Posted on by Nancy Atkinson

More Chunks of SUV-Smashing Meteorite Found

Grimsby homeowner Yvonne Garchinski and Western Physics and Astronomy associate professor Peter Brown speak to national media where a 4.6-billion-year-old meterorite smashed the window of Garchinski's truck Sept. 25. The pair are wearing gloves to protect the meteorite.


Three golf ball-sized fragments have been found from a meteorite that created a brilliant fireball seen over Ontario, Canada on September 25, 2009. The first meteorite fragment recovered did some damage to the windshield of a Nissan Pathfinder, and now two other fragments have been found on nearby properties. The meteor made headlines initially because it was captured on video by Western’s Southern Ontario Meteor Network (SOMN) on seven of its ‘all-sky’ cameras. The brightness was estimated to be approximately 100 times brighter than a full moon.

Initially, the owners of the SUV didn’t realize the “unusual” rock they found on the hood of the vehicle was a meteorite and chalked up the shattered windshield to vandalism and filed a police report.
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Tony Garchinski said heard a loud crash just after 9 p.m. the night of the meteor flyby he didn’t think much of it. That is, until he awoke the next morning to find the windshield of his mom’s truck with a huge crack in it.

It wasn’t until two weeks later that his mother, Yvonne Garchinski, heard media reports that researchers from Western were searching West Grimsby, Ontario for possible fragments of a freshly fallen meteorite. The Garchinskis realized who the real culprit was in the case of the broken windshield — or more specifically, what.

The ‘what’ was a 46-gram completely fusion-crusted (melted exterior) fragment of an ordinary chondrite meteorite. Chondrites are arguably the most important type of meteorite because they are the least processed of meteorites and provide a window into the material which formed the early solar system. The meteorite is estimated to be 4.6 billion years old.

Phil McCausland, a postdoctoral fellow at Western’s Centre for Planetary Science & Exploration said, “Having both the video and the sample is golden because we get the dynamic information and the orbital direction from the video, and by having recovered material on the ground, we can complete the picture. We can take a rock that we now have in hand and we can study it in the best laboratories in the world and we can put it back into its solar system context. We can put it back into where it came from.”

The Garchinski property is just 200 meters off the fall line of the meteorite the Western Meteor Physics Group calculated using data from its video, radar and sound detection systems and thanks in large part to this research – along with a lot of luck – two more meteorite fragments have been found.

The second meteorite was found by the Western team not far from the Garchinski home but the land owner wishes to remain anonymous. The third fragment was found Oct. 18 by professional meteorite hunter Mike Farmer (www.meteoriteguy.com) on the side of a road in West Grimsby.

The Western-led search continues and both Brown and McCausland believe more fragments will be found.

Source: Western University

Posted on by Nancy Atkinson

Pictures and Videos Capture Canadian Fireball from Sept. 25, 2009

Composite all-sky camera image of the end of the fireball as seen from Hamilton (Camera #3, McMaster). Available below are movies of the event as seen by several of the SOMN cameras, as well as animations of the object's arrival at Earth. Credit: University of Western Ontario

A brilliant fireball seen over Ontario, Canada on September 25, 2009 was captured by seven all-sky cameras of the University of Western Ontario’s Southern Ontario Meteor Network (SOMN.) The fireball was seen widely by observers throughout southern Ontario and adjacent areas. The fireball was first detected by Western’s camera systems at an altitude of 100km, and moving southeastwards at 20.8 km/s. From the data collected, the researchers believe the meteoroid was initially about a meter wide, or about the size of a child’s tricycle. At its brightest, the fireball was approximately 100 times as bright as the full moon.

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Researchers at Western are interested in hearing from anyone within 10 km of Grimsby, Ontario who may have witnessed or recorded this evening event, seen or heard unusual events at the time, or who may have found possible fragments of the freshly fallen meteorite.

The event occurred at 9:03 pm local time on Sept. 25, or 01:03 UT Sept. 26.

Analysis of the all-sky camera records as well as data from Western’s meteor radar and infrasound equipment indicates that this bright fireball was large enough to have dropped meteorites in a region south of Grimsby on the Niagara Peninsula, providing masses that may total as much as several kilograms.

To see more videos or images, or if you have questions, observations or possible meteorites check out Western’s website.

