, and lighting systems. Tesla also explored early demonstrations of shadowgraphs similar to X‑rays and experimented with electrical resonance and the transmission of energy without wires. His inventive mind led him to envision global networks for communication and energy distribution, although many of his most ambitious projects, such as wireless power transmission on a worldwide scale, were never fully realized due to financial and technical obstacles. Tesla’s career included intense experimentation, public demonstrations, and patent battles, and he received both acclaim and financial instability throughout his life. He gave exhibitions in his laboratory in which he lit lamps by allowing electricity to flow through his body to allay fears of alternating currents, and his AC power system was used to light the World’s Columbian Exposition in Chicago in 1893, contributing to Westinghouse’s success in installing power machinery at Niagara Falls by 1896. In later years, Tesla pursued projects such as terrestrial stationary waves and wireless world broadcasting towers, but many of these ventures were abandoned due to lack of funds or support. Although he faced setbacks, including the loss of potential Nobel Prizes and financial difficulties, he remained dedicated to research and innovation. After his death, his papers, notes, and inventions were preserved, and he has since been recognized as one of the most influential figures in the history of electrical engineering, with his legacy continuing to shape modern technology.
He investigated the wireless transmission of power and information and conducted experiments with high‑frequency currents, resonance phenomena, and lighting systems. Tesla also explored early demonstrations of shadowgraphs similar to X‑rays and experimented with electrical resonance and the transmission of energy without wires. His inventive mind led him to envision global networks for communication and energy distribution, although many of his most ambitious projects, such as wireless power transmission on a worldwide scale, were never fully realized due to financial and technical obstacles. Tesla’s career included intense experimentation, public demonstrations, and patent battles, and he received both acclaim and financial instability throughout his life. He gave exhibitions in his laboratory in which he lit lamps by allowing electricity to flow through his body to allay fears of alternating currents, and his AC power system was used to light the World’s Columbian Exposition in Chicago in 1893, contributing to Westinghouse’s success in installing power machinery at Niagara Falls by 1896. In later years, Tesla pursued projects such as terrestrial stationary waves and wireless world broadcasting towers, but many of these ventures were abandoned due to lack of funds or support. Although he faced setbacks, including the loss of potential Nobel Prizes and financial difficulties, he remained dedicated to research and innovation. After his death, his papers, notes, and inventions were preserved, and he has since been recognized as one of the most influential figures in the history of electrical engineering, with his legacy continuing to shape modern technology.
Shevek go
THE ONE?
Carbon (C)
Foundatio→
Evangelion
ANGULAR
Ferromagnetism is a property of certain materials such as iron, cobalt and nickel that results in significant observable magnetic permeability and in many cases significant magnetic coercivity, allowing the material to form a permanent magnet. Ferromagnetic materials are noticeably attracted to a magnet, which is a consequence of their substantial magnetic permeability. Magnetic permeability describes the induced magnetization due to the presence of an external magnetic field. Whether a piece of steel acquires permanent magnetization depends on both the strength of the applied field and the coercivity of that particular piece of steel, which varies with its composition and heat treatment. In physics, multiple types of material magnetism have been distinguished. Ferromagnetism, along with the similar effect ferrimagnetism, is the strongest type and is responsible for the common phenomenon of everyday magnetism. A common example of a permanent magnet is a refrigerator magnet. Substances respond weakly to magnetic fields by paramagnetism, diamagnetism and antiferromagnetism, but the forces are so weak that they can be detected only by instruments.
Ferromagnetism is a property of certain materials such as iron, cobalt and nickel that results in significant observable magnetic permeability and in many cases significant magnetic coercivity, allowing the material to form a permanent magnet. Ferromagnetic materials are noticeably attracted to a magnet, which is a consequence of their substantial magnetic permeability. Magnetic permeability describes the induced magnetization due to the presence of an external magnetic field. Whether a piece of steel acquires permanent magnetization depends on both the strength of the applied field and the coercivity of that particular piece of steel, which varies with its composition and heat treatment. In physics, multiple types of material magnetism have been distinguished. Ferromagnetism, along with the similar effect ferrimagnetism, is the strongest type and is responsible for the common phenomenon of everyday magnetism. A common example of a permanent magnet is a refrigerator magnet. Substances respond weakly to magnetic fields by paramagnetism, diamagnetism and antiferromagnetism, but the forces are so weak that they can be detected only by instruments.
Ferromagnetism is a property of certain materials such as iron, cobalt and nickel that results in significant observable magnetic permeability and in many cases significant magnetic coercivity, allowing the material to form a permanent magnet. Ferromagnetic materials are noticeably attracted to a magnet, which is a consequence of their substantial magnetic permeability. Magnetic permeability describes the induced magnetization due to the presence of an external magnetic field. Whether a piece of steel acquires permanent magnetization depends on both the strength of the applied field and the coercivity of that particular piece of steel, which varies with its composition and heat treatment. In physics, multiple types of material magnetism have been distinguished. Ferromagnetism, along with the similar effect ferrimagnetism, is the strongest type and is responsible for the common phenomenon of everyday magnetism. A common example of a permanent magnet is a refrigerator magnet. Substances respond weakly to magnetic fields by paramagnetism, diamagnetism and antiferromagnetism, but the forces are so weak that they can be detected only by instruments.
Ferromagnetism is a property of certain materials such as iron, cobalt and nickel that results in significant observable magnetic permeability and in many cases significant magnetic coercivity, allowing the material to form a permanent magnet. Ferromagnetic materials are noticeably attracted to a magnet, which is a consequence of their substantial magnetic permeability. Magnetic permeability describes the induced magnetization due to the presence of an external magnetic field. Whether a piece of steel acquires permanent magnetization depends on both the strength of the applied field and the coercivity of that particular piece of steel, which varies with its composition and heat treatment. In physics, multiple types of material magnetism have been distinguished. Ferromagnetism, along with the similar effect ferrimagnetism, is the strongest type and is responsible for the common phenomenon of everyday magnetism. A common example of a permanent magnet is a refrigerator magnet. Substances respond weakly to magnetic fields by paramagnetism, diamagnetism and antiferromagnetism, but the forces are so weak that they can be detected only by instruments.
Black Hole
Magnemite
Time Cap.
Earthsea
ANSIBLE
Teleport
Permanent magnets, materials magnetized by an external magnetic field and remaining magnetized, are either ferromagnetic or ferrimagnetic. Relatively few materials are ferromagnetic; common ones are the metals iron, cobalt and nickel, most of their alloys and certain rare‑earth metals. Ferromagnetism is widely used in industrial applications and modern technology, in electromagnetic and electromechanical devices such as electromagnets, electric motors, generators, transformers, magnetic storage including tape recorders and hard disks, and nondestructive testing of materials. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned. Permanent magnets are made from hard ferromagnetic or ferrimagnetic materials subjected to special processing in a strong magnetic field to align their internal microcrystalline structure, making them difficult to demagnetize. The overall strength of a magnet is measured by its magnetic moment or total magnetic flux, and the local strength of magnetism in a material is measured by its magnetization. The Bohr‑Van Leeuwen theorem showed that classical physics is unable to account for magnetic phenomena, which depend on the quantum mechanical description of atoms.
Permanent magnets, materials magnetized by an external magnetic field and remaining magnetized, are either ferromagnetic or ferrimagnetic. Relatively few materials are ferromagnetic; common ones are the metals iron, cobalt and nickel, most of their alloys and certain rare‑earth metals. Ferromagnetism is widely used in industrial applications and modern technology, in electromagnetic and electromechanical devices such as electromagnets, electric motors, generators, transformers, magnetic storage including tape recorders and hard disks, and nondestructive testing of materials. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned. Permanent magnets are made from hard ferromagnetic or ferrimagnetic materials subjected to special processing in a strong magnetic field to align their internal microcrystalline structure, making them difficult to demagnetize. The overall strength of a magnet is measured by its magnetic moment or total magnetic flux, and the local strength of magnetism in a material is measured by its magnetization. The Bohr‑Van Leeuwen theorem showed that classical physics is unable to account for magnetic phenomena, which depend on the quantum mechanical description of atoms.
Permanent magnets, materials magnetized by an external magnetic field and remaining magnetized, are either ferromagnetic or ferrimagnetic. Relatively few materials are ferromagnetic; common ones are the metals iron, cobalt and nickel, most of their alloys and certain rare‑earth metals. Ferromagnetism is widely used in industrial applications and modern technology, in electromagnetic and electromechanical devices such as electromagnets, electric motors, generators, transformers, magnetic storage including tape recorders and hard disks, and nondestructive testing of materials. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned. Permanent magnets are made from hard ferromagnetic or ferrimagnetic materials subjected to special processing in a strong magnetic field to align their internal microcrystalline structure, making them difficult to demagnetize. The overall strength of a magnet is measured by its magnetic moment or total magnetic flux, and the local strength of magnetism in a material is measured by its magnetization. The Bohr‑Van Leeuwen theorem showed that classical physics is unable to account for magnetic phenomena, which depend on the quantum mechanical description of atoms.
Permanent magnets, materials magnetized by an external magnetic field and remaining magnetized, are either ferromagnetic or ferrimagnetic. Relatively few materials are ferromagnetic; common ones are the metals iron, cobalt and nickel, most of their alloys and certain rare‑earth metals. Ferromagnetism is widely used in industrial applications and modern technology, in electromagnetic and electromechanical devices such as electromagnets, electric motors, generators, transformers, magnetic storage including tape recorders and hard disks, and nondestructive testing of materials. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned. Permanent magnets are made from hard ferromagnetic or ferrimagnetic materials subjected to special processing in a strong magnetic field to align their internal microcrystalline structure, making them difficult to demagnetize. The overall strength of a magnet is measured by its magnetic moment or total magnetic flux, and the local strength of magnetism in a material is measured by its magnetization. The Bohr‑Van Leeuwen theorem showed that classical physics is unable to account for magnetic phenomena, which depend on the quantum mechanical description of atoms.
Hainish
[1856—43]
Red/Blue?
The Mule
ENTANGLED
Psychohist
Each atom’s electrons have magnetic moments due to their spin, and in ferromagnetic materials, unpaired electron spins tend to align in the same direction. Because of Hund’s rules and the Pauli exclusion principle, certain atoms have net magnetic moments, and the exchange interaction between neighboring atoms’ magnetic dipoles causes them to align spontaneously, resulting in spontaneous magnetization of domains. Ferromagnetic materials are divided into tiny regions called magnetic domains, within which the spins are aligned. In an unmagnetized state the domains point in different directions so their magnetic fields cancel, but an external magnetic field causes domain reorientation and growth, leading to net magnetization. Magnetic anisotropy, such as magnetocrystalline anisotropy and shape anisotropy, influences how spins align and affects hysteresis behavior. Domain walls separate regions of different magnetization direction and can be altered by external fields, producing phenomena such as the Barkhausen effect, a series of discrete magnetization changes. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned.
Each atom’s electrons have magnetic moments due to their spin, and in ferromagnetic materials, unpaired electron spins tend to align in the same direction. Because of Hund’s rules and the Pauli exclusion principle, certain atoms have net magnetic moments, and the exchange interaction between neighboring atoms’ magnetic dipoles causes them to align spontaneously, resulting in spontaneous magnetization of domains. Ferromagnetic materials are divided into tiny regions called magnetic domains, within which the spins are aligned. In an unmagnetized state the domains point in different directions so their magnetic fields cancel, but an external magnetic field causes domain reorientation and growth, leading to net magnetization. Magnetic anisotropy, such as magnetocrystalline anisotropy and shape anisotropy, influences how spins align and affects hysteresis behavior. Domain walls separate regions of different magnetization direction and can be altered by external fields, producing phenomena such as the Barkhausen effect, a series of discrete magnetization changes. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned.
Each atom’s electrons have magnetic moments due to their spin, and in ferromagnetic materials, unpaired electron spins tend to align in the same direction. Because of Hund’s rules and the Pauli exclusion principle, certain atoms have net magnetic moments, and the exchange interaction between neighboring atoms’ magnetic dipoles causes them to align spontaneously, resulting in spontaneous magnetization of domains. Ferromagnetic materials are divided into tiny regions called magnetic domains, within which the spins are aligned. In an unmagnetized state the domains point in different directions so their magnetic fields cancel, but an external magnetic field causes domain reorientation and growth, leading to net magnetization. Magnetic anisotropy, such as magnetocrystalline anisotropy and shape anisotropy, influences how spins align and affects hysteresis behavior. Domain walls separate regions of different magnetization direction and can be altered by external fields, producing phenomena such as the Barkhausen effect, a series of discrete magnetization changes. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned.
Each atom’s electrons have magnetic moments due to their spin, and in ferromagnetic materials, unpaired electron spins tend to align in the same direction. Because of Hund’s rules and the Pauli exclusion principle, certain atoms have net magnetic moments, and the exchange interaction between neighboring atoms’ magnetic dipoles causes them to align spontaneously, resulting in spontaneous magnetization of domains. Ferromagnetic materials are divided into tiny regions called magnetic domains, within which the spins are aligned. In an unmagnetized state the domains point in different directions so their magnetic fields cancel, but an external magnetic field causes domain reorientation and growth, leading to net magnetization. Magnetic anisotropy, such as magnetocrystalline anisotropy and shape anisotropy, influences how spins align and affects hysteresis behavior. Domain walls separate regions of different magnetization direction and can be altered by external fields, producing phenomena such as the Barkhausen effect, a series of discrete magnetization changes. Ferromagnetic materials can be divided into magnetically soft materials having low coercivity, which do not tend to stay magnetized, and magnetically hard materials having high coercivity, which do tend to remain magnetized once aligned.
