1996 Adams

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1996 Adams
250px
Light curve-based 3D-model of 1996 Adams
Discovery [1][2]
Discovered by Indiana Asteroid Program
Discovery site Goethe Link Obs.
Discovery date 16 October 1961
Designations
MPC designation 1996 Adams
Named after
John Couch Adams
(mathematician)[3]
1961 UA · 1932 RM
1961 TB2 · 1969 TW2
1971 BY1 · 1973 SJ3
main-belt
Eunomia[4] · Maria[5]
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 54.45 yr (19889 days)
Aphelion 2.9132 AU (435.81 Gm)
Perihelion 2.2041 AU (329.73 Gm)
2.5587 AU (382.78 Gm)
Eccentricity 0.13855
4.09 yr (1494.9 d)
116.39°
Inclination 15.140°
1.1107°
354.35°
Earth MOID 1.19868 AU (179.320 Gm)
Jupiter MOID 2.52284 AU (377.411 Gm)
Physical characteristics
Dimensions 12.05±0.44 km[6]
13.529±0.069 km[7]
10.12±0.41 km[8]
13.26 km (calculated)[4]
3.311 h (0.1380 d)[1][9][10][lower-alpha 1]
3.560 h[5]
3.316±0.079 h[lower-alpha 1]
3.31138±0.00006 h[11]
3.27±0.02 h[12]
0.177±0.014[6]
0.1405±0.0118[7]
0.395±0.066[8]
0.21 (assumed)[4]
S[4]
11.6[1]

1996 Adams, provisional designation 1961 UA, is a stony asteroid from the inner regions of the asteroid belt, about 13 kilometers in diameter. It was discovered on 16 October 1961, at the U.S. Goethe Link Observatory near Brooklyn, Indiana, by the Indiana Asteroid Program.[2]

The Collaborative Asteroid Lightcurve Link (CALL) classifies the asteroid as a member of the Eunomia family, a large group of S-type asteroids and the most prominent family in the intermediate main-belt. However, based on its concurring orbital elements, Alvarez-Candal from the Universidad Nacional de Córdoba, groups the asteroid into the Maria family, which is named after 170 Maria (also see 9175 Graun).[5]:389

The S-type asteroid orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 1 month (1,494 days). Its orbit is tilted by 15 degrees to the plane of the ecliptic and shows an eccentricity of 0.14. It has an albedo in the range of 0.14–0.40, according to observations made by the space-based satellites Akari and WISE/NEOWISE,[6][7][8] while CALL assumed an intermediate albedo of 0.21, which is typical value for stony asteroids.[4] Based upon a large number of measurements of its light-curve, the body has a concurring synodic rotation period of 3.3 hours.[lower-alpha 1][5][9][10][11][12]

The minor planet is named after John Couch Adams (1819–1892), British mathematician and astronomer, who predicted the existence and position of Neptune, simultaneously with French mathematician Urbain Le Verrier, (also see 1997 Leverrier). The lunar crater Adams is also named in his honour.[3]

References

  1. 1.0 1.1 1.2 Mazzone (2011) web: rotation period 3.311±0.001 hours with a brightness amplitude of 0.44 mag, and Aznar (2011) web: rotation period 3.316±0.079 hours with a brightness amplitude of 0.6 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (1996) Adams
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External links