Astronomy:(237442) 1999 TA10

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Short description: Asteroid and near-Earth object


(237442) 1999 TA10
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Laboratory ETS
Discovery date5 October 1999
Designations
(237442) 1999 TA10
Minor planet categoryAmor asteroid (NEO)[2]
Orbital characteristics[2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc5592 days (15.31 yr)
|{{{apsis}}}|helion}}1.8695 astronomical unit|AU (279.67 Gm) (Q)
|{{{apsis}}}|helion}}1.1419 AU (170.83 Gm) (q)
1.5057 AU (225.25 Gm) (a)
Eccentricity0.24161 (e)
Orbital period1.85 yr (674.85 d)
Mean anomaly342.45° (M)
Mean motion0° 32m 0.42s / day (n)
Inclination20.843° (i)
Longitude of ascending node214.68° (Ω)
84.791° (ω)
Earth MOID0.303797 AU (45.4474 Gm)
Physical characteristics
Dimensions500–1500 meters[2][3]
Rotation period14 h (0.58 d)
Sidereal rotation period14 hr(?)[2]
Apparent magnitude16.77 (close approach) to 22.29
Absolute magnitude (H)18.1[2]


(237442) 1999 TA10, provisionally known as 1999 TA10, is a near-Earth object (NEO) from the Amor asteroid group.[2] It is suspected of being an inner fragment of the differentiated asteroid 4 Vesta.[4]

Given an absolute magnitude (H) of 17.9,[2] and that the albedo is unknown, this NEO could vary from 500 to 1500 meters in diameter.[3]

1999 TA10 was discovered by LINEAR at Lincoln Laboratory ETS on 5 October 1999 at apparent magnitude 17.7,[1] when it was only 0.39 AU from Earth.[5] In 2010, it came within 0.3 AU of Earth.[5] During the 2010 close approach, NASA Infrared Telescope Facility (NASA IRTF) studies suggested that 1999 TA10 originated from the interior of Vesta.[4] The next close approach will be in 2023.[5] In 2086, it will come within 0.017 astronomical unit|AU (2,500,000 km; 1,600,000 mi) of Mars.[5]

See also

References

External links