Agent S.
Anarres v
Diamond
MORPHEUS
Lagrange
Event Hor.
Angular momentum is a measure of the amount of rotation an object has, taking into account its mass, shape, and speed. It is a vector quantity, which means it has both magnitude and direction. In classical mechanics, angular momentum is defined as the cross product of the position vector and the linear momentum vector. For a rigid body rotating about a fixed axis, it can also be expressed as the product of the moment of inertia and angular velocity. Conservation of angular momentum states that if no external torque acts on a system, its total angular momentum remains constant. This principle explains why a figure skater spins faster when pulling their arms in, why planets maintain stable orbits, and how celestial bodies interact. Angular momentum is also crucial in engineering and technology, appearing in turbines, gyroscopes, rotating machinery, and spacecraft dynamics. In quantum mechanics, angular momentum is quantized and manifests as orbital and intrinsic spin components of particles. Electron spin, nuclear spin, and photon angular momentum obey discrete rules, unlike continuous classical rotation. Conservation laws govern interactions at atomic and subatomic scales, influencing phenomena such as the Zeeman effect, spectral transitions, and selection rules. Angular momentum links classical and quantum descriptions, providing a unifying principle for the behavior of systems ranging from microscopic particles to macroscopic bodies and celestial objects. Its study is essential in physics, astrophysics, and engineering, shaping our understanding of motion, forces, and energy in the universe.
Angular momentum is a measure of the amount of rotation an object has, taking into account its mass, shape, and speed. It is a vector quantity, which means it has both magnitude and direction. In classical mechanics, angular momentum is defined as the cross product of the position vector and the linear momentum vector. For a rigid body rotating about a fixed axis, it can also be expressed as the product of the moment of inertia and angular velocity. Conservation of angular momentum states that if no external torque acts on a system, its total angular momentum remains constant. This principle explains why a figure skater spins faster when pulling their arms in, why planets maintain stable orbits, and how celestial bodies interact. Angular momentum is also crucial in engineering and technology, appearing in turbines, gyroscopes, rotating machinery, and spacecraft dynamics. In quantum mechanics, angular momentum is quantized and manifests as orbital and intrinsic spin components of particles. Electron spin, nuclear spin, and photon angular momentum obey discrete rules, unlike continuous classical rotation. Conservation laws govern interactions at atomic and subatomic scales, influencing phenomena such as the Zeeman effect, spectral transitions, and selection rules. Angular momentum links classical and quantum descriptions, providing a unifying principle for the behavior of systems ranging from microscopic particles to macroscopic bodies and celestial objects. Its study is essential in physics, astrophysics, and engineering, shaping our understanding of motion, forces, and energy in the universe.
Angular momentum is a measure of the amount of rotation an object has, taking into account its mass, shape, and speed. It is a vector quantity, which means it has both magnitude and direction. In classical mechanics, angular momentum is defined as the cross product of the position vector and the linear momentum vector. For a rigid body rotating about a fixed axis, it can also be expressed as the product of the moment of inertia and angular velocity. Conservation of angular momentum states that if no external torque acts on a system, its total angular momentum remains constant. This principle explains why a figure skater spins faster when pulling their arms in, why planets maintain stable orbits, and how celestial bodies interact. Angular momentum is also crucial in engineering and technology, appearing in turbines, gyroscopes, rotating machinery, and spacecraft dynamics. In quantum mechanics, angular momentum is quantized and manifests as orbital and intrinsic spin components of particles. Electron spin, nuclear spin, and photon angular momentum obey discrete rules, unlike continuous classical rotation. Conservation laws govern interactions at atomic and subatomic scales, influencing phenomena such as the Zeeman effect, spectral transitions, and selection rules. Angular momentum links classical and quantum descriptions, providing a unifying principle for the behavior of systems ranging from microscopic particles to macroscopic bodies and celestial objects. Its study is essential in physics, astrophysics, and engineering, shaping our understanding of motion, forces, and energy in the universe.
Angular momentum is a measure of the amount of rotation an object has, taking into account its mass, shape, and speed. It is a vector quantity, which means it has both magnitude and direction. In classical mechanics, angular momentum is defined as the cross product of the position vector and the linear momentum vector. For a rigid body rotating about a fixed axis, it can also be expressed as the product of the moment of inertia and angular velocity. Conservation of angular momentum states that if no external torque acts on a system, its total angular momentum remains constant. This principle explains why a figure skater spins faster when pulling their arms in, why planets maintain stable orbits, and how celestial bodies interact. Angular momentum is also crucial in engineering and technology, appearing in turbines, gyroscopes, rotating machinery, and spacecraft dynamics. In quantum mechanics, angular momentum is quantized and manifests as orbital and intrinsic spin components of particles. Electron spin, nuclear spin, and photon angular momentum obey discrete rules, unlike continuous classical rotation. Conservation laws govern interactions at atomic and subatomic scales, influencing phenomena such as the Zeeman effect, spectral transitions, and selection rules. Angular momentum links classical and quantum descriptions, providing a unifying principle for the behavior of systems ranging from microscopic particles to macroscopic bodies and celestial objects. Its study is essential in physics, astrophysics, and engineering, shaping our understanding of motion, forces, and energy in the universe.
Polyphase
HDD Plat.
Singular.
SHINJI
Asimov
Bullet T.
Magnemite is an Electric/Steel-type Pokémon known as the Magnet Pokémon. It is composed of a spherical, metallic body with a single large eye and two powerful magnets on its sides. Magnemite generates and manipulates electromagnetic fields to levitate and move, and it can attract or repel metallic objects at will. This Pokémon is capable of emitting strong electric currents and discharging electricity to defend itself or attack opponents. In the Pokémon world, Magnemite is often found near power plants, substations, and areas with high concentrations of electricity, where it absorbs energy to sustain its own. It evolves into Magneton when multiple Magnemite come together, and later can evolve into Magnezone under special conditions involving magnetic fields. Magnemite has abilities such as Magnet Pull, which prevents Steel-type opponents from escaping, and Sturdy, which allows it to survive hits that would normally knock it out. Its behavior is influenced by electromagnetic forces, and it has a habit of floating silently through the air, sometimes forming clusters with other Magnemite. The species has been featured in numerous Pokémon games, animated series episodes, and trading cards, often demonstrating its utility in manipulating metal objects or generating electricity in creative ways. It is known for its unusual combination of mechanical appearance and sentient behavior, highlighting the blend of technology and biology typical of many Electric-type Pokémon. Magnemite has a base experience yield of 89, a catch rate of 190, and is considered part of the Mineral egg group, with a hatch time of 20 cycles. It is generally friendly toward humans and other Pokémon but will attack if threatened, using electric discharges and magnetic force to immobilize opponents. Its small size, around 0.3 meters tall and weighing approximately 6 kilograms, belies its powerful electrical capabilities and strategic potential in battles and environmental interactions.
Magnemite is an Electric/Steel-type Pokémon known as the Magnet Pokémon. It is composed of a spherical, metallic body with a single large eye and two powerful magnets on its sides. Magnemite generates and manipulates electromagnetic fields to levitate and move, and it can attract or repel metallic objects at will. This Pokémon is capable of emitting strong electric currents and discharging electricity to defend itself or attack opponents. In the Pokémon world, Magnemite is often found near power plants, substations, and areas with high concentrations of electricity, where it absorbs energy to sustain its own. It evolves into Magneton when multiple Magnemite come together, and later can evolve into Magnezone under special conditions involving magnetic fields. Magnemite has abilities such as Magnet Pull, which prevents Steel-type opponents from escaping, and Sturdy, which allows it to survive hits that would normally knock it out. Its behavior is influenced by electromagnetic forces, and it has a habit of floating silently through the air, sometimes forming clusters with other Magnemite. The species has been featured in numerous Pokémon games, animated series episodes, and trading cards, often demonstrating its utility in manipulating metal objects or generating electricity in creative ways. It is known for its unusual combination of mechanical appearance and sentient behavior, highlighting the blend of technology and biology typical of many Electric-type Pokémon. Magnemite has a base experience yield of 89, a catch rate of 190, and is considered part of the Mineral egg group, with a hatch time of 20 cycles. It is generally friendly toward humans and other Pokémon but will attack if threatened, using electric discharges and magnetic force to immobilize opponents. Its small size, around 0.3 meters tall and weighing approximately 6 kilograms, belies its powerful electrical capabilities and strategic potential in battles and environmental interactions.
Magnemite is an Electric/Steel-type Pokémon known as the Magnet Pokémon. It is composed of a spherical, metallic body with a single large eye and two powerful magnets on its sides. Magnemite generates and manipulates electromagnetic fields to levitate and move, and it can attract or repel metallic objects at will. This Pokémon is capable of emitting strong electric currents and discharging electricity to defend itself or attack opponents. In the Pokémon world, Magnemite is often found near power plants, substations, and areas with high concentrations of electricity, where it absorbs energy to sustain its own. It evolves into Magneton when multiple Magnemite come together, and later can evolve into Magnezone under special conditions involving magnetic fields. Magnemite has abilities such as Magnet Pull, which prevents Steel-type opponents from escaping, and Sturdy, which allows it to survive hits that would normally knock it out. Its behavior is influenced by electromagnetic forces, and it has a habit of floating silently through the air, sometimes forming clusters with other Magnemite. The species has been featured in numerous Pokémon games, animated series episodes, and trading cards, often demonstrating its utility in manipulating metal objects or generating electricity in creative ways. It is known for its unusual combination of mechanical appearance and sentient behavior, highlighting the blend of technology and biology typical of many Electric-type Pokémon. Magnemite has a base experience yield of 89, a catch rate of 190, and is considered part of the Mineral egg group, with a hatch time of 20 cycles. It is generally friendly toward humans and other Pokémon but will attack if threatened, using electric discharges and magnetic force to immobilize opponents. Its small size, around 0.3 meters tall and weighing approximately 6 kilograms, belies its powerful electrical capabilities and strategic potential in battles and environmental interactions.
Magnemite is an Electric/Steel-type Pokémon known as the Magnet Pokémon. It is composed of a spherical, metallic body with a single large eye and two powerful magnets on its sides. Magnemite generates and manipulates electromagnetic fields to levitate and move, and it can attract or repel metallic objects at will. This Pokémon is capable of emitting strong electric currents and discharging electricity to defend itself or attack opponents. In the Pokémon world, Magnemite is often found near power plants, substations, and areas with high concentrations of electricity, where it absorbs energy to sustain its own. It evolves into Magneton when multiple Magnemite come together, and later can evolve into Magnezone under special conditions involving magnetic fields. Magnemite has abilities such as Magnet Pull, which prevents Steel-type opponents from escaping, and Sturdy, which allows it to survive hits that would normally knock it out. Its behavior is influenced by electromagnetic forces, and it has a habit of floating silently through the air, sometimes forming clusters with other Magnemite. The species has been featured in numerous Pokémon games, animated series episodes, and trading cards, often demonstrating its utility in manipulating metal objects or generating electricity in creative ways. It is known for its unusual combination of mechanical appearance and sentient behavior, highlighting the blend of technology and biology typical of many Electric-type Pokémon. Magnemite has a base experience yield of 89, a catch rate of 190, and is considered part of the Mineral egg group, with a hatch time of 20 cycles. It is generally friendly toward humans and other Pokémon but will attack if threatened, using electric discharges and magnetic force to immobilize opponents. Its small size, around 0.3 meters tall and weighing approximately 6 kilograms, belies its powerful electrical capabilities and strategic potential in battles and environmental interactions.
Hari S.
COIL volt
Wachowski
Dispos.
TERMINUS
Angel
Minitel, officially known as TELETEL, was an interactive videotex online service accessible through telephone lines that became the world’s first and most successful mass‑market online service prior to the World Wide Web. It was developed in Cesson‑Sévéigné, Brittany, by the government‑owned France Télécom and launched experimentally on 15 July 1980 in Saint‑Malo before being extended to other regions later that year. The service was commercially introduced throughout France in 1982 by the PTT, the French administration of postal services and telecommunications, and offered a wide range of functionalities including online purchases, train ticket reservations, business information services, telephone directory searches, mailbox management, and chat functions similar to those now supported by the Web. Minitel terminals were distributed freely to households, which encouraged rapid adoption, and by the 1980s millions of users were connected monthly. The system allowed both individuals and businesses to create and access information services, providing an early model for electronic commerce and online communication. Users could interact in real time, and the service supported applications from news and banking to messaging and dating services. Despite the later emergence of the Internet, Minitel remained in widespread use, reporting 10 million monthly connections as late as February 2009, and it was officially discontinued on 30 June 2012 after more than three decades of operation.
