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The Fibonacci sequence is an infinite series of numbers (0, 1, 1, 2, 3, 5, 8, 13, 21...) where each number is the sum of the two preceding ones. Named after the 13th-century Italian mathematician Leonardo of Pisa (known as Fibonacci), it was popularized in the West through a problem tracking the idealized population growth of rabbits. The sequence holds a profound place in science and art because the ratio between consecutive numbers closely approximates 1.618, the famous Golden Ratio. This mathematical proportion is mirrored throughout nature, dictating the spiral patterns of seashells, sunflowers, pinecones, and even galaxies. In the modern era, Fibonacci numbers are highly practical, serving as a foundational concept for creating search algorithms in computer science and forming the basis for retracement tools used by traders to analyze price movements in financial markets. #mathematics #math #education #science

The Fibonacci sequence is an infinite series of numbers (0, 1, 1, 2, 3, 5, 8, 13, 21...) where each number is the sum of the two preceding ones. Named after the 13th-century Italian mathematician Leonardo of Pisa (known as Fibonacci), it was popularized in the West through a problem tracking the idealized population growth of rabbits. The sequence holds a profound place in science and art because the ratio between consecutive numbers closely approximates 1.618, the famous Golden Ratio. This mathematical proportion is mirrored throughout nature, dictating the spiral patterns of seashells, sunflowers, pinecones, and even galaxies. In the modern era, Fibonacci numbers are highly practical, serving as a foundational concept for creating search algorithms in computer science and forming the basis for retracement tools used by traders to analyze price movements in financial markets. #mathematics #math #education #science

641,100 views

Astronomers calculate a black hole's mass indirectly by measuring its gravitational pull on surrounding matter using Newton's and Kepler's laws. By tracking the orbital speeds and distances of nearby stars or gas clouds, scientists can determine the mass of the invisible center, as faster orbits indicate a heavier black hole. For more distant galaxies, researchers employ "reverberation mapping" to measure the time delay between light flares from the center and their reflections off outer gas clouds, which helps estimate the system's scale. The most direct modern technique involves analyzing radio images to measure the size of the black hole's "shadow" — this dark silhouette is strictly proportional to the radius of the event horizon, allowing physicists to accurately "weigh" the object. #blackhole #scary #astro #spacetok

Astronomers calculate a black hole's mass indirectly by measuring its gravitational pull on surrounding matter using Newton's and Kepler's laws. By tracking the orbital speeds and distances of nearby stars or gas clouds, scientists can determine the mass of the invisible center, as faster orbits indicate a heavier black hole. For more distant galaxies, researchers employ "reverberation mapping" to measure the time delay between light flares from the center and their reflections off outer gas clouds, which helps estimate the system's scale. The most direct modern technique involves analyzing radio images to measure the size of the black hole's "shadow" — this dark silhouette is strictly proportional to the radius of the event horizon, allowing physicists to accurately "weigh" the object. #blackhole #scary #astro #spacetok

547,000 views

The Fibonacci sequence is a famous series of numbers where each number is the sum of the two preceding ones. Typically starting with 0 and 1, the sequence unfolds as 0, 1, 1, 2, 3, 5, 8, 13, 21, 34, 55, and so on. This mathematical progression was introduced to Western mathematics in 1202 by the Italian mathematician Leonardo of Pisa, later known as Fibonacci, who used it to model the idealized growth of a rabbit population. The core mathematical magic of this sequence lies in its direct connection to the Golden Ratio. If you divide any Fibonacci number by the one immediately before it (such as 55 by 34), the result closely approaches the proportional constant of ≈ 1.618. The further you advance down the sequence, the more precisely the ratio between consecutive elements aligns with this universal standard of geometric harmony and balance. This specific proportion is found everywhere around us, earning the Fibonacci sequence its reputation as nature's visual blueprint. The numbers dictate the expansion of the golden spiral, which perfectly matches the shapes of seashells, storm hurricanes, and spiral galaxies. In biology, Fibonacci patterns govern the arrangement of seeds in sunflowers, the scales of pinecones, the layout of leaves on plant stems, and even the skeletal proportions of the human hand. #mathematics #science #education #sciencetok