Posted on by Nancy Atkinson

Understanding 2008 TC3 a Year After Impact

Discovery images of asteroid 2008 TC3, as it was seen on October 6, 2008, by the Catalina Sky Survey at Mount Lemmon in Arizona (Richard Kowalski).

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The first asteroid to have been spotted before hitting Earth, 2008 TC3, crashed in northern Sudan one year ago on October 6. Several astronomers have been trying to piece together a profile of this asteroid, pulling together information from meteorites found at the impact site and the images captured of the object in the hours before it crashed to Earth.

“We have a gigantic jigsaw puzzle on our hands, from which we try to create a picture of the asteroid and its origins,” said SETI Institute astronomer Peter Jenniskens, who worked at the crash site, “and now we have with a composite sketch of the culprit, cleverly using the eyewitness accounts of astronomers that saw the asteroid sneak up on us.” Their description? 2008 TC3 looked like a loaf of walnut-raisin bread.

“The asteroid now has a face,” said Jenniskens, chair of the special session at the fall meeting for the Division for Planetary Sciences of the American Astronomical Society. Last December, Jenniskens and Sudan astronomer Muawia Shaddad went to the crash site and recovered 300 fragments in the Nubian Desert. Like detectives, students from the University of Khartoum helped sweep the desert to look for remains of the asteroid. They found many different-looking meteorites close to, but a little south, of the calculated impact trajectory.

The team has also been able to recreate the shape of the asteroid from looking at images captured by Astronomers Marek Kozubal and Ron Dantowitz of the Clay Center Observatory in Brookline, Massachusetts, who tracked the asteroid with a telescope and captured the flicker of light during a two hour period just before impact.

An irregular shape and rapid tumbling caused asteroid 2008 TC3 to flicker when it reflected sunlight on approach to Earth.

Peter Scheirich and colleagues at Ondrejov Observatory and Charles University in the Czech Republic combined all the various observations to work out the shape and orientation of the asteroid.

Watch a video recreation of 2008 TC3 tumbling in space.

Larger version. (1.32 MB Mpeg 4 file)

Video of 2008 TC3 as seen through a telescope (large file, 7.63 MB)

Other forensic evidence based on analysis of the recovered meteorites at the Almahata Sitta site showed the asteroid was an unusual “polymict ureilite” type. Jason S. Herrin of NASA’s Johnson Space Center confirmed that the meteorites still carry traces of being heated to 1150-1300 degrees C, before rapidly cooling down at a rate of tens of degrees C per hour, during which carbon in the asteroid turned part of the olivine mineral iron into metallic iron. Hence, asteroid 2008 TC3 is the remains of a minor planet that endured massive collisions billions of years ago, melting some of the minerals, but not all, before a final collision shattered the planet into asteroids.

Mike Zolensky of NASA’s Johnson Space Center first pointed out that, as far as ureilites are concerned, his meteorite is unusually rich in pores, with pore walls coated by crystals of the mineral olivine. He now reports, from X-ray tomography work with Jon Friedrich of Fordham University in New York, that those pores appear to outline grains that have been incompletely welded together and that the pore linings appear to be vapor phase deposits. According to Zolensky, “Almahata Sitta may represent an agglomeration of coarse- to fine-grained, incompletely reduced pellets formed during impact, and subsequently welded together at high temperature.”

The carbon in the recovered meteorites is among the most cooked of all known meteorites. Carbon crystals of graphite and nanodiamonds have been detected. Still, it turns out that some of the organic matter in the original material survived the heating. Amy Morrow, Hassan Sabbah, and Richard Zare of Stanford University have found polycyclic aromatic hydrocarbons in high abundances. Amazingly, Michael Callahan and colleagues of NASA’s Goddard Space Flight Center now report that even some amino acids have survived.

Jenniskens and Shaddad plan to revisit the scene of the crash in the Nubian Desert. They reported their findings at the Division for Planetary Sciences of the American Astronomical Society meeting in Puerto Rico.

Listen to Oct. 6th’s 365 Days of Astronomy podcast by Emily Lakdawalla about 2008 TC3.

Source: AAS Planetary Science Division

Posted on by Nancy Atkinson

Opportunity Finds Another Big Meteorite

Another Mars meteorite seen by Opportunity. Image Credit: NASA/JPL-Caltech

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It’s amazing what a rover can find laying by the side of the road. The Mars Exploration Rover Opportunity has found a rock that apparently is another meteorite. Less than three weeks ago, Opportunity drove away from a larger meteorite called “Block Island” that the rover examined for six weeks. Now, this new meteorite, dubbed “Shelter Island,” is another fairly big rock, about 47 centimeters (18.8 inches) long, that fell from the skies. Block Island is about 60 centimeters (2 feet) across and was just 700 meters (about 2,300 feet) away from this latest meteorite find. At first look, the two meteorites look to be of a similar makeup; Opportunity found that Block Island was is made of nickel and iron.

This image was taken during Oppy’s 2,022nd Martian day, or sol, (Oct. 1, 2009).

See below for a 3-D version of this image created by Stu Atkinson.

Shelter Island in 3-D. Dimensionalized by Stu Atkinson
Shelter Island in 3-D. Dimensionalized by Stu Atkinson

Posted on by Anne Minard

Heat-Shocked Diamonds Provide New Clue of Horse-Killing Impact

California's Channel Islands, where heat-shocked soot and diamonds are suggesting a killing comsic impact. Courtesy NOAA and UC Santa Barbara

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Archeologists have been divided about whether an extraterrestiral impact blasted North America about 12,900 years ago, wreaking havoc on Earth’s surface and sending scores of species — including a pygmy mammoth and the horse — into oblivion.

New clues from California’s Channel Islands should put any doubt to rest, says an international team of researchers.

This transmission electron microscopy close-up shows a single lonsdaleite crystal, left, and associated diffraction pattern. Credit: University of Oregon
This transmission electron microscopy close-up shows a single lonsdaleite crystal, left, and associated diffraction pattern. Credit: University of Oregon

The 17-member team, led by University of Oregon archaeologist Douglas J. Kennett, has found what may be the smoking gun.

The team has found shock-synthesized hexagonal diamonds in 12,900-year-old sediments on the Northern Channel Islands off the southern California coast.

The tiny diamonds and diamond clusters were buried deeply below four meters (13 feet) of sediment. They date to the end of Clovis — a Paleoindian culture long thought to be North America’s first human inhabitants. The nano-sized diamonds were pulled from Arlington Canyon on the island of Santa Rosa, which had once been joined with three other Northern Channel Islands in a landmass known as Santarosae.

The diamonds were found in association with soot that forms in extremely hot fires, and they suggest associated regional wildfires, based on nearby environmental records.

Such soot and diamonds are rare in the geological record. They were found in sediment dating to massive asteroid impacts 65 million years ago in a layer widely known as the K-T Boundary. The thin layer of iridium-and-quartz-rich sediment dates to the transition of the Cretaceous and Tertiary periods, which mark the end of the Mesozoic Era and the beginning of the Cenozoic Era.

“The type of diamond we have found — Lonsdaleite — is a shock-synthesized mineral defined by its hexagonal crystalline structure. It forms under very high temperatures and pressures consistent with a cosmic impact,” Kennett said. “These diamonds have only been found thus far in meteorites and impact craters on Earth and appear to be the strongest indicator yet of a significant cosmic impact [during Clovis].”

The age of this event also matches the extinction of the pygmy mammoth on the Northern Channel Islands, as well as numerous other North American mammals, including the horse, which Europeans later reintroduced. In all, an estimated 35 mammal and 19 bird genera became extinct near the end of the Pleistocene with some of them occurring very close in time to the proposed cosmic impact, first reported in October 2007 in PNAS.

Source: University of Oregon, via Eurekalert. The results appear in a paper online ahead of print in the Proceedings of the National Academy of Sciences.

Posted on by Nancy Atkinson

Meteorite May Hold Clues to Solar System Formation

Philipp Heck with the Allende Meteorite. Credit: Dan Dry

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Maybe we’re not as old as we think (or feel?). The interstellar stuff that was integrated into the planets and life on Earth has younger cosmic roots than theories predict, according to the University of Chicago scholar Philipp Heck and his international team of colleagues.

Heck’s team analyzed 22 interstellar grains from the Murchison meteorite. Dying sun-like stars flung the Murchison grains into space more than 4.5 billion years ago, before the birth of the solar system. Scientists know the grains formed outside the solar system because of their exotic composition.

“The concentration of neon, produced during cosmic-ray irradiation, allows us to determine the time a grain has spent in interstellar space,” Heck said. His team determined that 17 of the grains spent somewhere between three million and 200 million years in interstellar space, far less than the theoretical estimates of approximately 500 million years. Only three grains met interstellar duration expectations (two grains yielded no reliable age).