Minitel, officially known as TELETEL, was an interactive videotex online service accessible through telephone lines that became the world’s first and most successful mass‑market online service prior to the World Wide Web. It was developed in Cesson‑Sévéigné, Brittany, by the government‑owned France Télécom and launched experimentally on 15 July 1980 in Saint‑Malo before being extended to other regions later that year. The service was commercially introduced throughout France in 1982 by the PTT, the French administration of postal services and telecommunications, and offered a wide range of functionalities including online purchases, train ticket reservations, business information services, telephone directory searches, mailbox management, and chat functions similar to those now supported by the Web. Minitel terminals were distributed freely to households, which encouraged rapid adoption, and by the 1980s millions of users were connected monthly. The system allowed both individuals and businesses to create and access information services, providing an early model for electronic commerce and online communication. Users could interact in real time, and the service supported applications from news and banking to messaging and dating services. Despite the later emergence of the Internet, Minitel remained in widespread use, reporting 10 million monthly connections as late as February 2009, and it was officially discontinued on 30 June 2012 after more than three decades of operation.
Minitel, officially known as TELETEL, was an interactive videotex online service accessible through telephone lines that became the world’s first and most successful mass‑market online service prior to the World Wide Web. It was developed in Cesson‑Sévéigné, Brittany, by the government‑owned France Télécom and launched experimentally on 15 July 1980 in Saint‑Malo before being extended to other regions later that year. The service was commercially introduced throughout France in 1982 by the PTT, the French administration of postal services and telecommunications, and offered a wide range of functionalities including online purchases, train ticket reservations, business information services, telephone directory searches, mailbox management, and chat functions similar to those now supported by the Web. Minitel terminals were distributed freely to households, which encouraged rapid adoption, and by the 1980s millions of users were connected monthly. The system allowed both individuals and businesses to create and access information services, providing an early model for electronic commerce and online communication. Users could interact in real time, and the service supported applications from news and banking to messaging and dating services. Despite the later emergence of the Internet, Minitel remained in widespread use, reporting 10 million monthly connections as late as February 2009, and it was officially discontinued on 30 June 2012 after more than three decades of operation.
Minitel, officially known as TELETEL, was an interactive videotex online service accessible through telephone lines that became the world’s first and most successful mass‑market online service prior to the World Wide Web. It was developed in Cesson‑Sévéigné, Brittany, by the government‑owned France Télécom and launched experimentally on 15 July 1980 in Saint‑Malo before being extended to other regions later that year. The service was commercially introduced throughout France in 1982 by the PTT, the French administration of postal services and telecommunications, and offered a wide range of functionalities including online purchases, train ticket reservations, business information services, telephone directory searches, mailbox management, and chat functions similar to those now supported by the Web. Minitel terminals were distributed freely to households, which encouraged rapid adoption, and by the 1980s millions of users were connected monthly. The system allowed both individuals and businesses to create and access information services, providing an early model for electronic commerce and online communication. Users could interact in real time, and the service supported applications from news and banking to messaging and dating services. Despite the later emergence of the Internet, Minitel remained in widespread use, reporting 10 million monthly connections as late as February 2009, and it was officially discontinued on 30 June 2012 after more than three decades of operation.
Ferrimag.
Isaac A.
Keanu Neo
NERV pilot
Tesla C.
Magnetic?
The most popular service of the Minitel was the Annuaire Electronique, the electronic telephone directory, which garnered significant usage with approximately half of the network’s calls directed to it in 1985. In May of that year, a nationwide white pages directory covering all 24 million telephone subscribers was introduced, accessible through a simple number, and later became accessible via shortened prefixes following changes to the French numbering system. Companies had the option to include supplementary information, effectively creating rudimentary company webpages within the Minitel network. Advertisement space within the directory was managed commercially, and “Minitel Websites” appeared for major brands and stores, containing dozens or even hundreds of pages of content. The system’s architecture allowed for a wide variety of services to be hosted and accessed, and the popular directory service remained in use even as overall network usage declined toward the end of the system’s life. The impact of Minitel on the development of digital services in France has been the subject of significant discussion, partly because Minitel offered more than a thousand services, many of which anticipated functions that later became common on the Internet. In 1986, French university students organized a national strike using Minitel, showcasing an early instance of digital communication tools being employed for political objectives.
The most popular service of the Minitel was the Annuaire Electronique, the electronic telephone directory, which garnered significant usage with approximately half of the network’s calls directed to it in 1985. In May of that year, a nationwide white pages directory covering all 24 million telephone subscribers was introduced, accessible through a simple number, and later became accessible via shortened prefixes following changes to the French numbering system. Companies had the option to include supplementary information, effectively creating rudimentary company webpages within the Minitel network. Advertisement space within the directory was managed commercially, and “Minitel Websites” appeared for major brands and stores, containing dozens or even hundreds of pages of content. The system’s architecture allowed for a wide variety of services to be hosted and accessed, and the popular directory service remained in use even as overall network usage declined toward the end of the system’s life. The impact of Minitel on the development of digital services in France has been the subject of significant discussion, partly because Minitel offered more than a thousand services, many of which anticipated functions that later became common on the Internet. In 1986, French university students organized a national strike using Minitel, showcasing an early instance of digital communication tools being employed for political objectives.
The most popular service of the Minitel was the Annuaire Electronique, the electronic telephone directory, which garnered significant usage with approximately half of the network’s calls directed to it in 1985. In May of that year, a nationwide white pages directory covering all 24 million telephone subscribers was introduced, accessible through a simple number, and later became accessible via shortened prefixes following changes to the French numbering system. Companies had the option to include supplementary information, effectively creating rudimentary company webpages within the Minitel network. Advertisement space within the directory was managed commercially, and “Minitel Websites” appeared for major brands and stores, containing dozens or even hundreds of pages of content. The system’s architecture allowed for a wide variety of services to be hosted and accessed, and the popular directory service remained in use even as overall network usage declined toward the end of the system’s life. The impact of Minitel on the development of digital services in France has been the subject of significant discussion, partly because Minitel offered more than a thousand services, many of which anticipated functions that later became common on the Internet. In 1986, French university students organized a national strike using Minitel, showcasing an early instance of digital communication tools being employed for political objectives.
The most popular service of the Minitel was the Annuaire Electronique, the electronic telephone directory, which garnered significant usage with approximately half of the network’s calls directed to it in 1985. In May of that year, a nationwide white pages directory covering all 24 million telephone subscribers was introduced, accessible through a simple number, and later became accessible via shortened prefixes following changes to the French numbering system. Companies had the option to include supplementary information, effectively creating rudimentary company webpages within the Minitel network. Advertisement space within the directory was managed commercially, and “Minitel Websites” appeared for major brands and stores, containing dozens or even hundreds of pages of content. The system’s architecture allowed for a wide variety of services to be hosted and accessed, and the popular directory service remained in use even as overall network usage declined toward the end of the system’s life. The impact of Minitel on the development of digital services in France has been the subject of significant discussion, partly because Minitel offered more than a thousand services, many of which anticipated functions that later became common on the Internet. In 1986, French university students organized a national strike using Minitel, showcasing an early instance of digital communication tools being employed for political objectives.
DOMAIN
(1929—19)
3‑body
Human farm
Rei Ayana
WEBFETCH
Neon Genesis Evangelion is a Japanese manga series written and illustrated by Yoshiyuki Sadamoto and published by Kadokawa Shoten. It began serialization in the magazine Monthly Shōnen Ace in December 1994 and later moved to Young Ace, with its run concluding in June 2013, spanning fourteen volumes composed of multiple chapters. The manga was originally released before the anime adaptation of the same name, with the intention of generating interest in the upcoming television series. Sadamoto, who served as the original character designer for the anime, based the manga on the story and characters from the show but developed it with his own creative vision and pacing, resulting in notable differences between the two mediums. The series is set in a post‑apocalyptic world where humanity faces the threat of enigmatic beings known as Angels, and the central narrative follows a group of adolescent pilots tasked with defending humanity by piloting giant biomechanical weapons called Evangelions, created by the secretive organization NERV. Neon Genesis Evangelion blends elements of apocalyptic drama, psychological exploration, and mecha action, examining themes of identity, trauma, interpersonal conflict, and the human condition through its characters’ struggles amid catastrophic stakes. The manga’s protagonist, Shinji Ikari, is a fourteen‑year‑old boy whose father, Gendo Ikari, commander of NERV, coerces him into piloting an Evangelion unit to confront the Angels threatening Earth.
Neon Genesis Evangelion is a Japanese manga series written and illustrated by Yoshiyuki Sadamoto and published by Kadokawa Shoten. It began serialization in the magazine Monthly Shōnen Ace in December 1994 and later moved to Young Ace, with its run concluding in June 2013, spanning fourteen volumes composed of multiple chapters. The manga was originally released before the anime adaptation of the same name, with the intention of generating interest in the upcoming television series. Sadamoto, who served as the original character designer for the anime, based the manga on the story and characters from the show but developed it with his own creative vision and pacing, resulting in notable differences between the two mediums. The series is set in a post‑apocalyptic world where humanity faces the threat of enigmatic beings known as Angels, and the central narrative follows a group of adolescent pilots tasked with defending humanity by piloting giant biomechanical weapons called Evangelions, created by the secretive organization NERV. Neon Genesis Evangelion blends elements of apocalyptic drama, psychological exploration, and mecha action, examining themes of identity, trauma, interpersonal conflict, and the human condition through its characters’ struggles amid catastrophic stakes. The manga’s protagonist, Shinji Ikari, is a fourteen‑year‑old boy whose father, Gendo Ikari, commander of NERV, coerces him into piloting an Evangelion unit to confront the Angels threatening Earth.
Neon Genesis Evangelion is a Japanese manga series written and illustrated by Yoshiyuki Sadamoto and published by Kadokawa Shoten. It began serialization in the magazine Monthly Shōnen Ace in December 1994 and later moved to Young Ace, with its run concluding in June 2013, spanning fourteen volumes composed of multiple chapters. The manga was originally released before the anime adaptation of the same name, with the intention of generating interest in the upcoming television series. Sadamoto, who served as the original character designer for the anime, based the manga on the story and characters from the show but developed it with his own creative vision and pacing, resulting in notable differences between the two mediums. The series is set in a post‑apocalyptic world where humanity faces the threat of enigmatic beings known as Angels, and the central narrative follows a group of adolescent pilots tasked with defending humanity by piloting giant biomechanical weapons called Evangelions, created by the secretive organization NERV. Neon Genesis Evangelion blends elements of apocalyptic drama, psychological exploration, and mecha action, examining themes of identity, trauma, interpersonal conflict, and the human condition through its characters’ struggles amid catastrophic stakes. The manga’s protagonist, Shinji Ikari, is a fourteen‑year‑old boy whose father, Gendo Ikari, commander of NERV, coerces him into piloting an Evangelion unit to confront the Angels threatening Earth.
Neon Genesis Evangelion is a Japanese manga series written and illustrated by Yoshiyuki Sadamoto and published by Kadokawa Shoten. It began serialization in the magazine Monthly Shōnen Ace in December 1994 and later moved to Young Ace, with its run concluding in June 2013, spanning fourteen volumes composed of multiple chapters. The manga was originally released before the anime adaptation of the same name, with the intention of generating interest in the upcoming television series. Sadamoto, who served as the original character designer for the anime, based the manga on the story and characters from the show but developed it with his own creative vision and pacing, resulting in notable differences between the two mediums. The series is set in a post‑apocalyptic world where humanity faces the threat of enigmatic beings known as Angels, and the central narrative follows a group of adolescent pilots tasked with defending humanity by piloting giant biomechanical weapons called Evangelions, created by the secretive organization NERV. Neon Genesis Evangelion blends elements of apocalyptic drama, psychological exploration, and mecha action, examining themes of identity, trauma, interpersonal conflict, and the human condition through its characters’ struggles amid catastrophic stakes. The manga’s protagonist, Shinji Ikari, is a fourteen‑year‑old boy whose father, Gendo Ikari, commander of NERV, coerces him into piloting an Evangelion unit to confront the Angels threatening Earth.
Tetrava.
Capsule95
June 2012
Month. Ace
NICKEL Fe
Coercivity
While the core premise resembles that of the anime, the manga diverges in several plot points, such as the omission of certain Angels, variations in character development, and differences in key battles and outcomes. Shinji, Rei Ayanami, Asuka Langley Soryu, and other characters exhibit distinct personalities and relationships that reflect Sadamoto’s interpretation of the story. In contrast to the anime’s portrayal, some events unfold at altered times, and the emotional dynamics between characters evolve in unique ways, including more explicit exploration of their inner thoughts and motivations. The manga’s irregular publication schedule was influenced by Sadamoto’s involvement in various other projects, resulting in hiatuses and delays between volumes, though the narrative ultimately reached its conclusion over nearly two decades, offering fans a definitive iteration of the Evangelion saga. The popularity of Neon Genesis Evangelion as a manga extended beyond Japan, with English language releases published by Viz Media in a variety of formats, including standard volumes and collector editions. The series achieved significant commercial success, with the first ten volumes selling millions of copies and several volumes topping manga sales charts. In addition to the main adaptation, the Evangelion franchise inspired numerous spin‑off manga and related works that explore alternate themes or reimagine characters in different settings, reflecting the broad cultural impact of the original series. Neon Genesis Evangelion remains a seminal work in both manga and anime communities, recognized for its mature storytelling, psychological depth, and enduring influence on the mecha genre and popular culture worldwide.