The Fibonacci sequence is a famous series of numbers where each number is the sum of the two preceding ones. Typically starting with 0 and 1, the sequence unfolds as 0, 1, 1, 2, 3, 5, 8, 13, 21, 34, 55, and so on. This mathematical progression was introduced to Western mathematics in 1202 by the Italian mathematician Leonardo of Pisa, later known as Fibonacci, who used it to model the idealized growth of a rabbit population. The core mathematical magic of this sequence lies in its direct connection to the Golden Ratio. If you divide any Fibonacci number by the one immediately before it (such as 55 by 34), the result closely approaches the proportional constant of ≈ 1.618. The further you advance down the sequence, the more precisely the ratio between consecutive elements aligns with this universal standard of geometric harmony and balance. This specific proportion is found everywhere around us, earning the Fibonacci sequence its reputation as nature's visual blueprint. The numbers dictate the expansion of the golden spiral, which perfectly matches the shapes of seashells, storm hurricanes, and spiral galaxies. In biology, Fibonacci patterns govern the arrangement of seeds in sunflowers, the scales of pinecones, the layout of leaves on plant stems, and even the skeletal proportions of the human hand. #mathematics #science #education #sciencetok

1,900,000 views

Pi (π) is a mathematical constant that shows the relationship between a circle's perimeter and its width. If you take any round object, measure the distance around its edge (circumference), and divide it by the distance straight across its center (diameter), you will always get the exact same result: approximately 3.14. The most fascinating fact about Pi is that it is an infinite number. Its decimals go on forever without any repeating pattern (3.14159...). Because it is impossible to write down the entire number, scientists and students usually shorten it to just 3.14 for everyday calculations. People use Pi every single day without realizing it. Engineers need it to design aircraft wheels and clock gears, architects use it to build domes, and space agencies use it to calculate spacecraft orbits. From the wheels on a bicycle to the waves of your Wi-Fi signal, Pi is hidden in everything that rotates or moves in waves. #mathematics #science #π #education

Pi (π) is a mathematical constant that shows the relationship between a circle's perimeter and its width. If you take any round object, measure the distance around its edge (circumference), and divide it by the distance straight across its center (diameter), you will always get the exact same result: approximately 3.14. The most fascinating fact about Pi is that it is an infinite number. Its decimals go on forever without any repeating pattern (3.14159...). Because it is impossible to write down the entire number, scientists and students usually shorten it to just 3.14 for everyday calculations. People use Pi every single day without realizing it. Engineers need it to design aircraft wheels and clock gears, architects use it to build domes, and space agencies use it to calculate spacecraft orbits. From the wheels on a bicycle to the waves of your Wi-Fi signal, Pi is hidden in everything that rotates or moves in waves. #mathematics #science #π #education

2,400,000 views

The Theodorus Spiral (or Pythagorean snail), first described by the ancient Greek mathematician Theodorus of Cyrene in the 5th century BC, is a sequence of contiguous right-angled triangles. Its core purpose was to serve as a geometric calculator for constructing irrational lengths, allowing ancient scholars to visually demonstrate and precisely measure numbers that cannot be expressed as simple fractions. The construction begins with a triangle whose shorter sides equal one, and each subsequent element is built upon the longest side of the previous one. By always adding a new outer side of the same fixed length of one, the spiral mechanically generates exact lines representing the values of consecutive square roots without using complex arithmetic. In its original form, the triangles complete a full turn and begin to overlap each other at the 17th step, which is exactly where Theodorus stopped his calculations. If you continue this mathematical process infinitely, the vertices of the figure smoothly approximate the shape of a continuous Archimedean spiral. #geometry #mathematics #school #physics

The Theodorus Spiral (or Pythagorean snail), first described by the ancient Greek mathematician Theodorus of Cyrene in the 5th century BC, is a sequence of contiguous right-angled triangles. Its core purpose was to serve as a geometric calculator for constructing irrational lengths, allowing ancient scholars to visually demonstrate and precisely measure numbers that cannot be expressed as simple fractions. The construction begins with a triangle whose shorter sides equal one, and each subsequent element is built upon the longest side of the previous one. By always adding a new outer side of the same fixed length of one, the spiral mechanically generates exact lines representing the values of consecutive square roots without using complex arithmetic. In its original form, the triangles complete a full turn and begin to overlap each other at the 17th step, which is exactly where Theodorus stopped his calculations. If you continue this mathematical process infinitely, the vertices of the figure smoothly approximate the shape of a continuous Archimedean spiral. #geometry #mathematics #school #physics

