|Discovered by||Catalina Sky Survey|
|Discovery date||October 6, 2008, 06:39 UTC|
|Near-Earth object (NEO), Apollo asteroid|
|Aphelion||1.71644 AU ±0.000011|
|Perihelion||0.899957 AU ±0.0000015|
|1.308201 AU ±0.0000087|
(546.525 days) ±0.0055 (0.000015)
|Mass||80,000 kg (8*104 kg)|
|96.99 seconds (0.0269409 h)|
2008 TC3 (Catalina Sky Survey temporary designation 8TA9D69) was an 80 tonnes 4.1 meters (13 ft) diameter asteroid that entered Earth's atmosphere on October 7, 2008 and exploded at an estimated 37 kilometers (23 mi) above the Nubian Desert in Sudan. Some 600 meteorites, weighing a total of 10.5 kilograms (23 lb), were recovered; many of these belonged to a rare type known as ureilites, which contain, among other minerals, nanodiamonds.
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 issued 25 Minor Planet Electronic Circulars with new orbit solutions in eleven hours 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.
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 12.8 kilometres per second (29,000 mph) 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 1,400 km (870 mi) away reported seeing the bright flash." A webcam captured the flash lighting up El-Gouna beach 725 kilometres north (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 100–200 kilometers (62–124 mi) west as it descended, somewhat east of the Nile River, and about 100 kilometers (62 mi) 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 65.4 kilometers (40.6 mi; 35.3 nmi) altitude and final explosion at at 37 kilometers (23 mi; 20 nmi) altitude. These images have not been publicly released.
Recovered fragments (Almahata Sitta meteorite)
A search of the impact zone that began on December 6, 2008, turned up 10.5 kilograms (23 lb) of rock in some 600 fragments. These meteorites are collectively named Almahata Sitta, which means "Station Six" in Arabic 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 asteroid 2008 TC3 as an F-type asteroid class. These fragile anomalous dark carbon-rich ureilites are now firmly linked to the group of F-class asteroids. Amino acids have been found on the meteorite.
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.
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Une webcam de surveillance, située sur la plage de la Mer Rouge à El Gouna en Egypte, a enregistré indirectement le flash de l'explosion qui s'est produit à environ 725 km plus au sud.
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|An image of 2008 TC3|
|Animation of 2008 TC3|
|Smoky trail (spaceweather.com November 8, 2008)|
|Wikimedia Commons has media related to 2008 TC3.|
- Remanzacco Observatory photographs of the incoming space rock
- Telescopio Nazionale Galileo photograph of 2008 TC3
- Announcement with animation
- "webcam record of flash effect from Red Sea beach at El Gouna, Egypt, 725 km away" (GIF). Archived from the original on 2009-06-10. Retrieved 2009-06-08.
- Almahata Sitta 15 Astronomy Picture of the Day