While the core premise resembles that of the anime, the manga diverges in several plot points, such as the omission of certain Angels, variations in character development, and differences in key battles and outcomes. Shinji, Rei Ayanami, Asuka Langley Soryu, and other characters exhibit distinct personalities and relationships that reflect Sadamoto’s interpretation of the story. In contrast to the anime’s portrayal, some events unfold at altered times, and the emotional dynamics between characters evolve in unique ways, including more explicit exploration of their inner thoughts and motivations. The manga’s irregular publication schedule was influenced by Sadamoto’s involvement in various other projects, resulting in hiatuses and delays between volumes, though the narrative ultimately reached its conclusion over nearly two decades, offering fans a definitive iteration of the Evangelion saga. The popularity of Neon Genesis Evangelion as a manga extended beyond Japan, with English language releases published by Viz Media in a variety of formats, including standard volumes and collector editions. The series achieved significant commercial success, with the first ten volumes selling millions of copies and several volumes topping manga sales charts. In addition to the main adaptation, the Evangelion franchise inspired numerous spin‑off manga and related works that explore alternate themes or reimagine characters in different settings, reflecting the broad cultural impact of the original series. Neon Genesis Evangelion remains a seminal work in both manga and anime communities, recognized for its mature storytelling, psychological depth, and enduring influence on the mecha genre and popular culture worldwide.
While the core premise resembles that of the anime, the manga diverges in several plot points, such as the omission of certain Angels, variations in character development, and differences in key battles and outcomes. Shinji, Rei Ayanami, Asuka Langley Soryu, and other characters exhibit distinct personalities and relationships that reflect Sadamoto’s interpretation of the story. In contrast to the anime’s portrayal, some events unfold at altered times, and the emotional dynamics between characters evolve in unique ways, including more explicit exploration of their inner thoughts and motivations. The manga’s irregular publication schedule was influenced by Sadamoto’s involvement in various other projects, resulting in hiatuses and delays between volumes, though the narrative ultimately reached its conclusion over nearly two decades, offering fans a definitive iteration of the Evangelion saga. The popularity of Neon Genesis Evangelion as a manga extended beyond Japan, with English language releases published by Viz Media in a variety of formats, including standard volumes and collector editions. The series achieved significant commercial success, with the first ten volumes selling millions of copies and several volumes topping manga sales charts. In addition to the main adaptation, the Evangelion franchise inspired numerous spin‑off manga and related works that explore alternate themes or reimagine characters in different settings, reflecting the broad cultural impact of the original series. Neon Genesis Evangelion remains a seminal work in both manga and anime communities, recognized for its mature storytelling, psychological depth, and enduring influence on the mecha genre and popular culture worldwide.
While the core premise resembles that of the anime, the manga diverges in several plot points, such as the omission of certain Angels, variations in character development, and differences in key battles and outcomes. Shinji, Rei Ayanami, Asuka Langley Soryu, and other characters exhibit distinct personalities and relationships that reflect Sadamoto’s interpretation of the story. In contrast to the anime’s portrayal, some events unfold at altered times, and the emotional dynamics between characters evolve in unique ways, including more explicit exploration of their inner thoughts and motivations. The manga’s irregular publication schedule was influenced by Sadamoto’s involvement in various other projects, resulting in hiatuses and delays between volumes, though the narrative ultimately reached its conclusion over nearly two decades, offering fans a definitive iteration of the Evangelion saga. The popularity of Neon Genesis Evangelion as a manga extended beyond Japan, with English language releases published by Viz Media in a variety of formats, including standard volumes and collector editions. The series achieved significant commercial success, with the first ten volumes selling millions of copies and several volumes topping manga sales charts. In addition to the main adaptation, the Evangelion franchise inspired numerous spin‑off manga and related works that explore alternate themes or reimagine characters in different settings, reflecting the broad cultural impact of the original series. Neon Genesis Evangelion remains a seminal work in both manga and anime communities, recognized for its mature storytelling, psychological depth, and enduring influence on the mecha genre and popular culture worldwide.
Spin align
GRAPHITE
Skater→
GYROSCOPE
Zeeman fx
Magneton
In physics, specifically classical mechanics, the three-body problem concerns determining the motions of three point masses interacting through gravity when their initial positions and velocities are known. Unlike the two-body problem, which has a closed-form solution, the three-body problem has no general analytical solution. The resulting system is highly sensitive to initial conditions, making its behavior largely chaotic and predictable only through numerical approximations. Historically, the problem first studied in detail involved the Earth, the Moon, and the Sun, with modern extensions considering any set of three interacting bodies in space. Mathematically, the three-body problem can be expressed using Newton’s laws of motion and universal gravitation, resulting in a set of coupled differential equations that are extremely difficult to solve analytically. Various special cases allow simplifications, such as the restricted three-body problem, where one body is assumed to have negligible mass, or configurations with symmetry that permit periodic solutions. Despite its complexity, the problem has been central to the development of celestial mechanics, informing the study of planetary motion, orbital stability, tidal forces, and chaotic dynamics. Over centuries, mathematicians such as Euler, Lagrange, and Poincaré contributed significant insights, including the identification of Lagrangian points where a small object can maintain a stable position relative to two larger bodies.
In physics, specifically classical mechanics, the three-body problem concerns determining the motions of three point masses interacting through gravity when their initial positions and velocities are known. Unlike the two-body problem, which has a closed-form solution, the three-body problem has no general analytical solution. The resulting system is highly sensitive to initial conditions, making its behavior largely chaotic and predictable only through numerical approximations. Historically, the problem first studied in detail involved the Earth, the Moon, and the Sun, with modern extensions considering any set of three interacting bodies in space. Mathematically, the three-body problem can be expressed using Newton’s laws of motion and universal gravitation, resulting in a set of coupled differential equations that are extremely difficult to solve analytically. Various special cases allow simplifications, such as the restricted three-body problem, where one body is assumed to have negligible mass, or configurations with symmetry that permit periodic solutions. Despite its complexity, the problem has been central to the development of celestial mechanics, informing the study of planetary motion, orbital stability, tidal forces, and chaotic dynamics. Over centuries, mathematicians such as Euler, Lagrange, and Poincaré contributed significant insights, including the identification of Lagrangian points where a small object can maintain a stable position relative to two larger bodies.
In physics, specifically classical mechanics, the three-body problem concerns determining the motions of three point masses interacting through gravity when their initial positions and velocities are known. Unlike the two-body problem, which has a closed-form solution, the three-body problem has no general analytical solution. The resulting system is highly sensitive to initial conditions, making its behavior largely chaotic and predictable only through numerical approximations. Historically, the problem first studied in detail involved the Earth, the Moon, and the Sun, with modern extensions considering any set of three interacting bodies in space. Mathematically, the three-body problem can be expressed using Newton’s laws of motion and universal gravitation, resulting in a set of coupled differential equations that are extremely difficult to solve analytically. Various special cases allow simplifications, such as the restricted three-body problem, where one body is assumed to have negligible mass, or configurations with symmetry that permit periodic solutions. Despite its complexity, the problem has been central to the development of celestial mechanics, informing the study of planetary motion, orbital stability, tidal forces, and chaotic dynamics. Over centuries, mathematicians such as Euler, Lagrange, and Poincaré contributed significant insights, including the identification of Lagrangian points where a small object can maintain a stable position relative to two larger bodies.
In physics, specifically classical mechanics, the three-body problem concerns determining the motions of three point masses interacting through gravity when their initial positions and velocities are known. Unlike the two-body problem, which has a closed-form solution, the three-body problem has no general analytical solution. The resulting system is highly sensitive to initial conditions, making its behavior largely chaotic and predictable only through numerical approximations. Historically, the problem first studied in detail involved the Earth, the Moon, and the Sun, with modern extensions considering any set of three interacting bodies in space. Mathematically, the three-body problem can be expressed using Newton’s laws of motion and universal gravitation, resulting in a set of coupled differential equations that are extremely difficult to solve analytically. Various special cases allow simplifications, such as the restricted three-body problem, where one body is assumed to have negligible mass, or configurations with symmetry that permit periodic solutions. Despite its complexity, the problem has been central to the development of celestial mechanics, informing the study of planetary motion, orbital stability, tidal forces, and chaotic dynamics. Over centuries, mathematicians such as Euler, Lagrange, and Poincaré contributed significant insights, including the identification of Lagrangian points where a small object can maintain a stable position relative to two larger bodies.
Catch 190
Steel-type
6 kg light
TELETEL
(July 1980)
PTT France
A hard disk drive is a data storage device used for storing and retrieving digital information using one or more rigid rapidly rotating disks coated with magnetic material. It is a type of non-volatile storage, retaining data even when powered off, and has been a primary storage medium for computers for several decades. HDDs consist of several key components, including spinning platters, read/write heads, actuators, and control circuitry. The platters store data magnetically in concentric tracks, and the heads access data by floating above the platter surfaces on a thin cushion of air generated by the disk rotation. Modern HDDs typically use multiple platters stacked vertically to increase storage capacity. The movement of the read/write heads is controlled by precision actuators, allowing access to billions of individual bits of data at high speed. Data is organized into sectors and tracks, and file systems coordinate how this data is stored, retrieved, and maintained. Hard drives connect to computers via interfaces such as SATA, SAS, or previously IDE/ATA, enabling communication between the storage medium and the system. Since their inception in the 1950s, HDDs have evolved from large, low-capacity, mechanically complex devices to compact, high-capacity, highly reliable storage solutions. Improvements in magnetic recording, platter density, and actuator precision have allowed drives to achieve terabytes of storage in a standard 3.5-inch or 2.5-inch form factor.
A hard disk drive is a data storage device used for storing and retrieving digital information using one or more rigid rapidly rotating disks coated with magnetic material. It is a type of non-volatile storage, retaining data even when powered off, and has been a primary storage medium for computers for several decades. HDDs consist of several key components, including spinning platters, read/write heads, actuators, and control circuitry. The platters store data magnetically in concentric tracks, and the heads access data by floating above the platter surfaces on a thin cushion of air generated by the disk rotation. Modern HDDs typically use multiple platters stacked vertically to increase storage capacity. The movement of the read/write heads is controlled by precision actuators, allowing access to billions of individual bits of data at high speed. Data is organized into sectors and tracks, and file systems coordinate how this data is stored, retrieved, and maintained. Hard drives connect to computers via interfaces such as SATA, SAS, or previously IDE/ATA, enabling communication between the storage medium and the system. Since their inception in the 1950s, HDDs have evolved from large, low-capacity, mechanically complex devices to compact, high-capacity, highly reliable storage solutions. Improvements in magnetic recording, platter density, and actuator precision have allowed drives to achieve terabytes of storage in a standard 3.5-inch or 2.5-inch form factor.
A hard disk drive is a data storage device used for storing and retrieving digital information using one or more rigid rapidly rotating disks coated with magnetic material. It is a type of non-volatile storage, retaining data even when powered off, and has been a primary storage medium for computers for several decades. HDDs consist of several key components, including spinning platters, read/write heads, actuators, and control circuitry. The platters store data magnetically in concentric tracks, and the heads access data by floating above the platter surfaces on a thin cushion of air generated by the disk rotation. Modern HDDs typically use multiple platters stacked vertically to increase storage capacity. The movement of the read/write heads is controlled by precision actuators, allowing access to billions of individual bits of data at high speed. Data is organized into sectors and tracks, and file systems coordinate how this data is stored, retrieved, and maintained. Hard drives connect to computers via interfaces such as SATA, SAS, or previously IDE/ATA, enabling communication between the storage medium and the system. Since their inception in the 1950s, HDDs have evolved from large, low-capacity, mechanically complex devices to compact, high-capacity, highly reliable storage solutions. Improvements in magnetic recording, platter density, and actuator precision have allowed drives to achieve terabytes of storage in a standard 3.5-inch or 2.5-inch form factor.
A hard disk drive is a data storage device used for storing and retrieving digital information using one or more rigid rapidly rotating disks coated with magnetic material. It is a type of non-volatile storage, retaining data even when powered off, and has been a primary storage medium for computers for several decades. HDDs consist of several key components, including spinning platters, read/write heads, actuators, and control circuitry. The platters store data magnetically in concentric tracks, and the heads access data by floating above the platter surfaces on a thin cushion of air generated by the disk rotation. Modern HDDs typically use multiple platters stacked vertically to increase storage capacity. The movement of the read/write heads is controlled by precision actuators, allowing access to billions of individual bits of data at high speed. Data is organized into sectors and tracks, and file systems coordinate how this data is stored, retrieved, and maintained. Hard drives connect to computers via interfaces such as SATA, SAS, or previously IDE/ATA, enabling communication between the storage medium and the system. Since their inception in the 1950s, HDDs have evolved from large, low-capacity, mechanically complex devices to compact, high-capacity, highly reliable storage solutions. Improvements in magnetic recording, platter density, and actuator precision have allowed drives to achieve terabytes of storage in a standard 3.5-inch or 2.5-inch form factor.
Chat room
10M users
Annuaire E
Gendo Dad
Asuka L.S.