962,000 views

The fact that Earth is a globe can be easily observed by looking up at the night sky. As you travel north or south, entirely new constellations appear while others sink below the horizon, which proves you are moving across a curved surface rather than a flat plane. Additionally, the North Star alters its position in the sky depending on your latitude, providing a reliable cosmic map that only makes sense on a round planet. On the ground, the physical geometry of our world is revealed through the behavior of light and shadows. If the Earth were flat, a high tower and a deep well hundreds of miles apart would cast identical shadows under the sun at noon, but real-world measurements show distinct variations in angles. This curvature is also why we can increase our line of sight and see much farther across the horizon simply by climbing to a higher altitude. Finally, modern technology and physics offer absolute certainty about our planet's shape. Satellite communication networks and GPS navigation rely entirely on mathematical models of a rotating sphere to transmit precise data around the globe. Furthermore, the fundamental law of gravity dictates that any cosmic body with enough mass will naturally pull itself into a compact, spherical shape over time. #earth #anime #fact #science

The fact that Earth is a globe can be easily observed by looking up at the night sky. As you travel north or south, entirely new constellations appear while others sink below the horizon, which proves you are moving across a curved surface rather than a flat plane. Additionally, the North Star alters its position in the sky depending on your latitude, providing a reliable cosmic map that only makes sense on a round planet. On the ground, the physical geometry of our world is revealed through the behavior of light and shadows. If the Earth were flat, a high tower and a deep well hundreds of miles apart would cast identical shadows under the sun at noon, but real-world measurements show distinct variations in angles. This curvature is also why we can increase our line of sight and see much farther across the horizon simply by climbing to a higher altitude. Finally, modern technology and physics offer absolute certainty about our planet's shape. Satellite communication networks and GPS navigation rely entirely on mathematical models of a rotating sphere to transmit precise data around the globe. Furthermore, the fundamental law of gravity dictates that any cosmic body with enough mass will naturally pull itself into a compact, spherical shape over time. #earth #anime #fact #science

1,300,000 views

The 6-orthoplex (also known as the hexacross or hexacontatetrahedron) is a regular six-dimensional geometric polytope. It belongs to the cross-polytope (hyperoctahedral) family, serving as the 6D analogue of a 3D octahedron and a 2D square. In Cartesian coordinates, its vertices are positioned in pairs along six mutually perpendicular axes, defining its highly symmetric structure. This multi-dimensional object consists of 12 vertices, 60 edges, 160 triangular faces, and 240 tetrahedral cells. Furthermore, its boundary is formed by 192 four-dimensional hyperfaces and 64 five-dimensional facets, each of which is a regular 5-simplex (the 5D analogue of a tetrahedron). All of these elements are perfectly uniform, creating an ideal enclosed figure in six-dimensional space. In higher-dimensional geometry, the 6-orthoplex is the dual polytope of the hexeract (the 6D hypercube), meaning the centers of a hexeract's facets correspond to the vertices of a 6-orthoplex. It is represented by the Schläfli symbol {3,3,3,3,4}. Its structural symmetry is governed by the hyperoctahedral group B₆, which consists of 46,080 distinct rotations and reflections. #geometry #mathematics #science #education

