2008 TC3

Template:Mp (Catalina Sky Survey temporary designation 8TA9D69) was an , diameter asteroid that entered Earth's atmosphere on October 7, 2008. It exploded at an estimated above the Nubian Desert in Sudan. Some 600 meteorites, weighing a total of , were recovered; many of these belonged to a rare type known as ureilites, which contain, among other minerals, nanodiamonds.

It was the first time that an asteroid impact had been predicted before its entry into the atmosphere as a meteor.

Discovery

File:2008 TC3 Tumbling (reduced).gif

An animation of 2008 TC3's excited rotation prior to entering the atmosphere

The asteroid was discovered by Richard A. Kowalski at the Catalina Sky Survey (CSS) 1.5-meter telescope at Mount Lemmon, north of Tucson, Arizona, US, on October 6, 06:39 UTC, 19 hours before the impact.

It was notable as the first such body to be observed and tracked prior to reaching Earth. The process of detecting and tracking a near-Earth object, an effort sometimes referred to as Spaceguard, was put to the test. In total, 586 astrometric and almost as many photometric observations were performed by 27 amateur and professional observers in less than 19 hours and reported to the Minor Planet Center, which in eleven hours issued 25 Minor Planet Electronic Circulars with new orbit solutions as observations poured in. On October 7, 01:49 UTC, the asteroid entered the shadow of the Earth, which made further observations impossible.

Impact predictions were performed by University of Pisa's CLOMON 2 semi-automatic monitoring system as well as Jet Propulsion Laboratory's Sentry system. Spectral observations that were performed by astronomers at the 4.2-meter William Herschel Telescope at La Palma, Canary Islands are consistent with either a C-type or M-type asteroid.

Entry

File:Eumetsat-composite-2008TC3-impact.jpg

Meteosat 8/EUMETSAT infrared image of the explosion

File:Animation of 2008 TC3 orbit around Sun.gif

Animation of 2008 TC3's orbit
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The meteor entered Earth's atmosphere above northern Sudan at 02:46 UTC (05:46 local time) on October 7, 2008, with a velocity of at an azimuth of 281 degrees and an altitude angle of 19 degrees to the local horizon. It exploded tens of kilometers above the ground with the energy of 0.9 to 2.1 kilotons of TNT over a remote area of the Nubian Desert, causing a large fireball or bolide.

The Times reported that the meteor's "light was so intense that it lit up the sky like a full moon, and an airliner away reported seeing the bright flash." A webcam captured the flash lighting up El-Gouna beach 725 kilometres north of the explosion (see this webcam frame). A low-resolution image of the explosion was captured by the weather satellite Meteosat 8. The Meteosat images place the fireball at . Infrasound detector arrays in Kenya also detected a sound wave from the direction of the expected impact corresponding to energy of 1.1 to 2.1 kilotons of TNT. Asteroids of this size hit Earth about two or three times a year.

The trajectory showed intersection with Earth's surface at roughly though the object was expected to break up perhaps west as it descended, somewhat east of the Nile River, and about south of the Egypt–Sudan border.

According to U.S. government sources U.S. satellites detected the impact at 02:45:40 UT, with the initial detection at at altitude and final explosion at at altitude. These images have not been publicly released.

Recovered fragments

File:323213main Petersmeteorites 946-710.jpg

Template:Mp fragment found on February 28, 2009, by Peter Jenniskens, with help from students and staff of the University of Khartoum. Nubian Desert, Sudan.

A search of the impact zone that began on December 6, 2008, turned up of rock in some 600 fragments. These meteorites are collectively named Almahata Sitta (Template:Langx), which means "Station Six" and is a train station between Wadi Halfa and Khartoum, Sudan. This search was led by Peter Jenniskens from the SETI Institute, California and Muawia Shaddad of the University of Khartoum in Sudan and carried out with the collaboration of students and staff of the University of Khartoum. The initial 15 meteorites were found in the first three days of the search. Numerous witnesses were interviewed, and the hunt was guided with a search grid and specific target area produced by NASA's Jet Propulsion Laboratory in Pasadena, California.

Samples of the Almahata Sitta meteorite were sent for analysis to a consortium of researchers led by Jenniskens, the Almahata Sitta consortium, including NASA Ames in California, the Johnson Space Center in Houston, the Carnegie Institution of Washington, and Fordham University in New York City. The first sample measured was an anomalous ultra-fine-grained porous polymict ureilite achondrite, with large carbonaceous grains. Reflectance spectra of the meteorite, combined with the astronomical observations, identified 2008 TC₃ as an F-type asteroid. Fragile anomalous dark carbon-rich ureilites like in the Almahata Sitta meteorite are now firmly linked to the group of F-class asteroids. Amino acids have been found on the meteorite. The nanodiamonds found in the meteorite were shown to have grown slowly, implying that the source is another planet in the Solar System. More recently, in December 2020, further studies on the fragments have been reported. These studies revealed an extremely rare form of hydrated crystals, in a fragment called AhS 202, known as amphibole, suggesting to the researchers that 2008 TC3 early on likely belonged to a very large Ceres-class dwarf planet.

Richard Kowalski, who discovered the object, received a tiny fragment of Almahatta Sitta, a gift from friends and well-wishers on the Minor Planet Mailing List, which Kowalski founded in order to help connect professional and amateur astronomers.

Gallery

• Meteosat 8/EUMETSAT visual image of first light flare from 2008 TC3 with lat/long reference
  Meteosat 8/EUMETSAT visual image of first light flare from 2008 TC₃ with lat/long reference
• Meteosat 8/EUMETSAT IR image of main fireball from 2008 TC3
  Meteosat 8/EUMETSAT IR image of main fireball from 2008 TC₃
• Meteosat images combined, showing offset from first light flare to main IR flare
  Meteosat images combined, showing offset from first light flare to main IR flare

See also

• Asteroid impact prediction
• 1972 Great Daylight Fireball
• 2014 AA
• 2018 LA
• 2019 MO
• Template:Mpl
• Template:Mpl
• Template:Mpl
• Impact event
• List of notable asteroids
• WT1190F

External links

• Remanzacco Observatory photographs of the incoming space rock
• Telescopio Nazionale Galileo photograph of 2008 TC₃
• Announcement with animation
• Template:APOD
• 2008 TC3 orbit and observations at IAU Minor Planet Center
• Template:NeoDys
• Template:ESA-SSA
• Template:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata