2000 SG344

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2000 SG344
Asteroid 2000 SG344.gif
The dim streak in this negative image is 2000 SG344 moving against the background field of stars on Sept. 29, 2000
Discovered by D. J. Tholen, and R. J. Whiteley
Discovery site Mauna Kea Observatory - UH88
Discovery date 2000-09-29
Aten Aten
Orbital characteristics[2]
Epoch 2454600.5
Aphelion 1.04286173 ± 7.4785e-07 AU
Perihelion .9119995 ± 4.3409e-06 AU
.97743066 ± 7.0093e-07 AU
Eccentricity .0669419 ± 3.7724e-06
352.9615239 ± 0.00037967 d
228.373742 ± 0.0031236°
Inclination .1103173 ± 8.2267e-06°
192.301028 ± 0.0015524°
274.922907 ± 0.00164°
Physical characteristics
Dimensions 37 meters (121 ft)[3]
Mass 7.1×107 kg[3]
24.788 ± 0.83657[2]

2000 SG344 (also written 2000 SG344) is a small Aten asteroid discovered in 2000. It is estimated have a diameter of 37 meters (twice that of the Chelyabinsk meteor) and a mass of 7.1×107 kg (71,000 tonnes).[3]

Because of its very Earth-like orbit and the fact that it would have been near the Earth in 1971 (coinciding with the Apollo program), there was speculation that 2000 SG344 might not be an Asteroid but actually a man made object such as an S-IVB booster stage from a Saturn V rocket.[4][5] (cf. J002E3, the S-IVB booster of Apollo 12 which was mistaken for an asteroid.)

Possible impacts with Earth[edit]

Until December 2004, it was considered to have the highest (though still very low) likelihood of any near-Earth object to impact Earth in the next 100 years. It is ranked a zero on the Torino Scale of impact risk because of its small size (the scale is 0–10) and is listed on Sentry Risk Table.[3][6] It was briefly surpassed in December 2004 by 99942 Apophis (which at the time was known only by its provisional designation 2004 MN4). The smaller asteroids 2006 JY26 and 2010 RF12 have a greater chance of impacting Earth.

Based on 31 observations of 2000 SG344 made from May 1999 to October 2000, there is about a 1 in 417 chance that it will collide with Earth between 2069 and 2113. Assuming the object is a rocky asteroid, the impact energy released would be an estimated 1.1 megatons of TNT,[3] which would create an impact crater approximately 100 feet (30 m) wide assuming it does not explode in the atmosphere

Planned NASA mission[edit]

NASA is considering it as a possible target for a manned mission (Exploration Mission 2) using the Orion spacecraft, prior to a projected 2030 push to Mars.[7] 2000 SG344 will be observable in April 2028 at an apparent magnitude of 19.[8]

Further reading[edit]

External links[edit]

  • Nasa NEO Study home page
    • [ti.arc.nasa.gov/m/project/neo/pdf/NEO_feasibility.pdf Piloted Orion Flight Feasibility Study]
    • Into the Beyond: A Crewed Mission to an Near-Earth Object - [ti.arc.nasa.gov/m/project/neo/pdf/neo_crewed_mission.pdf text] [ti.arc.nasa.gov/m/project/neo/pdf/IAC-07-slides.pdf slides]


  1. ^ "IAU Circular: MPEC 2000-U19". 2000-10-24. Retrieved 18 May 2008. 
  2. ^ a b "JPL Small-Body Database Browser on 2000 SG344". NASA. Retrieved 18 May 2008. 
  3. ^ a b c d e "2000 SG344 Earth Impact Risk Summary". 2002-05-15. Archived from the original on 24 October 2004. Retrieved 2004-11-12. 
  4. ^ "Much Ado about 2000 SG344". NASA. 2000-11-07. Retrieved 19 May 2008. 
  5. ^ Chodas, P. W.; Chesley, S. R. (November 2001). "2000 SG344: The Story of a Potential Earth Impactor". Bulletin of the American Astronomical Society 33: 1196. Retrieved 19 May 2008. 
  6. ^ "NASA Near Earth Object Program: Current Impact Risks". Retrieved 2004-11-12. 
  7. ^ Sample, Ian (2008-05-07). "Closer encounter: Nasa plans landing on 40m-wide asteroid travelling at 28,000mph". The Guardian. Archived from the original on 9 May 2008. Retrieved 9 May 2008. 
  8. ^ "Near-Earth Object Human Space Flight Accessible Targets Study (NHATS)". NASA/JPL Near-Earth Object Program Office. Retrieved 2012-06-08.