The 6-orthoplex (also known as the hexacross or hexacontatetrahedron) is a regular six-dimensional geometric polytope. It belongs to the cross-polytope (hyperoctahedral) family, serving as the 6D analogue of a 3D octahedron and a 2D square. In Cartesian coordinates, its vertices are positioned in pairs along six mutually perpendicular axes, defining its highly symmetric structure. This multi-dimensional object consists of 12 vertices, 60 edges, 160 triangular faces, and 240 tetrahedral cells. Furthermore, its boundary is formed by 192 four-dimensional hyperfaces and 64 five-dimensional facets, each of which is a regular 5-simplex (the 5D analogue of a tetrahedron). All of these elements are perfectly uniform, creating an ideal enclosed figure in six-dimensional space. In higher-dimensional geometry, the 6-orthoplex is the dual polytope of the hexeract (the 6D hypercube), meaning the centers of a hexeract's facets correspond to the vertices of a 6-orthoplex. It is represented by the Schläfli symbol {3,3,3,3,4}. Its structural symmetry is governed by the hyperoctahedral group B₆, which consists of 46,080 distinct rotations and reflections. #geometry #mathematics #science #education

626,500 views

TON 618 is not just a black hole, but a superluminous quasar, at the center of which lies one of the most massive known black holes. Its precise celestial coordinates are right ascension 12h 28m 24.9s, declination +31° 28′ 38″. The object is located on the border of the constellations Canes Venatici and Coma Berenices. The light we observe today left TON 618 about 10.8 billion years ago, when the universe was less than 3 billion years old. Its redshift is z = 2.219, making it one of the most distant and ancient objects available for detailed study. TON 618's most famous feature is its central supermassive black hole. Current estimates place its mass at approximately 40.7 billion solar masses, although earlier studies have suggested values as high as 66 billion solar masses. Even by a more conservative estimate, it is one of the largest known objects of its type. The Schwarzschild radius of this black hole is approximately 1,300 astronomical units, more than 60 times the distance from the Sun to Pluto. For comparison, if TON 618's event horizon were placed at the center of the Solar System, it would engulf space far beyond the orbit of Neptune. However, we observe not the black hole itself, but the accretion disk surrounding it — a gigantic structure of gas and plasma heated to millions of degrees. As matter falls into the gravitational well, a tremendous amount of energy is released, causing the quasar to shine approximately 140 trillion times brighter than the Sun and completely outshine the galaxy in which it resides. #ton618 #blackhole #scary #astrophysics

TON 618 is not just a black hole, but a superluminous quasar, at the center of which lies one of the most massive known black holes. Its precise celestial coordinates are right ascension 12h 28m 24.9s, declination +31° 28′ 38″. The object is located on the border of the constellations Canes Venatici and Coma Berenices. The light we observe today left TON 618 about 10.8 billion years ago, when the universe was less than 3 billion years old. Its redshift is z = 2.219, making it one of the most distant and ancient objects available for detailed study. TON 618's most famous feature is its central supermassive black hole. Current estimates place its mass at approximately 40.7 billion solar masses, although earlier studies have suggested values as high as 66 billion solar masses. Even by a more conservative estimate, it is one of the largest known objects of its type. The Schwarzschild radius of this black hole is approximately 1,300 astronomical units, more than 60 times the distance from the Sun to Pluto. For comparison, if TON 618's event horizon were placed at the center of the Solar System, it would engulf space far beyond the orbit of Neptune. However, we observe not the black hole itself, but the accretion disk surrounding it — a gigantic structure of gas and plasma heated to millions of degrees. As matter falls into the gravitational well, a tremendous amount of energy is released, causing the quasar to shine approximately 140 trillion times brighter than the Sun and completely outshine the galaxy in which it resides. #ton618 #blackhole #scary #astrophysics

4,600,000 views

The number Pi (π) is a mathematical constant representing the ratio of a circle's circumference to its diameter. Regardless of the circle's size, this ratio always remains the same and is commonly rounded to 3.14 for everyday calculations. The symbol π, derived from the Greek word for perimeter, was first introduced by William Jones in 1706 and later popularized by Leonhard Euler, leading to the global celebration of Pi Day on March 14th (3/14). The defining characteristic of Pi is that it is both irrational and transcendental, meaning its decimal expansion is infinite and never falls into a repeating pattern. Scientists and mathematicians use powerful supercomputers to continuously push boundaries, having already calculated more than 100 trillion digits past the decimal point. For most precise scientific calculations, however, just the first few digits — 3.14159265 — are more than enough. In the practical world, Pi is indispensable across geometry, architecture, physics, and aerospace engineering. Beyond measuring the area of a circle or the volume of a sphere, it allows engineers to calculate satellite orbits, wave oscillations, and electromagnetic fields. It inherently weaves through the fabric of our universe wherever circular motion, rotation, or waves occur. #pi #mathematics #science #facts

