8373 Stephengould
Appearance
Discovery[1] | |
---|---|
Discovered by | Carolyn S. Shoemaker and Eugene Merle Shoemaker |
Discovery site | Palomar |
Discovery date | 1 January 1992 |
Designations | |
8373 | |
Named after | Stephen Jay Gould |
1992 AB | |
Orbital characteristics[2][3] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 8844 days (24.21 yr) |
Aphelion | 5.09996 AU (762.943 Gm) |
Perihelion | 1.45970 AU (218.368 Gm) |
3.27983 AU (490.656 Gm) | |
Eccentricity | 0.554947 |
5.94 yr (2169.6 d) | |
358.004° | |
0° 9m 57.352s / day | |
Inclination | 40.7923° |
88.8722° | |
55.5019° | |
Earth MOID | 0.643589 AU (96.2795 Gm) |
Jupiter MOID | 1.4741 AU (220.52 Gm) |
TJupiter | 2.587 |
Physical characteristics | |
4.435 h (0.1848 d) | |
14.0 | |
8373 Stephengould (1992 AB) is an outer main-belt binary asteroid[4] discovered on January 1, 1992 by Carolyn S. Shoemaker and Eugene Merle Shoemaker at Palomar.[1] The asteroid was named after the Harvard paleontologist Stephen Jay Gould. The asteroid has a very high inclination, having the second highest inclination of any of the first 10,000 discovered asteroids in the asteroid belt, after 2938 Hopi.
This is a member of the Griqua family of asteroids that share similar orbital elements.[5] It is one of very few asteroids located in the 2 : 1 mean motion resonance with Jupiter.[6]
The asteroid has a moon orbiting it, discovered in 2010 with an orbital period of 1 day, 10 hours, and 9 minutes.[4]
References
- ^ a b "Discovery Circumstances: Numbered Minor Planets (5001)-(10000)". IAU: Minor Planet Center. Retrieved 7 December 2008.
- ^ "(8373) Stephengould". AstDyS. Italy: University of Pisa. Retrieved 10 December 2008.
- ^ "8373 Stephengould (1992 AB)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 13 April 2016.
- ^ a b Johnston, Robert. "(8373) Stephengould". johnstonsarchive.net. Retrieved 29 May 2015.
- ^ Moore, Patrick; Rees, Robin, eds. (2011), Patrick Moore's Data Book of Astronomy (2nd ed.), Cambridge University Press, pp. 164–165.
- ^ Roig, F.; Nesvorný, D.; Ferraz-Mello, S. (September 2002). "Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution". Monthly Notices of the Royal Astronomical Society. 335 (2): 417–431. Bibcode:2002MNRAS.335..417R. doi:10.1046/j.1365-8711.2002.05635.x.
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External links
- JPL Small-Body Database Browser on 8373 Stephengould
- 8373 Stephengould at the JPL Small-Body Database