“The knowledge of this lifetime is essential for an improved understanding of interstellar processes, and to better contain the timing of formation processes of the solar system,” Heck said. A period of intense star formation that preceded the sun’s birth may have produced large quantities of dust, thus accounting for the timing discrepancy, according to the research team.

Abstract

Source: EurekAlert

Posted on by Nancy Atkinson

Scientist Claims UFO Collided with Tunguska Meteorite to Save Earth

Supposedly, the Tunguska crytals. Credit: Mina

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Classify this under news of the weird. A Russian scientist claims that aliens downed the Tunguska meteorite 101 years ago to protect our planet from devastation. Yuri Lavbin says he found unusual quartz crystals at the site of the massive Siberian explosion. Ten crystals have holes in them, placed so the stones can be united in a chain, and other have drawings on them. “We don’t have any technologies that can print such kind of drawings on crystals,” said Lavbin. “We also found ferrum silicate that can not be produced anywhere, except in space.”

OK, just a few holes in this story, too.

Photograph from the Soviet Academy of Science 1927 expedition led by Leonid Kulik
Photograph from the Soviet Academy of Science 1927 expedition led by Leonid Kulik

The Tunguska Event was a powerful explosion that occurred in an uninhabited and desolate area near the Tunguska River in Russia, on June 30, 1908. Although the cause of the explosion is the subject of debate, it is commonly believed to have been caused by the explosion of a large meteoroid or comet fragment, occurring the in Earth’s atmosphere about 5–10 kilometers (3–6 miles) high. The blast flattened an estimated 60 million trees over 2,150 square kilometers, but no crater or “smoking gun” meteorite has ever been found. Different studies have yielded varying estimates of the object’s size, but there is general agreement that it was a few tens of meters across.

A couple of expeditions have gone to the remote site of the crash. Lavbin says that one expedition located the unusual crystals.

While I’m not a chemist, I couldn’t find any information on “ferrum silicate.” Seemingly, it doesn’t exist.

One small, nondescript photo accompanied Lavbin’s claims, published by the Macedonian International News Agency.

This isn’t the first time a UFO has been claimed to associated with the Tunguska event. Another report from 2004 said a scientific expedition to the site found blocks of an extraterrestrial technical device, and one 50-kilogram piece of the stone was brought to the city of Krasnoyarsk to be studied and analyzed. No subsequent reports or analysis could be located during an internet search.

Other claims of exploding alien spaceships or alien weapons detonating to “save the Earth from an imminent threat” appear to originate from a science fiction story “A Visitor From Outer Space” written by Soviet engineer Alexander Kazantsev in 1946, in which a nuclear-powered Martian spaceship, seeking fresh water from a lake blew up in mid-air. This story was was said to be inspired by Kazantsev’s visit to Hiroshima in late 1945.

Many events in Kazantsev’s tale were subsequently confused with the actual occurrences at Tunguska. A “reveal-all” book was published in 1976 (The Fire Came By) but was written by two television drama critics — so much for a scientific background. In 1998 the television series The Secret KGB UFO Files was broadcast on Turner Network Television, and referred to the Tunguska event as “the Russian Roswell” and claimed that crashed UFO debris had been recovered from the site.

However, not one proponent of the Tunguska/UFO hypothesis have ever been able to provide any significant evidence for their claims.

Lavbin says the stones, when put together form a map, and might be part of a navigational system of a spaceship.

But Lavbin says what proves his hypothesis is a strange portrait of a strange person on one of the stones.

Hmm, strange looking person on a stone….sounds like….pareidolia. Check out the Bad Astronomer’s take on that phenomenon.

Just as in any other UFO claim, this one fails to deliver any evidence.

Source: Mina

Posted on by Nancy Atkinson

Unusual Micrometeorite Found in Antarctica

Micrometeorite. Credit: Washington State University

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A miniature meteorite unlike any other has been discovered in Antarctica. The tiny rock, known as MM40, is the first achondritic basaltic micrometeorite ever found on Earth. Detailed analysis shows it has an unusual chemical composition the researchers say raises questions about where it originated in the Solar System and how it was created. “We have basaltic meteorites that are thought to come from an asteroid called 4 Vesta and we also have basaltic meteorites from the Moon and Mars,” said Dr. Caroline Smith, curator of meteorites at the Natural History Museum, London “But MM04’s chemistry does not match any of those places. It has to be from somewhere else.”