The number Pi (π) is a mathematical constant representing the ratio of a circle's circumference to its diameter. Regardless of the circle's size, this ratio always remains the same and is commonly rounded to 3.14 for everyday calculations. The symbol π, derived from the Greek word for perimeter, was first introduced by William Jones in 1706 and later popularized by Leonhard Euler, leading to the global celebration of Pi Day on March 14th (3/14). The defining characteristic of Pi is that it is both irrational and transcendental, meaning its decimal expansion is infinite and never falls into a repeating pattern. Scientists and mathematicians use powerful supercomputers to continuously push boundaries, having already calculated more than 100 trillion digits past the decimal point. For most precise scientific calculations, however, just the first few digits — 3.14159265 — are more than enough. In the practical world, Pi is indispensable across geometry, architecture, physics, and aerospace engineering. Beyond measuring the area of a circle or the volume of a sphere, it allows engineers to calculate satellite orbits, wave oscillations, and electromagnetic fields. It inherently weaves through the fabric of our universe wherever circular motion, rotation, or waves occur. #pi #mathematics #science #facts

412,200 views

The new second-generation Tesla Roadster lifts off the ground and performs controlled jumps using cold-gas pneumatic thrusters developed in partnership with SpaceX. Instead of wings or propellers, the electric supercar pumps air under high pressure into a 600-liter composite tank and releases it in sharp bursts through a system of nozzles. This allows the top-tier single-seat Rocket trim to leap up to 10 meters into the air, clear obstacles like semi-trucks, execute barrel rolls or flips mid-air, and land smoothly back on its wheels. Additionally, powerful underbody suction fans generate intense downforce, enabling the car to drive upside down along specially designed ramps. #tesla #usa #elonmusk #spacetok

The new second-generation Tesla Roadster lifts off the ground and performs controlled jumps using cold-gas pneumatic thrusters developed in partnership with SpaceX. Instead of wings or propellers, the electric supercar pumps air under high pressure into a 600-liter composite tank and releases it in sharp bursts through a system of nozzles. This allows the top-tier single-seat Rocket trim to leap up to 10 meters into the air, clear obstacles like semi-trucks, execute barrel rolls or flips mid-air, and land smoothly back on its wheels. Additionally, powerful underbody suction fans generate intense downforce, enabling the car to drive upside down along specially designed ramps. #tesla #usa #elonmusk #spacetok

48,800 views

The Hadean (or Katarchean) Eon is the earliest geological eon in Earth's history (4.57 – 4.03 billion years ago), during which modern science increasingly suggests the emergence of primitive life, challenging older views of a completely barren world. While the young planet experienced the birth of the Moon from a collision with Theia, differentiated into a core and mantle, and cooled under a dense carbon dioxide atmosphere, the first basins of hot liquid water had already condensed by 4.4 billion years ago. In this extreme environment, rich in geothermal vents and volcanic glass, chemical evolution thrived, laying the groundwork for the RNA world. Although direct fossils have been erased by the continuous recycling of the early crust, compelling indirect evidence — such as 4.1-billion-year-old biogenic carbon isotopes trapped inside Australian zircon crystals and genetic modeling of the universal ancestor LUCA — strongly indicates that primitive, anaerobic life may have already originated and adapted to these harsh conditions by the late Hadean. #earth #science #education #spacetok

The Hadean (or Katarchean) Eon is the earliest geological eon in Earth's history (4.57 – 4.03 billion years ago), during which modern science increasingly suggests the emergence of primitive life, challenging older views of a completely barren world. While the young planet experienced the birth of the Moon from a collision with Theia, differentiated into a core and mantle, and cooled under a dense carbon dioxide atmosphere, the first basins of hot liquid water had already condensed by 4.4 billion years ago. In this extreme environment, rich in geothermal vents and volcanic glass, chemical evolution thrived, laying the groundwork for the RNA world. Although direct fossils have been erased by the continuous recycling of the early crust, compelling indirect evidence — such as 4.1-billion-year-old biogenic carbon isotopes trapped inside Australian zircon crystals and genetic modeling of the universal ancestor LUCA — strongly indicates that primitive, anaerobic life may have already originated and adapted to these harsh conditions by the late Hadean. #earth #science #education #spacetok

