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Bill Haley
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Heart-shaped tape of an audio cassette
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Black Holes Fusion - Artist view - Black holes collide - Artist view - Artist view of a collision of galactic black holes. Galactic black holes merge
Supermassif black hole - Artist view - Supermassive Black hole - Artist view - Artist view of a supermassive black hole in the center of a galaxy. This artist's concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies. (Smaller black holes also exist throughout galaxies.) In this illustration, the supermassive black hole at the center is surrounded by matter flowing onto the black hole in what is termed an accretion disk. This disk forms as the dust and gas in the galaxy falls onto the hole, attracted by its gravity
Supermassif black hole - Artist's view - Supermassive black hole with torn-apart star (artist's impression): Artist's view of a supermassive black hole in the center of a galaxy. This artist's impression depicts a rapidly spinning supermassive black hole surrounded by an accretion disc. This thin disc of rotating material consists of the leftovers of a Sun-like star which was ripped apart by the tidal forces of the black hole. Shocks in the colliding debris as well as heat generated in accretion led to a burst of light, resembling a supernova explosion
Relief of Amenophis IV (Akhenaten) (c.1352-1336 BC) as a sphinx, New Kingdom (limestone)
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Artist's view of a proto-star - Protostar Disk: A star proto is a pile of dust and gas that contracts to form a star
La formation du Système solaire - Vue d'artiste - Solar system formation - Artist view - Vue d'artiste de la naissance du système solaire. After the explosion of a supernova, an interstellar cloud of gas and dust heated and contracted to give birth to our star. In a few tens of millions of years, debris assembles around the sun and planets form. Following a supernova explosion, a cloud of gas and dust start to collapse forming a solar nebula. Particles around spinning, begin to stick together through accretion to make planetesimals, and then planets
Artist view of Beta Pictoris b - Beta Pictoris b. Artwork: Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbit around the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three-thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light-years away towards the constellation of Pictor (the Painter) and is one of the best-known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell-tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth-Sun separation - or Astronomical Units - which is about the distance Saturn is from the Sun. The planet has a mass of about nine Jupiter masses and is right mass and location to explain the observed warp in the inner parts of the disc
Scenario of a star formation - In a cloud of gas and interstellar dust, a blood cell contracts and heats. The blood cell flattens in a disc around the young star. The star starts to shine. In a cloud of gaz and interstellar dust a dark globule will contract to create a rotating disk flattening; at the center of this disk, the stars ingnites
Artist view of Cygnus X-1 - Cygnus X-1 is a binary star X and was the first black hole candidate. This system consists of the 226868 HD star, a supergeant star, orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. Cygnus X-1 is an X-ray binary system and the first black hole candidates to be discovered
Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape
PI (ceremonial disk) (jade)
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Black hole - Artist view - Black Hole and Red Giant - Artist view - A giant red star orbiting a black hole. A black hole doing some damage to a passing red giant star
Stellar black hole - Artist view - Stellar black hole - Artist view - A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. A stellar black hole is a black hole formed by the gravitational collapse of a massive star; it is also a region of space in which the gravitational field is so powerful that nothing can escape
Bi (olive green, buff altered nephrite)
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Artist's view of the double star Epsilon Aurigae (Almaaz) - Binary star Epsilon Aurigae. Artwork - Almaaz is a binary star with a strange eclipse; it is eclipsed by a gigantic companion for two years. It is believed that this companion could be composed of one or two stars surrounded by a large disc of dust. The visible companion is a yellow supergiant type F, one of the brightest stars in the sky. Epsilon Aurigae (Almaaz) is an eclipsing binary star
Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and positrons (antielectrons) move outward from this ring to brighten the outer ring and produce an extended X - ray glow. The fingers, loops, and bays in the image all indicate that the magnetic field of the nebula and filaments of cooler matter are controlling the motion of the electrons and positrons. The particles can move rapidly along the magnetic field and travel several light years before radiating away their energy. In contrast, they move much more slowly perpendicular to the magnetic field, and travel only a short distance before losing their energy. This effect can explain the long, thin, fingers and loops, as well as the sharp boundaries of the bays. The conspicuous dark bays on the lower right and left are likely due to the effects of a toroidal magnetic field that is a relic of the progenitor star. Image taken by Chandra X - ray telescope
Primitive black hole - Artist view - Primitive Black hole - Artist view - Artist view of a primitive galactic black hole. The presence of 13 billion-year-old black holes was observed by the Spitzer space telescope. These distant black holes appear in the early stages of their formation; their accretion disc contains no dust. This artist's conception illustrates one of the most primitive supermassive black holes known (central black dot) at the core of a young, star-rich galaxy. Astronomers using Nasa's Spitzer Space Telescope have uncovered two of these early objects, dating back to about 13 billion years ago. The monstrous black holes are among the most distant known, and appear to be in the very earliest stages of formation, earlier than any observed so far. Unlike all other supermassive black holes probed to date, this primitive duo, called J0005-0006 and J0303-0019, lacks dust. As the drawing shows, gas swirls around a black hole in what is called an accretion disk. Usually, the accretion disk is surrounded by a dark doughnut-like dusty structure called a dust torus. But for the primitive black holes, the dust tori are missing and only gas disks are observed. This is because the early universe was clean as a whistle. Enough time had not passed for molecules to clump together into dust particles. Some black holes forming in this era thus started out lacking dust. As they grew, gobbling up more and more mass, they are thought to have accumulated dusty rings. This illustration also shows how supermassive black holes can distort space and light around them (see warped stars behind black hole). Stars from the galaxy can be seen sprinkled throughout, and distant mergers between other galaxies are illustrated in the background
Ballot Discs, 480 BC (terracotta)
Scarab beetle and vulture wings under disk of the sun. Limestone relief, Edfu.
Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a star orbiting around a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space where gravity is so strong that it stops any form of material or radiation from escaping. Combining observations done with Eso's Very Large Telescope and Nasa's Chandra X-ray telescope, astronomers have uncovered the most powerful pair of jets ever seen from a stellar black hole. The black hole blows a huge bubble of hot gas, 1000 light-years across or twice as large and tens of times more powerful than the other such microquasars. The stellar black hole belongs to a binary system as pictured in this artist's impression
Still Life of CD
Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a Wolf-Rayet star orbiting a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. This artist's impression depicts a star-mass black hole. The black hole has a mass of about twenty times the mass of the Sun and is associated with a Wolf-Rayet star: a star that will become a black hole itself. The black hole is stripping matter away from the star as they orbit each other
Central disc round 33 laps, with the dog: “” The voice of his master”””.1965.
Beta Pictoris b - Artist's view of Beta Pictoris b, a giant exoplanet with a mass equivalent to 9 times the mass of Jupiter orbiting the star Beta Pictoris. This artist's impression shows how the planet inside the disc of Beta Pictoris may look. Only 12 million years old, or less than three - thousandths of the age of the Sun, Beta Pictoris is 75% more massive than our parent star. It is located about 60 light - years away towards the constellation of Pictor (the Painter) and is one of the best - known examples of a star surrounded by a dusty debris disc. Earlier observations showed a warp of the disc, a secondary inclined disc and comets falling onto the star, all indirect, but tell - tale signs that strongly suggested the presence of a massive planet. Observations done with the NACO instrument on Eso's Very Large Telescope in 2003, 2008 and 2009, have proven the presence of a planet around Beta Pictoris. It is located at a distance between 8 and 15 times the Earth - Sun separation - - or Astronomical Units - - which is about the distance Saturn is from the Sun. The planet has a mass of about nine Jupiter masses and is right mass and location to explain the observed warp in the inner parts of the disc
Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical units. (One astronomical unit is the distance from Earth to the Sun, which is 150 - million kilometers or 93 - million miles). Scientists compared the surface brightness of the disk in the infrared wavelengths to determine the temperature distribution of the disk and then refer the corresponding particle size in the disk. Most of the particles in the disk are only a few microns in size, or 100 times smaller than a grain of Earth sand. These fine dust particles originate from collisions of embryonic planets near the star at a radius of approximately 90 astronomical units, and are then blown away by Vega's intense radiation. The mass and short lifetime of these small particles indicate that the disk detected by Spitzer is the aftermath of a large and relatively recent collision, involving bodies perhaps as big as the planet Pluto. The images are 3 arcminutes on each side. North is oriented upward and east is to the left
Stellar black hole - Artist view - Stellar Black Hole - Artist view - A stellar black hole powered by a K-type star makes a contribution to an orbiting black hole
Kim Wilde
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Carved disk from Copan showing priests. Mayan civilisation, Honduras
Brown dwarf with a large debris ring - Artist's view of a brown dwarf star surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet illuminated by the star. This imaginary high - mass brown dwarf has a larger disk than the previous renderings. The perspective is from the equator of an airless planet, orbiting the brown dwarf at a distance of about 4 million miles. This planet's orbit is very nearly aligned to the plane of the rings, hence the debris appears as a sword - like straight line
The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist
Collared disk, 1200s BC (nephrite)
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Pectoral jewel from treasure of Tutankhamun showing falcon headed god with sun disk (Aton)
The Magic Violin
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Pierced disc with notched edges (pale green nephrite)
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Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - Artist's view of the extrasolar planet Fomalhaut b, a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years ago - light from Earth in the constellation of the Southern Fish. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. This illustration shows the discovered planet, Fomalhaut b, orbiting its sun, Fomalhaut. This structure is a Saturn - like ring that astronomers say may encircle the planet. Fomalhaut also is surrounded by a ring of material. The edge of this vast disk is shown in the background as the curving cloud - like feature that appears to intersect the 200 - million year - old star. Fomalhaut b lies three billion kilometers inside the disk's inner edge. The planet completes an orbit around Fomalhaut every 872 years
SS 433 - Artist's view: SS 433 is a binary star in the constellation of the Eagle, composed of a supergeant star orbiting around a black hole
Pierced disk (nephrite)
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La formation du système solaire - Vue d'artiste - Artist's impression of the development of the Solar System - Vue d'artiste de planete en formation dans le disque de gaz et de dusts (disque protoplanetaire) autour de son toile. This artist's impression shows four stages of the development of the inner Solar System over a period of almost five billion years. The top panel shows the earliest stage where the debris disc around the Sun was composed of gas and tiny particles, typically less than one millimetre across. At the second stage the particles have formed large clumps, roughly 100 kilometers across and, similar to the asteroid Lutetia. These bodies in turn formed the rocky planets including the Earth, shown in the third panel down. Over the subsequent four billion years the surface of the Earth developed to what we know now under the influence of meteor bombardment that delivered volatile materials including water, and the evolution of life on its surface
