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'Asteroid' images and/or videos results page 1 of 5

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An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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An asteroid threatens the Earth - An asteroid threatens the Earth - Photomontage Composite image
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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Asteroide Vesta and other asteroides - Asteroid Vesta compared to other asteroids - Comparison of the sizes of the nine asteroides visits to date by space probes. The asteroid Vesta, with a diameter of 530 km, is the largest. This composite image shows the comparative sizes of nine asteroids. Up until now, Lutetia, with a diameter of 81 miles (130 kilometers), was the largest asteroid visited by a spacecraft, which occurred during a flyby. Vesta, which is also considered a protoplanet because it's a large body that almost became a planet, dwarfs all other small bodies in this image, with its diameter sizing up at approximately 330 miles (530 kilometers)
Tunguska valley - Artist view (2/3)
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The probes Osiris-Rex and Hayabusa 2 - Artist's view - Osiris-rex and Hayabusa 2 - Artwork: Artist's view of the probe Osiris-Rex near the asteroid Bennu (right) and the probe Hayabusa 2 near the asteroid (162173) Ryugu (upper left). OSIRIS-REX was launched on 8 September 2016 to reach the asteroid Bennu in 2018 and bring a sample back to Earth in 2023. Hayabusa 2 is a space probe of JAXA, the Japanese space agency, launched in December 2014, which will study the asteroid (162173) Ryugu from July 2018 to February 2019 and bring a sample to Earth in December 2020. Osiris-rex will travel to a near-earth asteroid called Bennu and bring a small sample back to Earth for study. It was launched on Sep 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023. Hayabusa2 is an asteroid sample return mission operated by the Japanese space agency, JAXA. Launched in December 2014 Hayabusa 2 is expected to arrive at the asteroid 162173 Ryugu in July 2018, survey the asteroid for a year and a half, depart in December 2019, and return to Earth in December 2020
Artist's view of the asteroid 2017 YE5 - Binary Asteroid 2017 YE5 - 2017 YE5 is a binary asteroid consisting of two asteroids of same sizes orbit each other.
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor
Artist view of an asteroid - Asteroid - Artwor
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Earth at the end of Permian - Ring arcs over the Permian Earth - A ring of rocks and dust is orbiting the Earth. The massive continent below is Pangee and the ocean to the west is Panthalassa. This is what Earth was supposed to look like at the end of Permian, about 260 million years ago, before the first dinosaurs appeared. This ring around the Earth was of earthly origin, constitutes debris thrown into orbit by collision with a meteorite or comet. Over time, these debris have either fallen or fallen back to Earth in a meteorite rain. A dusty ring arc orbits four thousand miles above Earth's equator. The massive continent below is Pangea and the ocean to the west is Panthalassa. This is how the Earth may have appeared during the end of the Permian period, a time just prior to the appearance of the dinosaurs, when continental drift was pulling Pangea apart into the seven continents we know today. 260 million years ago the Earth may have been host to ring arcs similar to the incomplete rings that currently circumscribe the planet Neptune. Unlike Neptune's rings, the ring arcs around the Earth were of terrestrial origin, debris thrown into orbit by a collision with a large meteorite or comet. The debris consisted of tiny pebbles that were once molten droplets of ejecta, long since cooled in the vacuum of space. The orbit of the ring arc would eventually decay, returning the debris back to Earth as a shower of meteorites. This debris is found on Earth's surface today in the form of dark, glassy objects known as tektites
Asteroids threatening the Earth - Artist view - Asteroids threaten to hit the Earth. Threatening asteroids going forward to impact Earth
Artist view of asteroid 216 Kleopatra: (216) Cleopatre (216 Kleopatra) is an asteroid of the main belt. 216 Kleopatra is an asteroid orbiting in the asteroid belt
The asteroid belt - The asteroid belt- Artwork - Artist's view of the asteroid belt, or main belt, located between the orbit of Mars and that of Jupiter. Artist view of the asteroid belt located between Mars and Jupiter orbits
The Osiris-Rex probe and the Bennu asteroid - Artist's view - OSIRIS-REx near asteroid Bennu - Artwork: Artist's view of the Osiris-Rex probe near the Asteroid Bennu - OSIRIS-REx is to be launched on September 8, 2016 to reach the Asteroid Bennu in 2018 and bring a sample back to Earth in 2023 - OSiRIS-Osiris-Osiris-Osiris-Osiris-Rex in 2023 Ris-rex will travel to a near-earth asteroid called Bennu and bring a small sample back to Earth for study. The mission is scheduled to launch Sep 8, 2016. As planned, the spacecraft will reach its asteroid target in 2018 and return a sample to Earth in 2023
An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie
Astronauts on an asteroid - Artist's view - Asteroid explorers: Astronauts explore the surface of an asteroid