61,600 views

TON 618 is an incredibly luminous quasar located in the constellation Canes Venatici, roughly 18.2 billion light-years away from Earth. At its heart lies one of the most massive black holes ever discovered in the universe. Weighing between 40.7 and 66 billion solar masses, this single object is heavy enough to rival the entire baryonic mass (stars, gas, and dust) of our whole Milky Way galaxy combined. This cosmic titan boasts staggering scales and power. Its event horizon spans nearly 390 billion kilometers in diameter, which is about 26 times the size of Pluto's entire orbit. The superheated disk of gas swirling around the black hole rotates at an astonishing 7,000 km/s and shines with the light of 140 trillion Suns, completely outshining its host galaxy. First discovered in 1954, the object was initially mistaken for a faint blue star. It wasn't until the 1970s that astronomers realized they were looking at an extremely distant active galactic nucleus from the early universe. The light we see from TON 618 traveled for 10.4 billion years to reach us, offering a rare glimpse into extreme physics just a few billion years after the Big Bang. #ton618 #scary #blackhole #astro

TON 618 is an incredibly luminous quasar located in the constellation Canes Venatici, roughly 18.2 billion light-years away from Earth. At its heart lies one of the most massive black holes ever discovered in the universe. Weighing between 40.7 and 66 billion solar masses, this single object is heavy enough to rival the entire baryonic mass (stars, gas, and dust) of our whole Milky Way galaxy combined. This cosmic titan boasts staggering scales and power. Its event horizon spans nearly 390 billion kilometers in diameter, which is about 26 times the size of Pluto's entire orbit. The superheated disk of gas swirling around the black hole rotates at an astonishing 7,000 km/s and shines with the light of 140 trillion Suns, completely outshining its host galaxy. First discovered in 1954, the object was initially mistaken for a faint blue star. It wasn't until the 1970s that astronomers realized they were looking at an extremely distant active galactic nucleus from the early universe. The light we see from TON 618 traveled for 10.4 billion years to reach us, offering a rare glimpse into extreme physics just a few billion years after the Big Bang. #ton618 #scary #blackhole #astro

733,100 views

Infinity is an abstract concept that denotes boundlessness, endlessness, or the absence of any limit and quantitative measure. Contrary to popular belief, infinity (represented by the symbol ∞) is not a number, but rather a property of mathematical sets, spaces, or processes that can never be exhausted or measured using standard digits. In science, the concept of infinity manifests in various ways. In mathematics, it describes endless series of numbers, where some infinities can actually be "larger" than others (for instance, the number of points on a line is greater than the total count of whole numbers). In physics and cosmology, the term is used when studying the structure of the Universe and the density of black holes, while in philosophy, it helps contemplate eternity and the absolute diversity of the world. The familiar symbol resembling a sideways figure eight is called a lemniscate. It was first introduced to science by the English mathematician John Wallis in 1655. Historians link the shape of the sign either to the Greek letter ω (omega) or to the ancient Roman notation for the number 1,000, which ancient peoples frequently associated with an uncountably large quantity. #sciencetok #mathematics #education #infinity

Infinity is an abstract concept that denotes boundlessness, endlessness, or the absence of any limit and quantitative measure. Contrary to popular belief, infinity (represented by the symbol ∞) is not a number, but rather a property of mathematical sets, spaces, or processes that can never be exhausted or measured using standard digits. In science, the concept of infinity manifests in various ways. In mathematics, it describes endless series of numbers, where some infinities can actually be "larger" than others (for instance, the number of points on a line is greater than the total count of whole numbers). In physics and cosmology, the term is used when studying the structure of the Universe and the density of black holes, while in philosophy, it helps contemplate eternity and the absolute diversity of the world. The familiar symbol resembling a sideways figure eight is called a lemniscate. It was first introduced to science by the English mathematician John Wallis in 1655. Historians link the shape of the sign either to the Greek letter ω (omega) or to the ancient Roman notation for the number 1,000, which ancient peoples frequently associated with an uncountably large quantity. #sciencetok #mathematics #education #infinity

