2008 TC3 (Catalina Sky Survey temporary designation 8TA9D69) was an 80-tonne (80-long-ton; 90-short-ton), 4.1-meter (13 ft) diameter asteroid[2] that entered Earth's atmosphere on October 7, 2008.[3] It exploded at an estimated 37 kilometers (23 mi) above the Nubian DesertinSudan. Some 600 meteorites, weighing a total of 10.5 kilograms (23.1 lb), were recovered; many of these belonged to a rare type known as ureilites, which contain, among other minerals, nanodiamonds.[2][4][5]
| |
| Discovery | |
|---|---|
| Discovered by | Catalina Sky Survey |
| Discovery date | October 6, 2008, 06:39 UTC |
| Designations | |
| 2008 TC3 | |
|
| |
| Orbital characteristics[1] | |
| Epoch October 7, 2008 (JD 2454746.5) | |
| Uncertainty parameter4 | |
| Observation arc | 1 day (575 observations) |
| Aphelion | 1.71644 AU (256.776 Gm) |
| Perihelion | 0.899957 AU (134.6317 Gm) |
| 1.308201 AU (195.7041 Gm) | |
| Eccentricity | 0.312065 |
| 1.50 yr (546.53 d) | |
| 330.7541° | |
| 0.6587071°/day | |
| Inclination | 2.54220° |
| 194.101138° | |
| 2008-Nov-20 | |
| 234.44897° | |
| Jupiter MOID | 3.57975 AU (535.523 Gm) |
| Physical characteristics | |
| Dimensions | 4.1 meters |
| Mass | 80tonnes (80,000 kg) |
Mean density | ~1.5 g/cm3 |
| 0.0269409 h (1.61645 min)[1] | |
| 0.1±0.03 | |
| F/M | |
| 30.4[1] | |
It was the first time that an asteroid impact had been predicted before its entry into the atmosphere as a meteor.[6]
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.[7][8][9]
It was notable as the first such body to be observed and tracked prior to reaching Earth.[6] 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,[9] 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[10][11] as well as Jet Propulsion Laboratory's Sentry system. Spectral observations that were performed by astronomers at the 4.2-meter William Herschel TelescopeatLa Palma, Canary Islands are consistent with either a C-typeorM-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 kilometers 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.[12]
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."[13] A webcam captured the flash lighting up El-Gouna beach 725 kilometres north of the explosion (see this webcam frame).[14] A low-resolution image of the explosion was captured by the weather satellite Meteosat 8.[15] The Meteosat images place the fireball at 21°00′N 32°09′E / 21.00°N 32.15°E / 21.00; 32.15 (2008 TC3 fireball).[16] 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.[17] Asteroids of this size hit Earth about two or three times a year.[18]
The trajectory showed intersection with Earth's surface at roughly 20°18′N 33°30′E / 20.3°N 33.5°E / 20.3; 33.5 (2008 TC3 projected impact)[19] though the object was expected to break up perhaps 100–200 kilometers (60–120 mi) west as it descended, somewhat east of the Nile River, and about 100 kilometers (60 mi) south of the Egypt–Sudan border.
According to U.S. government sources[20][21] U.S. satellites detected the impact at 02:45:40 UT, with the initial detection at 20°54′N 31°24′E / 20.9°N 31.4°E / 20.9; 31.4 (2008 TC3 initial detection) at 65.4 kilometers (40.6 mi; 35.3 nmi) altitude and final explosion at 20°48′N 32°12′E / 20.8°N 32.2°E / 20.8; 32.2 (2008 TC3 final explosion) at 37 kilometers (23 mi; 20 nmi) altitude. These images have not been publicly released.
This section needs to be updated. The reason given is: In 2022, Bischoff et al. concluded that the meteorite's classification as a ureilite may not be correct.[1] Their findings and the impact they may have on the 2009 Jenniskens study need to be incorporated. Please help update this article to reflect recent events or newly available information. (November 2023)
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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[22] (Arabic: المحطة ستة), which means "Station Six"[23] 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 KhartouminSudan 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 LaboratoryinPasadena, California.[24][25][26][27][28]
Samples of the Almahata Sitta meteorite were sent for analysis to a consortium of researchers led by Jenniskens, the Almahata Sitta consortium, including NASA AmesinCalifornia, the Johnson Space CenterinHouston, the Carnegie Institution of Washington, and Fordham UniversityinNew 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.[2][clarification needed] Amino acids have been found on the meteorite.[29] The nanodiamonds found in the meteorite were shown to have grown slowly, implying that the source is another planet in the solar system.[30] 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.[31]
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.[32]
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.
| External images | |
|---|---|
 An image of 2008 TC3 | |
| Animation of 2008 TC3 | |
| Smoky trail (spaceweather.com November 8, 2008) |
