1996 Adams

1996 Adams

Light curve-based 3D-model of 1996 Adams
Discovery [1][2]
Discovered by Indiana University
(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°
0° 14m 26.952s / day
Inclination 15.140°
1.1107°
354.35°
Earth MOID 1.19868 AU (179.320 Gm)
Jupiter MOID 2.52284 AU (377.411 Gm)
Jupiter Tisserand parameter 3.374
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, by the Indiana Asteroid Program at Goethe Link Observatory near Brooklyn, Indiana, United States.[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 2 3 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
    1. 1 2 3 4 "JPL Small-Body Database Browser: 1996 Adams (1961 UA)" (2015-11-21 last obs.). Jet Propulsion Laboratory. Retrieved 17 April 2016.
    2. 1 2 "1996 Adams (1961 UA)". Minor Planet Center. Retrieved 24 October 2015.
    3. 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1996) Adams. Springer Berlin Heidelberg. p. 162. ISBN 978-3-540-29925-7. Retrieved 24 October 2015.
    4. 1 2 3 4 5 "LCDB Data for (1996) Adams". Asteroid Lightcurve Database (LCDB). Retrieved 17 December 2015.
    5. 1 2 3 4 Alvarez-Candal, Alvaro; Duffard, René; Angeli, Cláudia A.; Lazzaro, Daniela; Fernández, Silvia (December 2004). "Rotational lightcurves of asteroids belonging to families". Icarus. 172 (2): 388–401. Bibcode:2004Icar..172..388A. doi:10.1016/j.icarus.2004.06.008. Retrieved 17 December 2015.
    6. 1 2 3 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 17 December 2015.
    7. 1 2 3 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 17 December 2015.
    8. 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794Freely accessible. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved 17 December 2015.
    9. 1 2 Durkee, Russell I. (January 2011). "Asteroids Observed from the Shed of Science Observatory: 2010 May-October". The Minor Planet Bulletin. 38 (1): 39–40. Bibcode:2011MPBu...38...39D. ISSN 1052-8091. Retrieved 17 December 2015.
    10. 1 2 Aymami, Josep Maria (January 2011). "CCD Photometry and Lightcurve Analysis of 1730 Marceline and 1996 Adams from Observatori Carmelita in Tiana". The Minor Planet Bulletin. 38 (1): 55–56. Bibcode:2011MPBu...38...55A. ISSN 1052-8091. Retrieved 17 December 2015.
    11. 1 2 Ambrosioni, Carlos; Colazo, Carlos; Mazzone, Fernando (April 2011). "Period Determination for 1996 Adams and 2699 Kalinn by AOACM". The Minor Planet Bulletin. 38 (2): 102. Bibcode:2011MPBu...38..102A. ISSN 1052-8091. Retrieved 17 December 2015.
    12. 1 2 Kim, M.-J.; Choi, Y.-J.; Moon, H.-K.; Byun, Y.-I.; Brosch, N.; Kaplan, M.; et al. (March 2014). "Rotational Properties of the Maria Asteroid Family". The Astronomical Journal. 147 (3): 15. arXiv:1311.5318Freely accessible. Bibcode:2014AJ....147...56K. doi:10.1088/0004-6256/147/3/56. Retrieved 17 December 2015.

    External links

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