388,300 views

A system where a black hole replaces a star is scientifically plausible, and planets orbiting within it are informally called "blaneets" (a mashup of black hole and planet). Contrary to popular myths, a black hole does not inevitably suck in everything around it; if it has the same mass as our Sun, planets will orbit it along the exact same stable paths as they do in the Solar System. The primary difference is the complete absence of familiar starlight and warmth. Such planets can originate in three ways: surviving the supernova explosion that created the black hole, forming anew from its surrounding dust and gas disk, or being gravitationally captured from deep space. Instead of a sun, the energy source for this system would be an accretion disk — a ring of matter swirling around the black hole that gets heated to millions of degrees by friction, causing it to glow intensely. Theoretically, life on a blaneet is possible, but only around supermassive black holes and under extremely hostile conditions. Instead of a sun, the local biosphere would be illuminated by a giant, radiant ring, and the planet would need an incredibly dense atmosphere to shield against deadly X-ray radiation. Furthermore, due to the colossal gravity, time on the surface of such a world would tick much slower than in the rest of the universe. #blackhole #scary #science #spacetok

A system where a black hole replaces a star is scientifically plausible, and planets orbiting within it are informally called "blaneets" (a mashup of black hole and planet). Contrary to popular myths, a black hole does not inevitably suck in everything around it; if it has the same mass as our Sun, planets will orbit it along the exact same stable paths as they do in the Solar System. The primary difference is the complete absence of familiar starlight and warmth. Such planets can originate in three ways: surviving the supernova explosion that created the black hole, forming anew from its surrounding dust and gas disk, or being gravitationally captured from deep space. Instead of a sun, the energy source for this system would be an accretion disk — a ring of matter swirling around the black hole that gets heated to millions of degrees by friction, causing it to glow intensely. Theoretically, life on a blaneet is possible, but only around supermassive black holes and under extremely hostile conditions. Instead of a sun, the local biosphere would be illuminated by a giant, radiant ring, and the planet would need an incredibly dense atmosphere to shield against deadly X-ray radiation. Furthermore, due to the colossal gravity, time on the surface of such a world would tick much slower than in the rest of the universe. #blackhole #scary #science #spacetok

264,200 views

pov: you found yourself in orbit around a pulsar💀 A PULSAR is a superdense, rapidly rotating neutron star born from the explosive death of a massive star in a supernova. It packs a mass greater than that of our Sun into a sphere only 20 to 25 kilometers in diameter. Because of this extreme density, a single teaspoon of pulsar material would weigh billions of tons on Earth. The defining feature of a pulsar is the powerful, narrowly focused beam of radiation blasting from its magnetic poles. As the star spins, its tilted magnetic axis causes these beams to sweep across space. Whenever a beam sweeps past Earth, telescopes detect it as a strictly periodic pulse, much like the flashing beam of a cosmic lighthouse. The rotation speeds of these objects are astonishing, with periods ranging from several seconds down to milliseconds, meaning some spin hundreds of times per second. Because this rotation is incredibly stable, pulsars act as the universe's most precise natural clocks, helping scientists test Einstein's theory of general relativity and detect gravitational waves. #pulsar #scary #spacetok #astro

pov: you found yourself in orbit around a pulsar💀 A PULSAR is a superdense, rapidly rotating neutron star born from the explosive death of a massive star in a supernova. It packs a mass greater than that of our Sun into a sphere only 20 to 25 kilometers in diameter. Because of this extreme density, a single teaspoon of pulsar material would weigh billions of tons on Earth. The defining feature of a pulsar is the powerful, narrowly focused beam of radiation blasting from its magnetic poles. As the star spins, its tilted magnetic axis causes these beams to sweep across space. Whenever a beam sweeps past Earth, telescopes detect it as a strictly periodic pulse, much like the flashing beam of a cosmic lighthouse. The rotation speeds of these objects are astonishing, with periods ranging from several seconds down to milliseconds, meaning some spin hundreds of times per second. Because this rotation is incredibly stable, pulsars act as the universe's most precise natural clocks, helping scientists test Einstein's theory of general relativity and detect gravitational waves. #pulsar #scary #spacetok #astro

