96 Aegle
Discovery | |
---|---|
Discovered by | Jérôme Eugène Coggia |
Discovery date | February 17, 1868 |
Designations | |
Named after | Aegle |
Main belt | |
Orbital characteristics | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 517.649 Gm (3.460 AU) |
Perihelion | 397.127 Gm (2.655 AU) |
457.388 Gm (3.057 AU) | |
Eccentricity | 0.132 |
1952.711 d (5.35 a) | |
Average orbital speed | 16.96 km/s |
354.814° | |
Inclination | 15.938° |
321.809° | |
206.967° | |
Physical characteristics | |
Dimensions | 167.92 ± 5.49 km[1] |
Mass | (6.48 ± 6.26) × 1018 kg[1] |
Mean density | 2.61 ± 2.53[1] g/cm3 |
0.0475 m/s² | |
0.0898 km/s | |
13.82 h[2] | |
Albedo | 0.052 [3] |
Temperature | ~159 K |
Spectral type | T[2][4] |
7.67 | |
|
96 Aegle (/ˈiːɡliː/ EE-glee) is a very large main-belt asteroid. It has a dark-colored surface and probably a primitive carbonaceous composition. It was discovered by Jérôme Coggia on February 17, 1868, and named after one of the three Aegles in Greek mythology.[5] Aegle has been observed occulting seven stars (on 18 Feb 2002, 10 Aug 2002, 3 Aug 2003, 8 Sep 2009, 5 Jan 2010, 29 Oct 2010, and 7 Sep 2013).[6]
References
- 1 2 3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- 1 2
- ↑ Asteroid Data Sets
- ↑ DeMeo, Francesca E.; et al. (2011), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus, 202 (1): 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.2009.02.005, archived from the original (PDF) on 17 March 2014, retrieved 22 March 2013. See appendix A.
- ↑ Schmadel, Lutz D. (1997). "Dictionary of Minor Planet Names". Germany: Springer. p. 33. ISBN 978-3-662-06617-1. Retrieved 24 January 2016.
- ↑ Watanabe, Hayato (3 January 2016), The Index of Asteroidal Occultation Results, Worldwide (ver. 2), retrieved 23 January 2016
External links
- 96 Aegle at the JPL Small-Body Database
This article is issued from Wikipedia - version of the 9/30/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.