astro.wikisort.org - Asteroid
8373 Stephengould (1992 AB) is an outer main-belt binary asteroid[5] discovered on 1 January 1992 by Carolyn S. Shoemaker and Eugene Merle Shoemaker at Palomar Observatory.[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.
| Discovery[1] | |
|---|---|
| Discovered by | |
| Discovery site | Palomar |
| Discovery date | 1 January 1992 |
| Designations | |
MPC designation | (8373) Stephengould |
Named after | Stephen Jay Gould |
Alternative designations | 1992 AB |
Minor planet category | |
| Orbital characteristics[4][2] | |
| 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) |
Semi-major axis | 3.27983 AU (490.656 Gm) |
| Eccentricity | 0.554947 |
Orbital period (sidereal) | 5.94 yr (2169.6 d) |
Mean anomaly | 358.004° |
Mean motion | 0° 9m 57.352s / day |
| Inclination | 40.7923° |
Longitude of ascending node | 88.8722° |
Argument of perihelion | 55.5019° |
| Known satellites | 1 |
| Jupiter MOID | 1.4741 AU (220.52 Gm) |
| TJupiter | 2.587 |
| Physical characteristics | |
Synodic rotation period | 4.435 h (0.1848 d) |
Absolute magnitude (H) | 14.0 |
Stephengould is one of few strongly unstable asteroids located near the 2:1 mean motion resonance with the gas giant Jupiter, that corresponds to one of the prominent Kirkwood gaps in the asteroid belt.[3]
The asteroid has a moon orbiting it, discovered in 2010 with an orbital period of 1 day, 10 hours, and 9 minutes.[5]
See also
References
- "Discovery Circumstances: Numbered Minor Planets (5001)–(10000)". IAU: Minor Planet Center. Retrieved 7 December 2008.
- "8373 Stephengould (1992 AB)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 13 April 2016.
- Roig, F.; Nesvorný, D.; Ferraz-Mello, S. (September 2002). "Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution [ Erratum: 2002MNRAS.336.1391R ]". Monthly Notices of the Royal Astronomical Society. 335 (2): 417–431. Bibcode:2002MNRAS.335..417R. doi:10.1046/j.1365-8711.2002.05635.x. Retrieved 31 March 2017.
- "(8373) Stephengould". AstDyS. Italy: University of Pisa. Archived from the original on 26 May 2011. Retrieved 10 December 2008.
- Johnston, Robert. "(8373) Stephengould". johnstonsarchive.net. Retrieved 29 May 2015.
External links
- Lightcurve plot of 8373 Stephengould, Palmer Divide Observatory, B. D. Warner (2004)
- Patrick Moore's Data Book of Astronomy, Cambridge University Press (2011)
- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)–(5000) – Minor Planet Center
- 8373 Stephengould at AstDyS-2, Asteroids—Dynamic Site
- 8373 Stephengould at the JPL Small-Body Database
 | This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |
На других языках
- [en] 8373 Stephengould
[ru] (8373) Стивенгулд
(8373) Стивенгулд (лат. Stephengould) — двойной астероид[2] внешней части главного пояса, который входит в состав семейства Гриквы[3]. Он был открыт 1 января 1992 года американскими астрономами Кэролин Шумейкер и Юджином Шумейкер в Паломарской обсерватории и назван в честь американского палеонтолога Стивена Гулда[4].Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
WikiSort.org - проект по пересортировке и дополнению контента Википедии