An asteroid threatens the Earth - Artist's view - Asteroid threatening the Earth - Artist vie
Asteroides threaten the Earth - Artist view - Asteroids threatening the Earth - Artist view - Title: Space Situational Awareness - Near Earth Objects Picture caption: The SSA-NEO system is based on syndicating and federating observation and tracking data provided by a large number of European and international sources. The key components include: -Observatories and astronomers with telescopes of various sizes, both professional and amateur -A central SSA-NEO data centre, the 'Small Bodies Data Centre', which uses astrometric measurements collected by the Minor Planet Center (USA) -An analysis capability to predict possible impact locations and assess dangers -Analyses related to risk mitigation, including the possible deflection of an asteroid -A system for issuing warnings and alerts to civil authorities in Europe Data on NeOS are collected from telescopes and radar systems worldwide. Each of these submit observations to the Minor Planet Center (MPC), operated by the International Astronomical Union (IAU) at Cambridge, Massachusetts, USA, which acts as a central clearing house for asteroid and comet observations. The measurements collected there are retrieved by the European Small Bodies Data Centre; orbits and miss distances are computed. In case of high-risk impact predictions, the data will be cross-checked with NASA's SENTRY system, operated by the Jet Propulsion Laboratory (JPL), California, before issuing alerts
Mine sur un asteroide - Illustration - Mining base on double asteroid 90 Antiope - Illustration - Artist view une base minere installee sur l'asteroid double 90 Antiope. Some day a it may be worthwhile to mine resources from a distant asteroid, whether for raw materials for building an orbiting structure (cheaper than rocketing the materials from Earth's surface) or for some exotic material found only on a particular asteroid. This image is a bird's eye view of a mining settlement on the double asteroid 90 Antiope, located in the main asteroid belt between the orbits of Mars and Jupiter. These two asteroids are about the same size - - 70 miles across - - and orbit around a common center like two ends of a barbell. The gap separating the two bodies is only about 40 miles. The extremely low surface gravity would permit the construction of delicate structures, such as the solar power array silhouetted against the sunny side of the sister asteroid, and would make it relatively easy to transport mined material off the surface
Le Soleil vu d'un asteroid - Viewing Artist - Sun seen from an asteroid
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Asteroid 951 Gaspra
The disappearance of dinosaurs - Artist view - Tylosaur and KT Event - Artist view - Impact of the asteroid responsible for the disappearance of dinosaurs about 65 million years ago. In the foreground, a tylosaurus, a large carnivorous marine lezard. The very end of the Mesozoic is marked by evidence of a devastating asteroid impact 65 million years ago, which is termed the KT event, referring to the Cretaceous (K) -Tertiary (T) transition. This impact likely contributed to the demise of the dinosaurs, although recent findings call into question how decisive the blow actually was. In this image, a huge tylosaur, a relative of today's varanid lizards such as the Komodo dragon, faces its last few minutes of existence in a Texas lagoon. Over the horizon looms the rising ejecta from the KT impact, which occurred in what is today the Yucatan
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor
Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view
Base on an asteroid - Illustration - Base on an asteroid surface - Illustratio
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Asteroid distribution
Asteroid Bennu
Tunguska valley - Artist view (3/3)
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Asteroide Ida seen by Galileo probe - Asteroid Ida seen by Galileo spacecraft - Mosaic of five images obtained by the Galileo probe on 28 August 1993 between 3000 and 3800 km from the asteroid. This view of the asteroid 243 Ida is a mosaic of five image frames acquired by the Galileo spacecraft's solid-state imaging system at ranges of 3,057 to 3,821 kilometers (1,900 to 2,375 miles) on August 28, 1993. Ida is the second asteroid ever encountered by a spacecraft. It appears to be about 52 kilometers (32 miles) in length, more than twice as large as Gaspra, the first asteroid observed by Galileo in October 1991
Based on an asteroid-Artist's view - Base on an asteroid - Illustratio
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An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor
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Illustration of a triple system of asteroids - Triple system of asteroids -Artwork - Artist's view of two small asteroids (Romulus and Remus) orbiting asteroid 87 Sylvia. Sylvia is about 380 km long and is one of the largest members of the asteroid belt. Two small asteroids are orbiting a larger one known since 1866 as 87 Sylvia. Sylvia is measuring 380 x 260 x 230 km; its moons are considerably smaller, orbiting in nearly circular orbits and in the same plane and direction. The closest and newly discovered moonlet, orbiting about 710 km from Sylvia, is Remus, a body only 7 km across and circling Sylvia every 33 hours. The second, Romulus, orbits at about 1360 km in 87.6 hours and measures about 18 km across. The asteroid 87 Sylvia is one of the largest known from the asteroid main belt, and is located about 3.5 times further away from the Sun than the Earth, between the orbits of Mars and Jupiter