Viz Media
The Dispossessed, subtitled An Ambiguous Utopia, is a 1974 science fiction novel by Ursula K. Le Guin, part of her Hainish Cycle. The novel explores anarchist and utopian themes through the story of Shevek, a brilliant physicist living on Anarres, a harsh desert moon that has been colonized by idealistic revolutionaries seeking to build a society free from oppression and hierarchical structures. Anarres is a world organized around communal ownership, mutual aid, and collective decision-making, in stark contrast to its sister planet Urras, which is wealthy, fertile, and politically stratified with entrenched systems of capitalism and authoritarianism. The narrative alternates between Shevek’s life on Anarres and his experiences on Urras, highlighting the contrasts between societies governed by ideology, material wealth, and social norms. Shevek’s development of a revolutionary theory of physics, which leads to the creation of the ansible, a device enabling instantaneous communication across interstellar distances, serves as both a scientific and symbolic breakthrough, illustrating the interplay between intellectual freedom and societal constraints. The novel examines tensions between individualism and collectivism, the nature of freedom, and the responsibilities of knowledge, questioning the assumptions of what it means to live in a truly free society. Through Shevek’s journey, Le Guin addresses ethical and philosophical questions regarding social organization, the potential of human creativity, and the costs of political and economic inequality.
The Dispossessed, subtitled An Ambiguous Utopia, is a 1974 science fiction novel by Ursula K. Le Guin, part of her Hainish Cycle. The novel explores anarchist and utopian themes through the story of Shevek, a brilliant physicist living on Anarres, a harsh desert moon that has been colonized by idealistic revolutionaries seeking to build a society free from oppression and hierarchical structures. Anarres is a world organized around communal ownership, mutual aid, and collective decision-making, in stark contrast to its sister planet Urras, which is wealthy, fertile, and politically stratified with entrenched systems of capitalism and authoritarianism. The narrative alternates between Shevek’s life on Anarres and his experiences on Urras, highlighting the contrasts between societies governed by ideology, material wealth, and social norms. Shevek’s development of a revolutionary theory of physics, which leads to the creation of the ansible, a device enabling instantaneous communication across interstellar distances, serves as both a scientific and symbolic breakthrough, illustrating the interplay between intellectual freedom and societal constraints. The novel examines tensions between individualism and collectivism, the nature of freedom, and the responsibilities of knowledge, questioning the assumptions of what it means to live in a truly free society. Through Shevek’s journey, Le Guin addresses ethical and philosophical questions regarding social organization, the potential of human creativity, and the costs of political and economic inequality.
The Dispossessed, subtitled An Ambiguous Utopia, is a 1974 science fiction novel by Ursula K. Le Guin, part of her Hainish Cycle. The novel explores anarchist and utopian themes through the story of Shevek, a brilliant physicist living on Anarres, a harsh desert moon that has been colonized by idealistic revolutionaries seeking to build a society free from oppression and hierarchical structures. Anarres is a world organized around communal ownership, mutual aid, and collective decision-making, in stark contrast to its sister planet Urras, which is wealthy, fertile, and politically stratified with entrenched systems of capitalism and authoritarianism. The narrative alternates between Shevek’s life on Anarres and his experiences on Urras, highlighting the contrasts between societies governed by ideology, material wealth, and social norms. Shevek’s development of a revolutionary theory of physics, which leads to the creation of the ansible, a device enabling instantaneous communication across interstellar distances, serves as both a scientific and symbolic breakthrough, illustrating the interplay between intellectual freedom and societal constraints. The novel examines tensions between individualism and collectivism, the nature of freedom, and the responsibilities of knowledge, questioning the assumptions of what it means to live in a truly free society. Through Shevek’s journey, Le Guin addresses ethical and philosophical questions regarding social organization, the potential of human creativity, and the costs of political and economic inequality.
The Dispossessed, subtitled An Ambiguous Utopia, is a 1974 science fiction novel by Ursula K. Le Guin, part of her Hainish Cycle. The novel explores anarchist and utopian themes through the story of Shevek, a brilliant physicist living on Anarres, a harsh desert moon that has been colonized by idealistic revolutionaries seeking to build a society free from oppression and hierarchical structures. Anarres is a world organized around communal ownership, mutual aid, and collective decision-making, in stark contrast to its sister planet Urras, which is wealthy, fertile, and politically stratified with entrenched systems of capitalism and authoritarianism. The narrative alternates between Shevek’s life on Anarres and his experiences on Urras, highlighting the contrasts between societies governed by ideology, material wealth, and social norms. Shevek’s development of a revolutionary theory of physics, which leads to the creation of the ansible, a device enabling instantaneous communication across interstellar distances, serves as both a scientific and symbolic breakthrough, illustrating the interplay between intellectual freedom and societal constraints. The novel examines tensions between individualism and collectivism, the nature of freedom, and the responsibilities of knowledge, questioning the assumptions of what it means to live in a truly free society. Through Shevek’s journey, Le Guin addresses ethical and philosophical questions regarding social organization, the potential of human creativity, and the costs of political and economic inequality.
Mecha war
Euler solv
Poincaré
LAGRANGE
Actuator
SATA drive
A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape its pull. The boundary of this region is called the event horizon, which marks the point of no return. Black holes are predicted by the equations of general relativity, first formulated by Albert Einstein, and arise when massive stars collapse under their own gravity at the end of their life cycles. The core of a black hole, known as the singularity, contains infinite density where classical physics breaks down and the effects of quantum gravity are expected to dominate. Black holes can vary in size from stellar-mass, formed by individual stars, to supermassive, found at the centers of galaxies, and potentially intermediate-mass black holes formed by mergers of smaller black holes. They can grow by accreting gas, dust, and other stars, often forming an accretion disk that emits tremendous amounts of radiation as material spirals inward. Black holes can also produce relativistic jets, where particles are accelerated along magnetic field lines at near-light speed. Observational evidence for black holes includes the motion of stars around invisible massive objects, gravitational lensing of light, X-ray emissions from accreting matter, and direct imaging of the event horizon shadow using very long baseline interferometry. The detection of gravitational waves from colliding black holes by observatories such as LIGO and Virgo has confirmed the existence of stellar-mass binary black hole systems.
A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape its pull. The boundary of this region is called the event horizon, which marks the point of no return. Black holes are predicted by the equations of general relativity, first formulated by Albert Einstein, and arise when massive stars collapse under their own gravity at the end of their life cycles. The core of a black hole, known as the singularity, contains infinite density where classical physics breaks down and the effects of quantum gravity are expected to dominate. Black holes can vary in size from stellar-mass, formed by individual stars, to supermassive, found at the centers of galaxies, and potentially intermediate-mass black holes formed by mergers of smaller black holes. They can grow by accreting gas, dust, and other stars, often forming an accretion disk that emits tremendous amounts of radiation as material spirals inward. Black holes can also produce relativistic jets, where particles are accelerated along magnetic field lines at near-light speed. Observational evidence for black holes includes the motion of stars around invisible massive objects, gravitational lensing of light, X-ray emissions from accreting matter, and direct imaging of the event horizon shadow using very long baseline interferometry. The detection of gravitational waves from colliding black holes by observatories such as LIGO and Virgo has confirmed the existence of stellar-mass binary black hole systems.
A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape its pull. The boundary of this region is called the event horizon, which marks the point of no return. Black holes are predicted by the equations of general relativity, first formulated by Albert Einstein, and arise when massive stars collapse under their own gravity at the end of their life cycles. The core of a black hole, known as the singularity, contains infinite density where classical physics breaks down and the effects of quantum gravity are expected to dominate. Black holes can vary in size from stellar-mass, formed by individual stars, to supermassive, found at the centers of galaxies, and potentially intermediate-mass black holes formed by mergers of smaller black holes. They can grow by accreting gas, dust, and other stars, often forming an accretion disk that emits tremendous amounts of radiation as material spirals inward. Black holes can also produce relativistic jets, where particles are accelerated along magnetic field lines at near-light speed. Observational evidence for black holes includes the motion of stars around invisible massive objects, gravitational lensing of light, X-ray emissions from accreting matter, and direct imaging of the event horizon shadow using very long baseline interferometry. The detection of gravitational waves from colliding black holes by observatories such as LIGO and Virgo has confirmed the existence of stellar-mass binary black hole systems.
A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape its pull. The boundary of this region is called the event horizon, which marks the point of no return. Black holes are predicted by the equations of general relativity, first formulated by Albert Einstein, and arise when massive stars collapse under their own gravity at the end of their life cycles. The core of a black hole, known as the singularity, contains infinite density where classical physics breaks down and the effects of quantum gravity are expected to dominate. Black holes can vary in size from stellar-mass, formed by individual stars, to supermassive, found at the centers of galaxies, and potentially intermediate-mass black holes formed by mergers of smaller black holes. They can grow by accreting gas, dust, and other stars, often forming an accretion disk that emits tremendous amounts of radiation as material spirals inward. Black holes can also produce relativistic jets, where particles are accelerated along magnetic field lines at near-light speed. Observational evidence for black holes includes the motion of stars around invisible massive objects, gravitational lensing of light, X-ray emissions from accreting matter, and direct imaging of the event horizon shadow using very long baseline interferometry. The detection of gravitational waves from colliding black holes by observatories such as LIGO and Virgo has confirmed the existence of stellar-mass binary black hole systems.
Platter++
Sector bit
IDE/ATA
Einstein
Accretion
LIGO wave
Earth’s magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth’s inner core out into space where it interacts with the solar wind. It is generated by electric currents due to the motion of convection currents of molten iron and nickel in Earth’s outer core, a natural geodynamo process driven by heat escaping from the core. At the surface, the field approximates that of a magnetic dipole tilted at an angle of about eleven degrees with respect to Earth’s rotational axis, as if a giant bar magnet were oriented through the center of the planet. Because opposite magnetic poles attract, the north end of a compass needle points toward the South magnetic pole of Earth’s field, and the south end points toward the North magnetic pole as conventionally defined. The field changes continuously over time, varying in strength and direction with both location and time, and influences navigation, animal migration, and protects the planet from charged particles from space by deflecting the solar wind. The magnetic poles are not fixed; they wander across the surface, and the north magnetic pole has been observed migrating from northern Canada toward Siberia in recent decades due to dynamic flows in the outer core where liquid iron generates electrical currents and influences the field.
Earth’s magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth’s inner core out into space where it interacts with the solar wind. It is generated by electric currents due to the motion of convection currents of molten iron and nickel in Earth’s outer core, a natural geodynamo process driven by heat escaping from the core. At the surface, the field approximates that of a magnetic dipole tilted at an angle of about eleven degrees with respect to Earth’s rotational axis, as if a giant bar magnet were oriented through the center of the planet. Because opposite magnetic poles attract, the north end of a compass needle points toward the South magnetic pole of Earth’s field, and the south end points toward the North magnetic pole as conventionally defined. The field changes continuously over time, varying in strength and direction with both location and time, and influences navigation, animal migration, and protects the planet from charged particles from space by deflecting the solar wind. The magnetic poles are not fixed; they wander across the surface, and the north magnetic pole has been observed migrating from northern Canada toward Siberia in recent decades due to dynamic flows in the outer core where liquid iron generates electrical currents and influences the field.
Earth’s magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth’s inner core out into space where it interacts with the solar wind. It is generated by electric currents due to the motion of convection currents of molten iron and nickel in Earth’s outer core, a natural geodynamo process driven by heat escaping from the core. At the surface, the field approximates that of a magnetic dipole tilted at an angle of about eleven degrees with respect to Earth’s rotational axis, as if a giant bar magnet were oriented through the center of the planet. Because opposite magnetic poles attract, the north end of a compass needle points toward the South magnetic pole of Earth’s field, and the south end points toward the North magnetic pole as conventionally defined. The field changes continuously over time, varying in strength and direction with both location and time, and influences navigation, animal migration, and protects the planet from charged particles from space by deflecting the solar wind. The magnetic poles are not fixed; they wander across the surface, and the north magnetic pole has been observed migrating from northern Canada toward Siberia in recent decades due to dynamic flows in the outer core where liquid iron generates electrical currents and influences the field.
Earth’s magnetic field, also known as the geomagnetic field, is the magnetic field that extends from Earth’s inner core out into space where it interacts with the solar wind. It is generated by electric currents due to the motion of convection currents of molten iron and nickel in Earth’s outer core, a natural geodynamo process driven by heat escaping from the core. At the surface, the field approximates that of a magnetic dipole tilted at an angle of about eleven degrees with respect to Earth’s rotational axis, as if a giant bar magnet were oriented through the center of the planet. Because opposite magnetic poles attract, the north end of a compass needle points toward the South magnetic pole of Earth’s field, and the south end points toward the North magnetic pole as conventionally defined. The field changes continuously over time, varying in strength and direction with both location and time, and influences navigation, animal migration, and protects the planet from charged particles from space by deflecting the solar wind. The magnetic poles are not fixed; they wander across the surface, and the north magnetic pole has been observed migrating from northern Canada toward Siberia in recent decades due to dynamic flows in the outer core where liquid iron generates electrical currents and influences the field.