MM40 is only 150 microns across as its widest point, (.0059055 inches) or about as big as the period at the end of this sentence.

Chondritic meteorites were formed during the the Solar System’s early days before material had accreted into planets. They have not been altered by the melting and re-crystalisation that takes place during planetary formation and erosional forces similar to what Earth rocks undergo.

Achondritic meteorites, by contrast, were formed when the Solar System’s planets were coming into being. The substances in such meteorites and the processes they have undergone can give clues about how the larger bodies were formed.

The research team, led by Matthieu Gounelle from the Laboratory of Mineralogy and Cosmochemistry at the French Natural History Museum, says the discovery of this new type of basaltic meteorite expands the solar system inventory of planetary crusts. “The parent asteroid of MM40 has undergone extensive metamorphism,” the researchers write, “which ended no earlier than 7.9 million years after solar system formation. Numerical simulations of dust transport dynamics suggest that MM40 might originate from one of the recently discovered basaltic asteroids that are not members of the Vesta family.”

While its ultimate origins are a mystery it does have implications for the ways that astrochemists thought planets could be formed. The analysis of MM04 showed that the “inventory” of such processes must be expanded, said Dr. Smith.

“Micrometeorites are often seen as the ‘poor man’s space probe’,” she said. “They land on Earth fortuitously and we do not have to spend millions of dollars or euros on a robotic mission to get them.”

Sources: Proceedings from the National Academy of Sciences, BBC

Posted on by Nancy Atkinson

Changing Opinions: Fireball Likely Not Part of Soyuz Rocket

A meteor falls to Earth. Credit: Spaceweather.com

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Officials are now saying the bright fireball seen over Virginia in the US on Sunday was probably a natural meteor event and not part of a Russian rocket, a reversal from yesterday’s initial analysis. Space.com reported that an official from the U.S. Naval Observatory believed the loud boom and flash of light seen in the skies over Norfolk and Virginia Beach was likely the second stage of the Soyuz rocket that launched Expedition 19 to the International Space Station last Thursday. However, U.S. Strategic Command has since reported that the rocket re-entered Earth’s atmosphere near Taiwan, on the other side of the world, several hours after the reports of the fireball. So both its timing and entry location rule out the rocket as the explanation for the fireball. But the investigation is continuing to determine exactly what the object was.

The Joint Space Operations Center at Vandenberg Air Force Base in California also confirmed “the ‘bright light’ that was reported on the East Coast on Sunday, 29 March at 9:45 p.m. EST was not a result of any trackable manmade object on reentry,” according to Patricia Phillips at the Space News Examiner.

Space rocks the size of small cars plunge into Earth’s atmosphere several times a year, typically burning up before reaching the ground. “The atmosphere is very good at protecting us from falling rocks,” said Bill Cooke of NASA’s Marshall Space Flight Center. Ones that do reach the ground go unreported since they fall over uninhabited areas or in the ocean.

A few space rocks do occasionally make it to the surface though. In recent years, pieces of a bolide were found after a meteor event in western Canada, and fragments of a meteor that originated from an asteroid that blew up over the skies of Africa last October were also recovered in the Sudanese desert.

Sources: Space.com, Space News Examiner

Posted on by Nancy Atkinson

Meteorites Found in Africa From First Predicted Asteroid Hit

Map of the Nubian Desert of northern Sudan with the groundprojected approach path of the asteroid 2008 TC3 and the location of the recovered meteorites. Credit: P. Jenniskens, et. al

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Remember in October 2008 when Asteroid 2008 TC3 hit the scene – literally? This was the first asteroid that was predicted –and predicted correctly — to impact the Earth. Luckily, it wasn’t big enough to cause any problems, and its path was over a remote area in Africa. It streaked into the skies over northern Sudan in the early morning of October 7, 2008, and then exploded at a high 37 km above the Nubian Desert, before the atmosphere could slow it down. It was believed that the asteroid likely had completely disintegrated into dust. But meteor astronomer Peter Jenniskens thought there might be a chance to recover some of the remains of this truck-sized asteroid. And he was right.

Never before have meteorites been collected from such a high altitude explosion. Additionally, as it turns out, the assembled remnants are unlike anything in our meteorite collections, and may be an important clue in unraveling the early history of the solar system.

