96 Aegle
Discovery | |
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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[1] km |
Mass | (6.48 ± 6.26) × 1018[1] kg |
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 | |
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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. Aegle has been observed occulting three stars.
References
- ↑ 1.0 1.1 1.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ↑ 2.0 2.1
- ↑ 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, retrieved 22 March 2013. See appendix A.
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