X-ray glow
Hari math
30,000 yrs
Dark age
The Empire
Prelude to
One of the most striking features of Earth’s magnetic field is that it does not remain constant over geological timescales. Throughout Earth’s history, the magnetic field has periodically reversed its polarity, meaning that the positions of magnetic north and magnetic south are interchanged. These geomagnetic reversals occur irregularly, with evidence from geological records showing at least one hundred eighty-three reversals in the last eighty-three million years. During a reversal, the main dipolar component of the field weakens and may even become complex, with multiple poles existing at different locations, before eventually stabilizing with opposite polarity. These periods of normal and reverse polarity are called chrons, and the sequence of reversals can be observed in the remanent magnetization of volcanic and sedimentary rocks that record the direction of the field as they cool or are deposited. The most recent major reversal, the Brunhes–Matuyama reversal, occurred approximately seven hundred eighty thousand years ago, and related excursions such as the Laschamp event represent brief departures from the dominant polarity that are not permanent reversals but reflect temporary instability in the geodynamo.
One of the most striking features of Earth’s magnetic field is that it does not remain constant over geological timescales. Throughout Earth’s history, the magnetic field has periodically reversed its polarity, meaning that the positions of magnetic north and magnetic south are interchanged. These geomagnetic reversals occur irregularly, with evidence from geological records showing at least one hundred eighty-three reversals in the last eighty-three million years. During a reversal, the main dipolar component of the field weakens and may even become complex, with multiple poles existing at different locations, before eventually stabilizing with opposite polarity. These periods of normal and reverse polarity are called chrons, and the sequence of reversals can be observed in the remanent magnetization of volcanic and sedimentary rocks that record the direction of the field as they cool or are deposited. The most recent major reversal, the Brunhes–Matuyama reversal, occurred approximately seven hundred eighty thousand years ago, and related excursions such as the Laschamp event represent brief departures from the dominant polarity that are not permanent reversals but reflect temporary instability in the geodynamo.
One of the most striking features of Earth’s magnetic field is that it does not remain constant over geological timescales. Throughout Earth’s history, the magnetic field has periodically reversed its polarity, meaning that the positions of magnetic north and magnetic south are interchanged. These geomagnetic reversals occur irregularly, with evidence from geological records showing at least one hundred eighty-three reversals in the last eighty-three million years. During a reversal, the main dipolar component of the field weakens and may even become complex, with multiple poles existing at different locations, before eventually stabilizing with opposite polarity. These periods of normal and reverse polarity are called chrons, and the sequence of reversals can be observed in the remanent magnetization of volcanic and sedimentary rocks that record the direction of the field as they cool or are deposited. The most recent major reversal, the Brunhes–Matuyama reversal, occurred approximately seven hundred eighty thousand years ago, and related excursions such as the Laschamp event represent brief departures from the dominant polarity that are not permanent reversals but reflect temporary instability in the geodynamo.
One of the most striking features of Earth’s magnetic field is that it does not remain constant over geological timescales. Throughout Earth’s history, the magnetic field has periodically reversed its polarity, meaning that the positions of magnetic north and magnetic south are interchanged. These geomagnetic reversals occur irregularly, with evidence from geological records showing at least one hundred eighty-three reversals in the last eighty-three million years. During a reversal, the main dipolar component of the field weakens and may even become complex, with multiple poles existing at different locations, before eventually stabilizing with opposite polarity. These periods of normal and reverse polarity are called chrons, and the sequence of reversals can be observed in the remanent magnetization of volcanic and sedimentary rocks that record the direction of the field as they cool or are deposited. The most recent major reversal, the Brunhes–Matuyama reversal, occurred approximately seven hundred eighty thousand years ago, and related excursions such as the Laschamp event represent brief departures from the dominant polarity that are not permanent reversals but reflect temporary instability in the geodynamo.
Gibbon
Terminus°
Isotope14
Steel prod
Graphene
Nano fiber
The process of geomagnetic reversal is not instantaneous; it unfolds over hundreds to thousands of years as the dynamo action in the outer core evolves. During transitions, which may take from around two thousand to twenty-two thousand years at a given location, the magnetic field strength often diminishes, allowing a greater flux of cosmic and solar radiation to reach Earth’s surface and near-Earth space. Geological evidence such as magnetic striping on the ocean floor, recorded as new basalt cools and preserves the direction of the magnetic field, provides a timeline for these reversals and has been instrumental in confirming the theory of seafloor spreading. Because the dynamo has no inherent preference for a specific polarity, when a reversal completes, the magnetic field can settle into either orientation. Reversals are random with no apparent periodicity, occurring as often as every ten thousand years or as infrequently as tens of millions of years. The ongoing study of Earth’s magnetic field, its secular variation, and long-term polarity changes remains crucial for understanding geophysical processes, planetary protection, paleomagnetism, and the history of the planet’s interior dynamics, offering insight into how the geodynamo that sustains the magnetic field has operated over billions of years.
The process of geomagnetic reversal is not instantaneous; it unfolds over hundreds to thousands of years as the dynamo action in the outer core evolves. During transitions, which may take from around two thousand to twenty-two thousand years at a given location, the magnetic field strength often diminishes, allowing a greater flux of cosmic and solar radiation to reach Earth’s surface and near-Earth space. Geological evidence such as magnetic striping on the ocean floor, recorded as new basalt cools and preserves the direction of the magnetic field, provides a timeline for these reversals and has been instrumental in confirming the theory of seafloor spreading. Because the dynamo has no inherent preference for a specific polarity, when a reversal completes, the magnetic field can settle into either orientation. Reversals are random with no apparent periodicity, occurring as often as every ten thousand years or as infrequently as tens of millions of years. The ongoing study of Earth’s magnetic field, its secular variation, and long-term polarity changes remains crucial for understanding geophysical processes, planetary protection, paleomagnetism, and the history of the planet’s interior dynamics, offering insight into how the geodynamo that sustains the magnetic field has operated over billions of years.
The process of geomagnetic reversal is not instantaneous; it unfolds over hundreds to thousands of years as the dynamo action in the outer core evolves. During transitions, which may take from around two thousand to twenty-two thousand years at a given location, the magnetic field strength often diminishes, allowing a greater flux of cosmic and solar radiation to reach Earth’s surface and near-Earth space. Geological evidence such as magnetic striping on the ocean floor, recorded as new basalt cools and preserves the direction of the magnetic field, provides a timeline for these reversals and has been instrumental in confirming the theory of seafloor spreading. Because the dynamo has no inherent preference for a specific polarity, when a reversal completes, the magnetic field can settle into either orientation. Reversals are random with no apparent periodicity, occurring as often as every ten thousand years or as infrequently as tens of millions of years. The ongoing study of Earth’s magnetic field, its secular variation, and long-term polarity changes remains crucial for understanding geophysical processes, planetary protection, paleomagnetism, and the history of the planet’s interior dynamics, offering insight into how the geodynamo that sustains the magnetic field has operated over billions of years.
The process of geomagnetic reversal is not instantaneous; it unfolds over hundreds to thousands of years as the dynamo action in the outer core evolves. During transitions, which may take from around two thousand to twenty-two thousand years at a given location, the magnetic field strength often diminishes, allowing a greater flux of cosmic and solar radiation to reach Earth’s surface and near-Earth space. Geological evidence such as magnetic striping on the ocean floor, recorded as new basalt cools and preserves the direction of the magnetic field, provides a timeline for these reversals and has been instrumental in confirming the theory of seafloor spreading. Because the dynamo has no inherent preference for a specific polarity, when a reversal completes, the magnetic field can settle into either orientation. Reversals are random with no apparent periodicity, occurring as often as every ten thousand years or as infrequently as tens of millions of years. The ongoing study of Earth’s magnetic field, its secular variation, and long-term polarity changes remains crucial for understanding geophysical processes, planetary protection, paleomagnetism, and the history of the planet’s interior dynamics, offering insight into how the geodynamo that sustains the magnetic field has operated over billions of years.
Lubricant
Revere box
Detroit '00
Helium TX
Blue pill
Red pill→
The Foundation series is a science fiction novel series written by American author Isaac Asimov that has become one of the most influential works in the genre. The stories were first published as interconnected short stories and novellas in the 1940s and early 1950s before being compiled into three books that make up the original Foundation trilogy. These novels, Foundation, Foundation and Empire, and Second Foundation, explore the rise and fall of a galactic empire set tens of thousands of years in the future, where humanity has spread across the Milky Way and formed a vast interstellar civilization. The central premise revolves around a new science called psychohistory, devised by the brilliant mathematician Hari Seldon, which combines history, sociology, and statistical mathematics to predict the large‑scale behavior of societies. Although psychohistory cannot determine the actions of individuals, it can forecast the broad movements of populations over long periods, allowing Seldon to foresee the imminent decline of the Galactic Empire and the onset of a dark age that he believes will last thirty thousand years unless action is taken. To mitigate this projected collapse, he establishes the Foundation, a repository of scientific knowledge on a remote planet called Terminus, designed to preserve human knowledge and shorten the period of barbarism to just one thousand years.
The Foundation series is a science fiction novel series written by American author Isaac Asimov that has become one of the most influential works in the genre. The stories were first published as interconnected short stories and novellas in the 1940s and early 1950s before being compiled into three books that make up the original Foundation trilogy. These novels, Foundation, Foundation and Empire, and Second Foundation, explore the rise and fall of a galactic empire set tens of thousands of years in the future, where humanity has spread across the Milky Way and formed a vast interstellar civilization. The central premise revolves around a new science called psychohistory, devised by the brilliant mathematician Hari Seldon, which combines history, sociology, and statistical mathematics to predict the large‑scale behavior of societies. Although psychohistory cannot determine the actions of individuals, it can forecast the broad movements of populations over long periods, allowing Seldon to foresee the imminent decline of the Galactic Empire and the onset of a dark age that he believes will last thirty thousand years unless action is taken. To mitigate this projected collapse, he establishes the Foundation, a repository of scientific knowledge on a remote planet called Terminus, designed to preserve human knowledge and shorten the period of barbarism to just one thousand years.
The Foundation series is a science fiction novel series written by American author Isaac Asimov that has become one of the most influential works in the genre. The stories were first published as interconnected short stories and novellas in the 1940s and early 1950s before being compiled into three books that make up the original Foundation trilogy. These novels, Foundation, Foundation and Empire, and Second Foundation, explore the rise and fall of a galactic empire set tens of thousands of years in the future, where humanity has spread across the Milky Way and formed a vast interstellar civilization. The central premise revolves around a new science called psychohistory, devised by the brilliant mathematician Hari Seldon, which combines history, sociology, and statistical mathematics to predict the large‑scale behavior of societies. Although psychohistory cannot determine the actions of individuals, it can forecast the broad movements of populations over long periods, allowing Seldon to foresee the imminent decline of the Galactic Empire and the onset of a dark age that he believes will last thirty thousand years unless action is taken. To mitigate this projected collapse, he establishes the Foundation, a repository of scientific knowledge on a remote planet called Terminus, designed to preserve human knowledge and shorten the period of barbarism to just one thousand years.
The Foundation series is a science fiction novel series written by American author Isaac Asimov that has become one of the most influential works in the genre. The stories were first published as interconnected short stories and novellas in the 1940s and early 1950s before being compiled into three books that make up the original Foundation trilogy. These novels, Foundation, Foundation and Empire, and Second Foundation, explore the rise and fall of a galactic empire set tens of thousands of years in the future, where humanity has spread across the Milky Way and formed a vast interstellar civilization. The central premise revolves around a new science called psychohistory, devised by the brilliant mathematician Hari Seldon, which combines history, sociology, and statistical mathematics to predict the large‑scale behavior of societies. Although psychohistory cannot determine the actions of individuals, it can forecast the broad movements of populations over long periods, allowing Seldon to foresee the imminent decline of the Galactic Empire and the onset of a dark age that he believes will last thirty thousand years unless action is taken. To mitigate this projected collapse, he establishes the Foundation, a repository of scientific knowledge on a remote planet called Terminus, designed to preserve human knowledge and shorten the period of barbarism to just one thousand years.
Morpheus?
Trinity
Wire-fu
Bullet FX
$400M box
Bennett93
The early books in the series follow the struggles of the Foundation as it deals with crises predicted by Seldon’s psychohistorical models, and prerecorded messages from Seldon provide guidance at pivotal moments throughout generations. In Foundation and Empire, the Foundation must contend with both the lingering influence of the declining Galactic Empire and the unexpected rise of a powerful mutant known only as the Mule, whose existence was not anticipated by Seldon’s equations. Second Foundation focuses on the search for the secretive organization established by Seldon to guide the development of mental sciences and preserve the original plan when it is threatened by forces who seek to derail it. Later novels expand the series beyond the original trilogy, including Foundation’s Edge and Foundation and Earth, which continue the narrative centuries after the initial establishment of the Foundation and explore further philosophical and existential questions about the fate of humanity in the galaxy. Asimov also wrote prequels such as Prelude to Foundation and Forward the Foundation, which trace the early life of Hari Seldon and the development of psychohistory itself, providing deeper context for his motivations and the unfolding of his grand plan. The Foundation novels were inspired in part by Edward Gibbon’s historical work The History of the Decline and Fall of the Roman Empire, reflecting a thematic concern with cycles of rise, decay, and renewal in civilizations.