Asteroide Vesta seen by the Hubble Space Telescope - Asteroid Vesta - Photo obtained in visible view of the Vesta asteroid in May 1996 by the Hubble Space Telescope. The images reveal a huge impact crater 450 km in diameter south of the asteroid; the original image is at the top left, modeled in 3D on the right. Astronomers have used the Hubble Space telescope to discover a giant impact crater on the asteroid Vesta. <BR>Left is a Hubble Space Telescope image of the asteroid Vesta, taken in May 1996 when the asteroid was 110 million miles from Earth. The asymmetry of the asteroid and “” nub”” and the south pole is suggestive that it suffered a large impact event. Center is a color-encoded elevation map of Vesta that clearly shows the giant 285- mile diameter impact basin and “” bull 's-eye”” central peak. Right is a 3-D computer model of the asteroid Vesta synthesized from Hubble topographic data. The crater's 8-mile high central peak can clearly be seen near the pole. At the bottom an elevation map has been reconstructed and clearly shows in blue the large impact basin and its central peak (in red)
An asteroid is on Mercury
Mission to an asteroid
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Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure
Artist's view of the asteroid 2060 Chiron: (2060) Chiron, also designed as 95P/Chiron, is a centaur type cometary asteroid, an ice body of 166 kilometres of diameter orbiting around the Sun between Saturn and Uranus. 2060 Chiron, also known as 95P/Chiron, is a minor planet in the outer Solar System, orbiting the Sun between Saturn and Uranus. Discovered in 1977 it was the first-identified member of a new class of objects now known as centaurs - bodies orbiting between the asteroid belt and the Kuiper belt. Besides the four giant planets, Chiron and 10199 Chariklo, also a centaur, are the only other bodies in the Solar System known to have rings. Although it was initially called an asteroid and classified only as a minor planet with the designation “” 2060 Chiron””, it was later found to exhibit behavior typical of a comet. Today it is classified as both a minor planet and a comet, and is accordingly also known by the cometary designation “” 95P/Chiron””
A geocroiser asteroid passes Jupiter's orbit, 2016 (photo)
Asteroides - Artist view
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Tunguska Event - Artist View - Tunguska Event - Artist view - On June 30, 1908, a car, several ten meters in diameter, exploded over the Tunguska region of Siberia. 2000 km of forest and taiga were destroyed, blown by the shock wave of the car. The explosion was heard up to 1500 km. Just after seven in the morning of June 30, 1908 a huge fireball appeared over the region, and detonated as it hit the upper atmosphere. The explosion broke windows over 500 miles away. There were some herdsmen and hunters in the area at the time who were able to provide eyewitness accounts of what became known as the Tunguska Event. Many would later die from what appears to have been radiation exposure
Asteroides Ceres and Vesta seen by the Hubble space telescope - Asteroids Ceres and Vesta seen by the Hubble space telescope - Ceres and Vesta are the two largest bodies of the asteroid belt, a region located between Mars and Jupiter. Since August 2006, Ceres is considered a dwarf planet. Ceres (left) has a diameter of about 950 km. Image obtained in January 2004. The image on the right, obtained on 14 and 16 May 2007, shows the asteroid Vesta. Its diameter is about 530 km. These Hubble Space Telescope images of Vesta and Ceres show two of the most massive asteroids in the asteroid belt, a region between Mars and Jupiter. At least 100,000 asteroids inhabit the asteroid belt, a reservoir of leftover material from the formation of our solar-system planets 4.6 billion years ago. The International Astronomical Union named Ceres one of three dwarf planets in 2006. Ceres is round like planets in our solar system, but it does not clear debris out of its orbit as our planets do. The image at right was taken on May 14 and 16, 2007. Using Hubble, astronomers mapped Vesta's southern hemisphere, a region dominated by a giant impact crater formed by a collision billions of years ago. The crater is 285 miles (456 kilometers) across, which is almost equal to Vesta's 330-mile (530-kilometer) diameter. The Hubble image of Ceres on the left, taken on January 2004, reveals bright and dark regions on the asteroid's surface that could be topographic features, such as craters, and/or areas containing different surface material. Ceres has a diameter of approximately 950 kilometers
Brown dwarf with asteroid ring - Artist's view of a brown dwarf star surrounded by an asteroid belt. In the foreground, a primitive exoplanet illuminated by the star. This brown dwarf is host to a disk composed primarily of asteroids and boulders. The light from this dwarf is barely enough to illuminate the surface of this primitive planet. At a distance of about 1.5 million miles, the orbit of this planet is aligned to the plane of the rings with the result that they appear as a fuzzy line occulting the glowing face of this brown dwarf