A meteor astronomer with the SETI Institute’s Carl Sagan Center, Jenniskens established a collaboration with Mauwia Shaddad of the Physics Department and Faculty of Sciences of the University of Khartoum. The two traveled to the Sudan.

Various meteorites from 2008 TC3. Credit: P. Jenniskens, et. al. Click image for full description
Various meteorites from 2008 TC3. Credit: P. Jenniskens, et. al. Click image for full description

Fifteen fresh-looking meteorites with a total mass of 563 g were recovered by 45 students and staff of the University of Khartoum during a field campaign on December 5-8, 2008. A second search on December 25-30 with 72 participants raised the total to 47 meteorites and 3.95 kg. Masses range from 1.5 g to 283 g, spread for 29km along the approach path in a manner expected for debris from 2008 TC3

“This was an extraordinary opportunity, for the first time, to bring into the lab actual pieces of an asteroid we had seen in space,” said Jenniskens, the lead author on a cover story article in the journal Nature that describes the recovery and analysis of 2008 TC3.

Click here for several images from NASA about the asteroid hit and the recovery of the meteorites.

Picked up by Arizona’s Catalina Sky Survey telescope on 6 October, 2008, Asteroid 2008 TC3 abruptly ended its 4.5 billion year solar-system odyssey only 20 hours after discovery, when it broke apart in the African skies. The incoming asteroid was tracked by several groups of astronomers, including a team at the La Palma Observatory in the Canary Islands that was able to measure sunlight reflected by the object.

Studying the reflected sunlight gives clues to the minerals at the surface of these objects. Astronomers group the asteroids into classes, and attempt to assign meteorite types to each class. But their ability to do this is often frustrated by layers of dust on the asteroid surfaces that scatter light in unpredictable ways.

Jenniskens teamed with planetary spectroscopist Janice Bishop of the SETI Institute to measure the reflection properties of the meteorite, and discovered that both the asteroid and its meteoritic remains reflected light in much the same way — similar to the known behavior of so-called F-class asteroids.

“F-class asteroids were long a mystery,” Bishop notes. “Astronomers have measured their unique spectral properties with telescopes, but prior to 2008 TC3 there was no corresponding meteorite class, no rocks we could look at in the lab.”

Petrography of Almahata Sitta. Credit: Jenniskens, et. al. Click for full description
Petrography of Almahata Sitta. Credit: Jenniskens, et. al. Click for full description

The good correspondence between telescopic and laboratory measurements for 2008 TC3 suggests that small asteroids don’t have the troublesome dust layers, and may therefore be more suitable objects for establishing the link between asteroid type and meteorite properties. That would allow us to characterize asteroids from afar.

Rocco Mancinelli, a microbial ecologist at the SETI Institute’s Carl Sagan Center, and a member of the research team, says that “2008 TC3 could serve as a Rosetta Stone, providing us with essential clues to the processes that built Earth and its planetary siblings.”

In the dim past, as the solar system was taking shape, small dust particles stuck together to form larger bodies, a process of accumulation that eventually produced the asteroids. Some of these bodies collided so violently that they melted throughout.

2008 TC3 turns out to be an intermediate case, having been only partially melted. The resulting material produced what’s called a polymict ureilite meteorite. The meteorites from 2008 TC3, now called “Almahata Sitta,” are anomalous ureilites: very dark, porous, and rich in highly cooked carbon. This new material may serve to rule out many theories about the origin of ureilites.

In addition, knowing the nature of F-class asteroids could conceivably pay off in protecting Earth from dangerous impactors. The explosion of 2008 TC3 at high altitude indicates that it was of highly fragile construction. Its estimated mass was about 80 tons, of which only some 5 kg has been recovered on the ground. If at some future time we discover an F-class asteroid that’s, say, several kilometers in size — one that could wipe out entire species — then we’ll know its composition and can devise appropriate strategies to ward it off.

As efforts such as the Pan-STARRS project uncover smaller near-Earth asteroids, Jenniskens expects more incidents similar to 2008 TC3. “I look forward to getting a call from the next person to spot one of these,” he says. “I would love to travel to the impact area in time to see the fireball in the sky, study its breakup and recover the pieces. If it’s big enough, we may well find other fragile materials not yet in our meteorite collections.”

Source: SETI