The early books in the series follow the struggles of the Foundation as it deals with crises predicted by Seldon’s psychohistorical models, and prerecorded messages from Seldon provide guidance at pivotal moments throughout generations. In Foundation and Empire, the Foundation must contend with both the lingering influence of the declining Galactic Empire and the unexpected rise of a powerful mutant known only as the Mule, whose existence was not anticipated by Seldon’s equations. Second Foundation focuses on the search for the secretive organization established by Seldon to guide the development of mental sciences and preserve the original plan when it is threatened by forces who seek to derail it. Later novels expand the series beyond the original trilogy, including Foundation’s Edge and Foundation and Earth, which continue the narrative centuries after the initial establishment of the Foundation and explore further philosophical and existential questions about the fate of humanity in the galaxy. Asimov also wrote prequels such as Prelude to Foundation and Forward the Foundation, which trace the early life of Hari Seldon and the development of psychohistory itself, providing deeper context for his motivations and the unfolding of his grand plan. The Foundation novels were inspired in part by Edward Gibbon’s historical work The History of the Decline and Fall of the Roman Empire, reflecting a thematic concern with cycles of rise, decay, and renewal in civilizations.
The early books in the series follow the struggles of the Foundation as it deals with crises predicted by Seldon’s psychohistorical models, and prerecorded messages from Seldon provide guidance at pivotal moments throughout generations. In Foundation and Empire, the Foundation must contend with both the lingering influence of the declining Galactic Empire and the unexpected rise of a powerful mutant known only as the Mule, whose existence was not anticipated by Seldon’s equations. Second Foundation focuses on the search for the secretive organization established by Seldon to guide the development of mental sciences and preserve the original plan when it is threatened by forces who seek to derail it. Later novels expand the series beyond the original trilogy, including Foundation’s Edge and Foundation and Earth, which continue the narrative centuries after the initial establishment of the Foundation and explore further philosophical and existential questions about the fate of humanity in the galaxy. Asimov also wrote prequels such as Prelude to Foundation and Forward the Foundation, which trace the early life of Hari Seldon and the development of psychohistory itself, providing deeper context for his motivations and the unfolding of his grand plan. The Foundation novels were inspired in part by Edward Gibbon’s historical work The History of the Decline and Fall of the Roman Empire, reflecting a thematic concern with cycles of rise, decay, and renewal in civilizations.
The early books in the series follow the struggles of the Foundation as it deals with crises predicted by Seldon’s psychohistorical models, and prerecorded messages from Seldon provide guidance at pivotal moments throughout generations. In Foundation and Empire, the Foundation must contend with both the lingering influence of the declining Galactic Empire and the unexpected rise of a powerful mutant known only as the Mule, whose existence was not anticipated by Seldon’s equations. Second Foundation focuses on the search for the secretive organization established by Seldon to guide the development of mental sciences and preserve the original plan when it is threatened by forces who seek to derail it. Later novels expand the series beyond the original trilogy, including Foundation’s Edge and Foundation and Earth, which continue the narrative centuries after the initial establishment of the Foundation and explore further philosophical and existential questions about the fate of humanity in the galaxy. Asimov also wrote prequels such as Prelude to Foundation and Forward the Foundation, which trace the early life of Hari Seldon and the development of psychohistory itself, providing deeper context for his motivations and the unfolding of his grand plan. The Foundation novels were inspired in part by Edward Gibbon’s historical work The History of the Decline and Fall of the Roman Empire, reflecting a thematic concern with cycles of rise, decay, and renewal in civilizations.
Photon '97
Satellite
Berkeley
Kroeber
Taoist
Anarchist
Carbon is a chemical element with symbol C and atomic number 6, essential to all known life forms. It is a nonmetallic element capable of forming a wide variety of compounds, more than any other element, due to its tetravalent nature, which allows it to form four covalent bonds with other atoms. Carbon exists in several allotropes, including diamond, graphite, graphene, fullerenes, and amorphous carbon, each exhibiting distinct physical properties. Diamond is a crystalline form with a three-dimensional network of strong covalent bonds, resulting in extreme hardness and high thermal conductivity. Graphite, on the other hand, consists of planar layers of carbon atoms arranged in hexagonal lattices, which can slide over one another, making it an excellent lubricant and conductor of electricity. Carbon atoms can also form long chains and rings, which are the basis of organic chemistry, creating the molecular backbone for thousands of biological molecules such as proteins, lipids, nucleic acids, and carbohydrates. Carbon occurs naturally in the atmosphere as carbon dioxide, in fossil fuels such as coal, petroleum, and natural gas, and in carbonate minerals in rocks. The carbon cycle describes the continuous exchange of carbon among the biosphere, geosphere, hydrosphere, and atmosphere, regulating Earth’s climate over geological time scales. Carbon isotopes, including carbon-12, carbon-13, and the radioactive carbon-14, are used in various scientific fields for tracing biological processes and dating archaeological artifacts. Industrially, carbon is used in steel production, filtration systems, batteries, and advanced materials like carbon fibers and nanomaterials.
Carbon is a chemical element with symbol C and atomic number 6, essential to all known life forms. It is a nonmetallic element capable of forming a wide variety of compounds, more than any other element, due to its tetravalent nature, which allows it to form four covalent bonds with other atoms. Carbon exists in several allotropes, including diamond, graphite, graphene, fullerenes, and amorphous carbon, each exhibiting distinct physical properties. Diamond is a crystalline form with a three-dimensional network of strong covalent bonds, resulting in extreme hardness and high thermal conductivity. Graphite, on the other hand, consists of planar layers of carbon atoms arranged in hexagonal lattices, which can slide over one another, making it an excellent lubricant and conductor of electricity. Carbon atoms can also form long chains and rings, which are the basis of organic chemistry, creating the molecular backbone for thousands of biological molecules such as proteins, lipids, nucleic acids, and carbohydrates. Carbon occurs naturally in the atmosphere as carbon dioxide, in fossil fuels such as coal, petroleum, and natural gas, and in carbonate minerals in rocks. The carbon cycle describes the continuous exchange of carbon among the biosphere, geosphere, hydrosphere, and atmosphere, regulating Earth’s climate over geological time scales. Carbon isotopes, including carbon-12, carbon-13, and the radioactive carbon-14, are used in various scientific fields for tracing biological processes and dating archaeological artifacts. Industrially, carbon is used in steel production, filtration systems, batteries, and advanced materials like carbon fibers and nanomaterials.
Carbon is a chemical element with symbol C and atomic number 6, essential to all known life forms. It is a nonmetallic element capable of forming a wide variety of compounds, more than any other element, due to its tetravalent nature, which allows it to form four covalent bonds with other atoms. Carbon exists in several allotropes, including diamond, graphite, graphene, fullerenes, and amorphous carbon, each exhibiting distinct physical properties. Diamond is a crystalline form with a three-dimensional network of strong covalent bonds, resulting in extreme hardness and high thermal conductivity. Graphite, on the other hand, consists of planar layers of carbon atoms arranged in hexagonal lattices, which can slide over one another, making it an excellent lubricant and conductor of electricity. Carbon atoms can also form long chains and rings, which are the basis of organic chemistry, creating the molecular backbone for thousands of biological molecules such as proteins, lipids, nucleic acids, and carbohydrates. Carbon occurs naturally in the atmosphere as carbon dioxide, in fossil fuels such as coal, petroleum, and natural gas, and in carbonate minerals in rocks. The carbon cycle describes the continuous exchange of carbon among the biosphere, geosphere, hydrosphere, and atmosphere, regulating Earth’s climate over geological time scales. Carbon isotopes, including carbon-12, carbon-13, and the radioactive carbon-14, are used in various scientific fields for tracing biological processes and dating archaeological artifacts. Industrially, carbon is used in steel production, filtration systems, batteries, and advanced materials like carbon fibers and nanomaterials.
Carbon is a chemical element with symbol C and atomic number 6, essential to all known life forms. It is a nonmetallic element capable of forming a wide variety of compounds, more than any other element, due to its tetravalent nature, which allows it to form four covalent bonds with other atoms. Carbon exists in several allotropes, including diamond, graphite, graphene, fullerenes, and amorphous carbon, each exhibiting distinct physical properties. Diamond is a crystalline form with a three-dimensional network of strong covalent bonds, resulting in extreme hardness and high thermal conductivity. Graphite, on the other hand, consists of planar layers of carbon atoms arranged in hexagonal lattices, which can slide over one another, making it an excellent lubricant and conductor of electricity. Carbon atoms can also form long chains and rings, which are the basis of organic chemistry, creating the molecular backbone for thousands of biological molecules such as proteins, lipids, nucleic acids, and carbohydrates. Carbon occurs naturally in the atmosphere as carbon dioxide, in fossil fuels such as coal, petroleum, and natural gas, and in carbonate minerals in rocks. The carbon cycle describes the continuous exchange of carbon among the biosphere, geosphere, hydrosphere, and atmosphere, regulating Earth’s climate over geological time scales. Carbon isotopes, including carbon-12, carbon-13, and the radioactive carbon-14, are used in various scientific fields for tracing biological processes and dating archaeological artifacts. Industrially, carbon is used in steel production, filtration systems, batteries, and advanced materials like carbon fibers and nanomaterials.
ANSIBLE
Urras rich
Shevek
Mutual aid
Physics++
RIGID body
A time capsule is a historic cache of goods or information, usually intended as a deliberate method of communication with future people and to help future archaeologists, anthropologists, or historians. The practice of preserving everyday artifacts and messages for future generations, although related to the preservation of holy relics for millennia, became a more organized and ceremonial practice in modern times. Time capsules are often created and buried during events such as world fairs, cornerstone layings for buildings, anniversaries, or other commemorative ceremonies. Early examples include artifacts placed in a hollow copper weathervane atop Faneuil Hall in Boston in the 18th century, as well as documents hidden within statues or religious objects in Europe dating back to the 1700s. In the United States, the oldest known time capsule is from 1795, attributed to figures like Samuel Adams and Paul Revere, which was placed within the cornerstone of the Massachusetts State House and has been opened and reinstalled multiple times, providing insight into the political and cultural context of its era. In the 20th century, the use of time capsules expanded widely, with the practice being embraced by institutions, governments, and individuals alike. Notable examples include the Detroit Century Box, containing letters and objects to be opened after several decades, and the Helium Centennial Time Columns Monument in Amarillo, Texas, which holds multiple stainless steel capsules intended to be opened after 25, 50, 100, and even 1,000 years.
A time capsule is a historic cache of goods or information, usually intended as a deliberate method of communication with future people and to help future archaeologists, anthropologists, or historians. The practice of preserving everyday artifacts and messages for future generations, although related to the preservation of holy relics for millennia, became a more organized and ceremonial practice in modern times. Time capsules are often created and buried during events such as world fairs, cornerstone layings for buildings, anniversaries, or other commemorative ceremonies. Early examples include artifacts placed in a hollow copper weathervane atop Faneuil Hall in Boston in the 18th century, as well as documents hidden within statues or religious objects in Europe dating back to the 1700s. In the United States, the oldest known time capsule is from 1795, attributed to figures like Samuel Adams and Paul Revere, which was placed within the cornerstone of the Massachusetts State House and has been opened and reinstalled multiple times, providing insight into the political and cultural context of its era. In the 20th century, the use of time capsules expanded widely, with the practice being embraced by institutions, governments, and individuals alike. Notable examples include the Detroit Century Box, containing letters and objects to be opened after several decades, and the Helium Centennial Time Columns Monument in Amarillo, Texas, which holds multiple stainless steel capsules intended to be opened after 25, 50, 100, and even 1,000 years.
A time capsule is a historic cache of goods or information, usually intended as a deliberate method of communication with future people and to help future archaeologists, anthropologists, or historians. The practice of preserving everyday artifacts and messages for future generations, although related to the preservation of holy relics for millennia, became a more organized and ceremonial practice in modern times. Time capsules are often created and buried during events such as world fairs, cornerstone layings for buildings, anniversaries, or other commemorative ceremonies. Early examples include artifacts placed in a hollow copper weathervane atop Faneuil Hall in Boston in the 18th century, as well as documents hidden within statues or religious objects in Europe dating back to the 1700s. In the United States, the oldest known time capsule is from 1795, attributed to figures like Samuel Adams and Paul Revere, which was placed within the cornerstone of the Massachusetts State House and has been opened and reinstalled multiple times, providing insight into the political and cultural context of its era. In the 20th century, the use of time capsules expanded widely, with the practice being embraced by institutions, governments, and individuals alike. Notable examples include the Detroit Century Box, containing letters and objects to be opened after several decades, and the Helium Centennial Time Columns Monument in Amarillo, Texas, which holds multiple stainless steel capsules intended to be opened after 25, 50, 100, and even 1,000 years.