Pierced disk (nephrite)
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Pierced Disc with To-Tie (T'ao-T'ieh) (brown nephrite)
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1950s: Hands touch steel rod to copper wire holding frog's legs
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U Geminorum in the sky of an exoplanet - U Geminorum seen from an exoplanet. Artwork - U Geminorum is a dwarf nova, a variable star composed of a white dwarf orbiting around a red dwarf. This binary greenhouse system is represented here in the sky of an extrasolar planet. Artwork showing U Geminorum in the sky of an exoplanet. U Geminorum, in the constellation Gemini, is an archetypal example of a dwarf nova. The binary star system consists of a white dwarf closely orbiting a red dwarf
1950s: Table with scientific apparatus
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Disc of Phaestos, 1700-1600 BC (fired clay)
Huan disc, c.2400 BC (green nephrite)
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Mayan turquoise-mosaic Disk
Collared disc (grey-white nephrite)
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Vinyl Records
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Star, Planet and Brown Dwarf Formation - Schema illustrating how stars (left), planets (middle) and brown dwarf (right) form based on the mass of their primitive nebula. Infographic showing how stars (left arrow), planets (middle), and brown dwarfs (right) form depending on the mass of their parent nebula. Artwor
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Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilometers across. Fomalhaut b lies three billion kilometers inside the ring's inner edge and orbits 17 billion kilometers from its star. The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. Astronomers have calculated that Fomalhaut b completes an orbit around its parent star every 872 years. The white dot in the centre of the image marks the star's location. The region around Fomalhaut's location is black because astronomers used the Advanced Camera's coronagraph to block out the star's bright glare so that the dim planet could be seen. Fomalhaut b is 100 million times fainter than its star. The radial streaks are scattered starlight. The red dot at lower left is a background star. The Fomalhaut system is 25 light - years away in the constellation Piscis Austrinus. This false - colour image was taken in October 2004 and July 2006
Circular disk, 10th century BC (green nephrite)
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BI (PI) disc (grey nephrite)
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Active galaxies in collision - Artist view - Active galaxies collide - Artist view - Artist view of a quasar whose jet is powered by the material of a galaxy rentree in collision. Active galaxies collide, feeding matter to the central black holes that power quasars
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Brown dwarf & debris ring from an oblique perspective - Artist's view of a brown dwarf star about 60 times the mass of Jupiter, surrounded by a disc of dust and rocks. In the foreground, a primitive exoplanet enlighted by the star. A small, barren planet orbits obliquely to the plane of a massive set of concentric dust rings surrounding a brown dwarf of about 60 Jupiter masses. These rings are evocative of Saturn's famous rings of rock and ice, however there is likely no ice in the rings around this dwarf. Recent observations have revealed that some brown dwarfs may be surrounded by rings of dust. While the origin of these rings, and the brown dwarfs themselves, is unclear, it's thought that material from these rings may even coalesce into planets, providing some brown dwarfs with their own solar systems
Huan disc, c.2400 BC (green nephrite)
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Ceremonial jade disc, c.100 B.C. (jade)
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Funerary stele, Meroitic Period, 2nd-3rd century AD (sandstone)
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Active galaxies in collision - Artist view - Active galaxies collide - Artist view - Artist view of a quasar whose jet is powered by the material of a galaxy rentree in collision. Intense jets of energy burst from the core of an active galaxy
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Pierced disc with four mice (nephrite)
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Still Life CD
Formation of a brown dwarf star - Artist's view - Formation of a brown dwarf star. Artwork - Brown dwarf star shines within its accretion disk. Streams of ionized dust and gas are drawn to the forming star by its magnetic field
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Ahuramazda in the Winged Disk, Persepolis, 486-460 BC (limestone)
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Central round of a disc "Gramophone" 78 turns
Circular disk (Bi), 1st century BC (nephrite)
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La formation d'une planete - Vue d'artiste - Forming solar system - Artist view: Vue d'artiste de planets à barely formed bombardees by comets. The early solar system was a maelstrom of violence as planetesimals collided with one another and with the forming planets
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Disk, end of the 3rd century BC (nephrite jade)
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Paul Young, 1983 (photo)
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Rear view of a Golok man and his wife, 1921 (glass plate gelatin print)
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Shock waves created by a supersonic T-38C
David Hasselhoff, 1989 (photo)
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Cayuse woman 1910 (photo)