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Meteorite fall, 1974
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The Destruction of Atlantis, illustration from 'Puissances Secretes', c.1935 (colour litho)
An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie
Space
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Tunguska valley - Artist view (2/3)
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Meteorites
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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
Tunguska meteorite damage
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Asteroids threatening the Earth - Artist view - Asteroids threaten to hit the Earth. Threatening asteroids going forward to impact Earth
Meteorites in the night sky
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An asteroid threatens the Earth - An asteroid threatens the Earth - Photomontage Composite image
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
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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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
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.
British Meteorites
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British Meteorites
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Meteorites, illustration
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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
Meteorolites and meteorites
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British Meteorites
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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)
Leonid Meteor Shower of 1833, USA, Illustration
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
Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity. Orbiting 14,600 miles above Mars' surface, Deimos completes one revolution every 30 hours
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
Leonids meteor shower (over England) July 2015.
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
The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays produce about 1,300 watts for probe's propulsion and other electrical systems. While no close - up observations of yet been made of Ceres itself, here it is rendered as appearing similar to a much smaller version of the Earth's Moon, heavily cratered with the addition of surface water ice and hypothesized plumes of ice crystals from water geysers on its surface
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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Balloon - Meteor Shower
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Quadruple bolide meteorites
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Tunguska meteorite damage
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Tunguska valley - Artist view (3/3)
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Shooting star rain on LAMOST telescope - China - Geminids over LAMOST telescope - China: Geminides shooting star rain above LAMOST telescope (Large Sky Area Multi-Object Fibre Spectroscopic Telescope), a 4-metre optical telescope, located on the site of the Xinglong Observatory in the Hebei region of China. December 2015. Space dust from asteroid 3200 Phaethon rained into the Earth's atmosphere, and burnt as meteors at about 100 km above Xinglong Station of National Astronomical Observatories of China, piercing the night sky over the Guoshoujing LAMOST telescope. All meteors seemed to radiate from the same point, which lies at Gemini, and that's how the meteor shower named Geminids.Over 100 meteors were captured in the composed image taken on the peak night of the 2015 Geminid meteor shower, and the brightest bolide even instantly lit up the landscape.
An asteroid threatens the artist's Earth-View - Asteroid threatening the Earth - Artist vie
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
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
WHEN METEORITES CRASH
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Inhabited mission to an asteroid - Artist's view - MMV begins descent to asteroid surface - An MMV, pilot by an astronaut, leaves his ship to descend to the surface of the asteroid. The Multi-Purpose Crew Vehicle (MPCV) should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehicle is connected to an additional housing module for a duration of more than three months, as well as to a module for extravehicular outputs equipped with two MVs (Manned Maneuvering Vehicles). The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. A Manned Maneuvering Vehicle (MMV) piloted by a single astronaut prepares to descend to the surface of a small asteroid
Le Soleil vu d'un asteroid - Viewing Artist - Sun seen from an asteroid
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Impact of asteroides on Earth - Asteroids impacting the Earth- Artwork - Artist's view
Meteor Crater - Arizona - USA - Anaglyph - Meteor Crater - Arizona - USA - Anaglyph - Impact Crater Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. It was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m. Anaglyph image, use 3D Eyeglasse
Artist impression of Oumuamua
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An asteroid threatens the Earth - Artist's view - Asteroid threatening the Earth - Artist vie
Gibeon meteorite, Gibeon, Great Nama Land, Namibia (iron, fine octahedrite)
Inhabited mission to an asteroid - Artist's view - MMV departs for asteroid surface - This capsule should be able to take a crew of six astronauts to an asteroid, the Moon or to take men to Mars. Here, the vehicle is connected to an additional housing module for a duration of more than three months, as well as to a module for extravehicular outputs equipped with two MVs (Manned Maneuvering Vehicles). One of the MVs, pilot by an astronaut, leaves the ship and descends to the surface of the asteroid. The Multi-Purpose Crew Vehicle (MPCV) is a spacecraft project currently being developed by Lockheed Martin for NASA. Based on specifications and tests already performed for the Orion spacecraft. It was announced by NASA on 24 May 2011. A Manned Maneuvering Vehicle (MMV) piloted by a single astronaut undocks from the main vessel and prepares to descend to the surface of a small asteroid
Etoile filante -Perseide - Perseid meteor - Rain d'étoiles filantes vue le 12/08/2008. Perseid meteor seem to radiate out of the same point in the constellation of Perseus in this composite exposure taken on August 12, 2008 during the Perseid Meteor Shower. The Perseids are tiny bits of dust left behind by Comet Swift-Tuttle on one of its day's through the Solar system. Although the comet is now far away, the dust left behind stays in orbit around the Sun, and sometimes the Earth passes through this dust trail, causing a meteor shower. The colors in the meteor's path come from different emissions as the meteor, speeding at 132,000 miles per hour, burns up and interacts with molecules in the upper atmosphere
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
A meteor shower of 103 BC
An asteroid threatens the Earth - An asteroid threatens the Earth - Illustration
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A large Gibeon meteorite slice, Gibeon, Great Nama Land, Namibia (iron, fine octahedrite)
Asteroids rush on Earth - Asteroids threaten the Eart
Impact of an asteroid on Earth - Asteroid impact on Earth- Artwor
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””
Aguas Zarcas CM2 Meteorite - Into the Doghouse (carbonaceous chondrite)
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