A time capsule is a historic cache of goods or information, usually intended as a deliberate method of communication with future people and to help future archaeologists, anthropologists, or historians. The practice of preserving everyday artifacts and messages for future generations, although related to the preservation of holy relics for millennia, became a more organized and ceremonial practice in modern times. Time capsules are often created and buried during events such as world fairs, cornerstone layings for buildings, anniversaries, or other commemorative ceremonies. Early examples include artifacts placed in a hollow copper weathervane atop Faneuil Hall in Boston in the 18th century, as well as documents hidden within statues or religious objects in Europe dating back to the 1700s. In the United States, the oldest known time capsule is from 1795, attributed to figures like Samuel Adams and Paul Revere, which was placed within the cornerstone of the Massachusetts State House and has been opened and reinstalled multiple times, providing insight into the political and cultural context of its era. In the 20th century, the use of time capsules expanded widely, with the practice being embraced by institutions, governments, and individuals alike. Notable examples include the Detroit Century Box, containing letters and objects to be opened after several decades, and the Helium Centennial Time Columns Monument in Amarillo, Texas, which holds multiple stainless steel capsules intended to be opened after 25, 50, 100, and even 1,000 years.
Orbit (law)
Torque = 0
Intrinsic*
QUANTIZED
Spectral→
Celestial
The Matrix is a 1999 science fiction action film written and directed by the Wachowskis and starring Keanu Reeves, Laurence Fishburne, Carrie‑Anne Moss, and Hugo Weaving. The story is set in a dystopian future where humanity is unknowingly trapped inside a simulated reality called the Matrix, created by sentient machines to pacify and subdue the human population while using their bodies as an energy source. The protagonist, Thomas Anderson, leads a double life as a software developer by day and a hacker known as Neo by night. Neo becomes aware that there is something fundamentally wrong with reality and is drawn into a rebellion against the machines after being contacted by Trinity and Morpheus, leaders of a group of free humans who have escaped the simulation. Morpheus believes Neo is “the One,” a prophesied savior who will liberate humanity. Neo is offered a choice between taking a blue pill, which returns him to the ignorance of everyday life, or a red pill, which reveals the truth about the Matrix and begins his journey into the real world. Upon choosing the red pill, Neo awakens in a devastated world dominated by machines and learns about the brutal truth of human existence under their control. As Neo trains with Morpheus and the resistance, he confronts Agents, powerful sentient programs that enforce order within the Matrix and can adapt to human strategies.
The Matrix is a 1999 science fiction action film written and directed by the Wachowskis and starring Keanu Reeves, Laurence Fishburne, Carrie‑Anne Moss, and Hugo Weaving. The story is set in a dystopian future where humanity is unknowingly trapped inside a simulated reality called the Matrix, created by sentient machines to pacify and subdue the human population while using their bodies as an energy source. The protagonist, Thomas Anderson, leads a double life as a software developer by day and a hacker known as Neo by night. Neo becomes aware that there is something fundamentally wrong with reality and is drawn into a rebellion against the machines after being contacted by Trinity and Morpheus, leaders of a group of free humans who have escaped the simulation. Morpheus believes Neo is “the One,” a prophesied savior who will liberate humanity. Neo is offered a choice between taking a blue pill, which returns him to the ignorance of everyday life, or a red pill, which reveals the truth about the Matrix and begins his journey into the real world. Upon choosing the red pill, Neo awakens in a devastated world dominated by machines and learns about the brutal truth of human existence under their control. As Neo trains with Morpheus and the resistance, he confronts Agents, powerful sentient programs that enforce order within the Matrix and can adapt to human strategies.
The Matrix is a 1999 science fiction action film written and directed by the Wachowskis and starring Keanu Reeves, Laurence Fishburne, Carrie‑Anne Moss, and Hugo Weaving. The story is set in a dystopian future where humanity is unknowingly trapped inside a simulated reality called the Matrix, created by sentient machines to pacify and subdue the human population while using their bodies as an energy source. The protagonist, Thomas Anderson, leads a double life as a software developer by day and a hacker known as Neo by night. Neo becomes aware that there is something fundamentally wrong with reality and is drawn into a rebellion against the machines after being contacted by Trinity and Morpheus, leaders of a group of free humans who have escaped the simulation. Morpheus believes Neo is “the One,” a prophesied savior who will liberate humanity. Neo is offered a choice between taking a blue pill, which returns him to the ignorance of everyday life, or a red pill, which reveals the truth about the Matrix and begins his journey into the real world. Upon choosing the red pill, Neo awakens in a devastated world dominated by machines and learns about the brutal truth of human existence under their control. As Neo trains with Morpheus and the resistance, he confronts Agents, powerful sentient programs that enforce order within the Matrix and can adapt to human strategies.
The Matrix is a 1999 science fiction action film written and directed by the Wachowskis and starring Keanu Reeves, Laurence Fishburne, Carrie‑Anne Moss, and Hugo Weaving. The story is set in a dystopian future where humanity is unknowingly trapped inside a simulated reality called the Matrix, created by sentient machines to pacify and subdue the human population while using their bodies as an energy source. The protagonist, Thomas Anderson, leads a double life as a software developer by day and a hacker known as Neo by night. Neo becomes aware that there is something fundamentally wrong with reality and is drawn into a rebellion against the machines after being contacted by Trinity and Morpheus, leaders of a group of free humans who have escaped the simulation. Morpheus believes Neo is “the One,” a prophesied savior who will liberate humanity. Neo is offered a choice between taking a blue pill, which returns him to the ignorance of everyday life, or a red pill, which reveals the truth about the Matrix and begins his journey into the real world. Upon choosing the red pill, Neo awakens in a devastated world dominated by machines and learns about the brutal truth of human existence under their control. As Neo trains with Morpheus and the resistance, he confronts Agents, powerful sentient programs that enforce order within the Matrix and can adapt to human strategies.
Moment: I
Subatomic
Spin rule
MECHANICS
Turbine–Go
Velocity²
The training sequences and action scenes, including martial arts and gunplay, draw heavily on Hong Kong wire‑fu techniques and stylized choreography, contributing to the film’s distinctive aesthetic that blends Western cinema with Eastern influences. One of the most iconic visual effects in the film is “bullet time,” where the simulation appears to slow or freeze while the camera moves dynamically around a scene, creating a dramatic sense of perception beyond normal human limits. The visual style and innovative effects were influential in defining late twentieth‑century action cinema and have been widely imitated across media. The Matrix also integrates philosophical, religious, and cyberpunk themes, exploring ideas about reality, perception, free will, identity, and control, and incorporates influences from mythology, postmodernism, and earlier works of speculative fiction. Upon its release, The Matrix became a major commercial success, grossing over four hundred million dollars worldwide on a budget of approximately sixty‑three million and earning critical acclaim for its storytelling, action sequences, and technical achievements. The film won multiple awards, particularly for its visual effects, editing, and sound, and was selected for preservation in the United States National Film Registry for being culturally, historically, or aesthetically significant.
The training sequences and action scenes, including martial arts and gunplay, draw heavily on Hong Kong wire‑fu techniques and stylized choreography, contributing to the film’s distinctive aesthetic that blends Western cinema with Eastern influences. One of the most iconic visual effects in the film is “bullet time,” where the simulation appears to slow or freeze while the camera moves dynamically around a scene, creating a dramatic sense of perception beyond normal human limits. The visual style and innovative effects were influential in defining late twentieth‑century action cinema and have been widely imitated across media. The Matrix also integrates philosophical, religious, and cyberpunk themes, exploring ideas about reality, perception, free will, identity, and control, and incorporates influences from mythology, postmodernism, and earlier works of speculative fiction. Upon its release, The Matrix became a major commercial success, grossing over four hundred million dollars worldwide on a budget of approximately sixty‑three million and earning critical acclaim for its storytelling, action sequences, and technical achievements. The film won multiple awards, particularly for its visual effects, editing, and sound, and was selected for preservation in the United States National Film Registry for being culturally, historically, or aesthetically significant.
The training sequences and action scenes, including martial arts and gunplay, draw heavily on Hong Kong wire‑fu techniques and stylized choreography, contributing to the film’s distinctive aesthetic that blends Western cinema with Eastern influences. One of the most iconic visual effects in the film is “bullet time,” where the simulation appears to slow or freeze while the camera moves dynamically around a scene, creating a dramatic sense of perception beyond normal human limits. The visual style and innovative effects were influential in defining late twentieth‑century action cinema and have been widely imitated across media. The Matrix also integrates philosophical, religious, and cyberpunk themes, exploring ideas about reality, perception, free will, identity, and control, and incorporates influences from mythology, postmodernism, and earlier works of speculative fiction. Upon its release, The Matrix became a major commercial success, grossing over four hundred million dollars worldwide on a budget of approximately sixty‑three million and earning critical acclaim for its storytelling, action sequences, and technical achievements. The film won multiple awards, particularly for its visual effects, editing, and sound, and was selected for preservation in the United States National Film Registry for being culturally, historically, or aesthetically significant.
The training sequences and action scenes, including martial arts and gunplay, draw heavily on Hong Kong wire‑fu techniques and stylized choreography, contributing to the film’s distinctive aesthetic that blends Western cinema with Eastern influences. One of the most iconic visual effects in the film is “bullet time,” where the simulation appears to slow or freeze while the camera moves dynamically around a scene, creating a dramatic sense of perception beyond normal human limits. The visual style and innovative effects were influential in defining late twentieth‑century action cinema and have been widely imitated across media. The Matrix also integrates philosophical, religious, and cyberpunk themes, exploring ideas about reality, perception, free will, identity, and control, and incorporates influences from mythology, postmodernism, and earlier works of speculative fiction. Upon its release, The Matrix became a major commercial success, grossing over four hundred million dollars worldwide on a budget of approximately sixty‑three million and earning critical acclaim for its storytelling, action sequences, and technical achievements. The film won multiple awards, particularly for its visual effects, editing, and sound, and was selected for preservation in the United States National Film Registry for being culturally, historically, or aesthetically significant.
Basic Latin
A B C D E F G G H I I J J K L M N O P Q Q R R S T U V W X Y Z
a a b c d e f g g h i i j j k l l m n o p q r r s t u v w x y y z
Extended Latin
Á Ă Ǎ Â Ä À Ā Ą Å Ã Æ Ǽ Ć Č Ç Ĉ Ċ Ð Ď Đ É Ĕ Ě Ê Ë Ė È Ē Ę Ə Ğ Ǧ Ĝ Ģ Ġ
Ğ Ǧ Ĝ Ģ Ġ Ħ Ĥ Í Ĭ Î Ï İ Ì Ī Į Ĩ IJ Í Ĭ Î Ï İ Ì Ī Į Ĩ IJ J Ĵ J Ĵ Ķ Ĺ Ľ Ļ Ŀ Ł Ń Ň
Ņ Ñ Ŋ Ó Ŏ Ô Ö Ò Ő Ō Ø Ǿ Õ Œ Þ Q Ŕ Ř Ŗ Ŕ Ř Ŗ Ś Š Ş Ŝ Ș ẞ Ŧ Ť Ţ Ț Ú Ŭ Û
Ü Ù Ű Ū Ų Ů Ũ Ẃ Ŵ Ẅ Ẁ Ý Ŷ Ÿ Ỳ Ź Ž Ż
á ă ǎ â ä à ā ą å ã æ ǽ á ă ǎ â ä à ā ą å ã ć č ç ĉ ċ ð ď đ é ĕ ě ê ë ė è ē
ę ə ğ ǧ ĝ ģ ġ ğ ǧ ĝ ģ ġ ħ ĥ ı í ĭ î ï i ì ī į ĩ ij ı í ĭ î ï i ì ī į ĩ ij ȷ j ĵ ȷ j ĵ ķ ĸ ĺ ľ ļ
ŀ ł ĺ ľ ļ ŀ ł ń ň ņ ñ ŋ ó ŏ ô ö ò ő ō ø ǿ õ œ þ ŕ ř ŗ ŕ ř ŗ ś š ş ŝ ș ß ŧ ť ţ ț ú
ŭ û ü ù ű ū ų ů ũ ẃ ŵ ẅ ẁ ý ŷ ÿ ỳ ý ŷ ÿ ỳ ź ž ż
Ordinals
ª ª º
Figures & currencies
№ 0 1 2 3 4 5 6 7 8 9 0 0 1 2 3 4 5 6 7 8 9 0
0 1 2 3 4 5 6 7 8 9 0 1 2 3 4 5 6 7 8 9
₀ ₁ ₂ ₃ ₄ ₅ ₆ ₇ ₈ ₉ ⁰ ¹ ² ³ ⁴ ⁵ ⁶ ⁷ ⁸ ⁹
¢ $ € £ ¥
Punctuation & symbols
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@ && | ¦ † ‡ ℮ ¶ § © ® ™ ° + − × ÷ = ≠ > < ± ¬ % ✔ ✖ ☜ ☞
↑ ↗ → ↘ ↓ ↙ ← ↖ ● ○ ◆ ◇ ■ □ ▲ ▶ ▼ ◀ △ ▷ ▽ ◁
Plain Form www.plain-form.com
Plain Form is an indepedent typographic practice, focusing on expressive letterforms, meant to be seen as much as to be read
Lucas Descroix www.lucasdescroix.fr
Lucas Descroix likes to draw shapes and to build systems. You can also find him experimenting alternative tools and organizing workshops with Bonjour Monde.
Benjamin Dumond www.benjamindumond.fr
Benjamin Dumond is a graphic designer and founder of grifi.fr, which explores textual potentials through essays, fictions, tools, thought experiments and typefaces.