Artist's impression of the asteroid Oumuamua
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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
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
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwork - Artist view
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A celeste body disloque - Artist view - Celestial body collapsed by tidal force - Artist vie
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Asteroid Colliding (illustration)
Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings
Vue d'artiste de l'asteroid 1036 Ganymede - Artist impression of the asteroid 1036 Ganymed near Mars: Vue d'artiste de l'asteroid 1036 Ganymede passing near Mars. It is the largest of the Amor asteroids, its average diameter reaches 31.7 km. 1036 Ganymed is the largest near-earth asteroid, at about 32-34 km in diameter. It was discovered by Walter Baade on October 23, 1924. It has a very well determined orbit, and its next pass of the Earth will be on 13 October 2024. It is an Amor asteroid, and also a Mars-crosser asteroid, and will pass March on 16 December 2176
Le Soleil vu d'un asteroid - Viewing Artist - Sun seen from an asteroid
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Asteroid belts around the star Epsilon Eridani - Asteroid belts around Epsilon Eridani - Artist's view of the planetary system around the star Epsilon Eridani. This star is located 10 years from Earth. Observations made by the Spitzer space telescope in 2008 show that this system has two asteroid belts. An exoplanet had already been discovered around this star in 2000. This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Observations from Nasa's Spitzer Space Telescope show that the system hosts two asteroid belts, in addition to previously identified candidate planets and an outer comet ring. Epsilon Eridani is located about 10 light - years away in the constellation Eridani. It is visible in the night skies with the naked eye. The system's inner asteroid belt appears as the yellowish ring around the star, while the outer asteroid belt is in the foreground. The outermost comet ring is too far out to be seen in this view, but comets originating from it are shown in the upper right corner. Astronomers think that each of Epsilon Eridani's asteroid belts could have a planet orbiting just outside it, shepherding its rocky debris into a ring in the same way that Jupiter helps keep our asteroid belt confined. The planet near the inner belt was previously identified in 2000 via the radial velocity, or “” star wobble,”” technique, while the planet near the outer belt was inferred when Spitzer discovered the belt. The inner belt orbits at a distance of about 3 astronomical units from its star - - or about the same position as the asteroid belt in our own solar system (an astronomical unit is the distance between Earth and our sun). The second asteroid belt lies at about 20 astronomical units from the star, or a position comparable to Uranus in our solar system. The outer comet ring orbits from 35 to 90 astronomical units from the star; our solar system's analogous Kuipe
Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets
Artist's view of the asteroid 10199 Chariklo - Artist impression of asteroid 10199 Chariklo: (10199) Chariklo, is a centaur, an asteroid whose orbit crosses that of the outer planets of the solar system. Discovered on 15 February 1997 by the Spacewatch program, it is the first known asteroid with rings. 10199 Chariklo is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chui), around Chariklo by observing a stellar occultation making it the first known minor planet to have rings
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwork - Artist view
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The Dawn probe near Vesta - Artist's view: Artist's view of the Dawn probe near the Vesta asteroid. On 16 July 2011 the probe went into orbit around Vesta and collected data that significantly improved our knowledge of asteroid. After studying Vesta for more than a year, the probe left on 5 September 2012 to reach the dwarf planet Ceres. Artist's concept of the Dawn spacecraft with asteroid Vesta. Dawn, part of Nasa's Discovery Program of competitively selected missions, was launched in 2007 to orbit the large asteroid Vesta (2011-2012) and the dwarf planet Ceres (2015).
Artist's view of the asteroid Lutetia - Artist impression of the asteroid Lutetia - Artist's view of the asteroid Lutetia passing by a rocky planet 4 billion years ago. This artist's impression shows an event in the early history of the Solar System that may explain how the unusual asteroid Lutetia came to now be located in the main asteroid belt, between Mars and Jupiter. Lutetia is seen passing close to one of the very young rocky planets about four billion years ago and having its orbit drastically altered. Its unusual spectral properties indicate that Lutetia started life as a fragment of the material that was forming the inner planets but it is now found to be an interloper much further from the Sun
Surface de Ceres - Ceres ice field: Ice surface of the dwarf planet Ceres. Artist view
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Artist's View of Ceres Degazages - Outgassing on Ceres: Artist's View of the Dwarf Planet Ceres with Panaches of Water Vapour
Asteroid Colliding (illustration)
Asteroid Colliding (illustration)