133,900 views

The Andromeda Galaxy is rapidly approaching the Milky Way at a speed of about 110–120 km/s due to mutual gravitational pull. Currently, about 2.5 million light-years separate us, but this distance is steadily shrinking, making a monumental cosmic collision inevitable in the deep future. The actual collision will begin in about 4 to 5 billion years. Direct physical impacts between individual stars are highly unlikely due to the vast empty spaces within both galaxies; however, immense gravitational forces will completely tear apart their familiar spiral structures. During this cosmic dance, interstellar gas will compress, triggering a brilliant but brief surge in the birth of billions of new stars. In about 6 to 7 billion years, the process will conclude with the formation of a single, giant elliptical galaxy colloquially named Milkomeda. The supermassive black holes at their cores will merge into one, the remaining gas reserves will be depleted, and this new cosmic system will begin to slowly fade, populated mostly by old, long-lived red stars. #andromeda #galaxy #astro #astronomy

The Andromeda Galaxy is rapidly approaching the Milky Way at a speed of about 110–120 km/s due to mutual gravitational pull. Currently, about 2.5 million light-years separate us, but this distance is steadily shrinking, making a monumental cosmic collision inevitable in the deep future. The actual collision will begin in about 4 to 5 billion years. Direct physical impacts between individual stars are highly unlikely due to the vast empty spaces within both galaxies; however, immense gravitational forces will completely tear apart their familiar spiral structures. During this cosmic dance, interstellar gas will compress, triggering a brilliant but brief surge in the birth of billions of new stars. In about 6 to 7 billion years, the process will conclude with the formation of a single, giant elliptical galaxy colloquially named Milkomeda. The supermassive black holes at their cores will merge into one, the remaining gas reserves will be depleted, and this new cosmic system will begin to slowly fade, populated mostly by old, long-lived red stars. #andromeda #galaxy #astro #astronomy

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Milkomeda is the name of the future galaxy that will form after the merger of the Milky Way and Andromeda galaxies in approximately 4-5 billion years. Andromeda is gradually approaching the Milky Way, and over time, their gravity will completely merge the two galaxies into a single, massive system. Despite the scale of the event, stars will rarely collide directly because the distances between them are enormous. During the merger, the orbits of the stars will change, powerful bursts of star formation will occur, and the supermassive black holes at the centers of the galaxies will also eventually merge. The resulting galaxy is expected to resemble a giant elliptical galaxy, and it is this galaxy that is provisionally called Milkomeda. It is believed that by the time of the final merger, the Sun will have already become significantly hotter, and conditions on Earth will likely be unsuitable for life. The night sky will look completely different over the next billions of years: Andromeda will gradually occupy a huge portion of the horizon and then dissolve into the overall structure of the new galaxy. Scientists also suggest that after Milkomeda forms, it will become one of the dominant galaxies in our local group and continue to absorb smaller satellite galaxies. #milkyway #andromeda #scary #galaxy

Milkomeda is the name of the future galaxy that will form after the merger of the Milky Way and Andromeda galaxies in approximately 4-5 billion years. Andromeda is gradually approaching the Milky Way, and over time, their gravity will completely merge the two galaxies into a single, massive system. Despite the scale of the event, stars will rarely collide directly because the distances between them are enormous. During the merger, the orbits of the stars will change, powerful bursts of star formation will occur, and the supermassive black holes at the centers of the galaxies will also eventually merge. The resulting galaxy is expected to resemble a giant elliptical galaxy, and it is this galaxy that is provisionally called Milkomeda. It is believed that by the time of the final merger, the Sun will have already become significantly hotter, and conditions on Earth will likely be unsuitable for life. The night sky will look completely different over the next billions of years: Andromeda will gradually occupy a huge portion of the horizon and then dissolve into the overall structure of the new galaxy. Scientists also suggest that after Milkomeda forms, it will become one of the dominant galaxies in our local group and continue to absorb smaller satellite galaxies. #milkyway #andromeda #scary #galaxy

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