From Wikipedia, the free encyclopedia

(237442) 1999 TA10
Discovery [1]
Discovered by LINEAR
Discovery site Lincoln Laboratory ETS
Discovery date5 October 1999
Designations
(237442) 1999 TA10
Amor asteroid ( NEO) [2]
Orbital characteristics [2]
Epoch 13 January 2016 ( JD 2457400.5)
Uncertainty parameter 0
Observation arc5592 days (15.31 yr)
Aphelion1.8695  AU (279.67  Gm) (Q)
Perihelion1.1419 AU (170.83 Gm) (q)
1.5057 AU (225.25 Gm) (a)
Eccentricity0.24161 (e)
1.85 yr (674.85 d)
342.45 ° (M)
0° 32m 0.42s / day (n)
Inclination20.843° (i)
214.68° (Ω)
84.791° (ω)
Earth  MOID0.303797 AU (45.4474 Gm)
Physical characteristics
Dimensions500–1500 meters [2] [3]
14  h (0.58  d)
14 hr(?) [2]
16.77 (close approach) to 22.29
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  AU (2,500,000  km; 1,600,000  mi) of Mars. [5]

See also

References

  1. ^ a b "MPEC 1999-T43 : 1999 TA10". IAU Minor Planet Center. 11 October 1999. Retrieved 12 January 2011.
  2. ^ a b c d e f g "JPL Small-Body Database Browser: 237442 (1999 TA10)" (last observation: 2010-11-08). Archived from the original on 20 September 2020. Retrieved 7 April 2016.
  3. ^ a b "Conversion of Absolute Magnitude to Diameter". Minor Planet Center. Archived from the original on 27 October 2010. Retrieved 12 January 2011.
  4. ^ a b "A look into Vesta's interior". Max Planck Society. 6 January 2011. Archived from the original on 13 January 2011. Retrieved 7 January 2011.
  5. ^ a b c d "JPL Close-Approach Data: 237442 (1999 TA10)" (2010-11-08 last obs). Retrieved 12 January 2011.
From Wikipedia, the free encyclopedia

(237442) 1999 TA10
Discovery [1]
Discovered by LINEAR
Discovery site Lincoln Laboratory ETS
Discovery date5 October 1999
Designations
(237442) 1999 TA10
Amor asteroid ( NEO) [2]
Orbital characteristics [2]
Epoch 13 January 2016 ( JD 2457400.5)
Uncertainty parameter 0
Observation arc5592 days (15.31 yr)
Aphelion1.8695  AU (279.67  Gm) (Q)
Perihelion1.1419 AU (170.83 Gm) (q)
1.5057 AU (225.25 Gm) (a)
Eccentricity0.24161 (e)
1.85 yr (674.85 d)
342.45 ° (M)
0° 32m 0.42s / day (n)
Inclination20.843° (i)
214.68° (Ω)
84.791° (ω)
Earth  MOID0.303797 AU (45.4474 Gm)
Physical characteristics
Dimensions500–1500 meters [2] [3]
14  h (0.58  d)
14 hr(?) [2]
16.77 (close approach) to 22.29
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  AU (2,500,000  km; 1,600,000  mi) of Mars. [5]

See also

References

  1. ^ a b "MPEC 1999-T43 : 1999 TA10". IAU Minor Planet Center. 11 October 1999. Retrieved 12 January 2011.
  2. ^ a b c d e f g "JPL Small-Body Database Browser: 237442 (1999 TA10)" (last observation: 2010-11-08). Archived from the original on 20 September 2020. Retrieved 7 April 2016.
  3. ^ a b "Conversion of Absolute Magnitude to Diameter". Minor Planet Center. Archived from the original on 27 October 2010. Retrieved 12 January 2011.
  4. ^ a b "A look into Vesta's interior". Max Planck Society. 6 January 2011. Archived from the original on 13 January 2011. Retrieved 7 January 2011.
  5. ^ a b c d "JPL Close-Approach Data: 237442 (1999 TA10)" (2010-11-08 last obs). Retrieved 12 January 2011.

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