168 Sibylla
| Discovery[1] | |
|---|---|
| Discovered by | J. C. Watson |
| Discovery site | Ann Arbor |
| Discovery date | 28 September 1876 |
| Orbital characteristics[2][3] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 136.01 yr (49676 d) |
| Aphelion | 3.6215 AU (541.77 Gm) |
| Perihelion | 3.1417 AU (469.99 Gm) |
| 3.3816 AU (505.88 Gm) | |
| Eccentricity | 0.070943 |
| 6.22 yr (2271.4 d) | |
Average orbital speed | 16.19 km/s |
| 171.517° | |
| 0° 9m 30.564s / day | |
| Inclination | 4.6617° |
| 205.959° | |
| 173.920° | |
| Earth MOID | 2.14278 AU (320.555 Gm) |
| Jupiter MOID | 1.8199 AU (272.25 Gm) |
| Jupiter Tisserand parameter | 3.142 |
| Physical characteristics | |
| Dimensions |
148.39±4.0 km[2] 149.06 ± 4.29 km[4] |
| Mass | (3.92 ± 1.80) × 1018 kg[4] |
Mean density | 2.26 ± 1.05 g/cm3[4] |
| 47.009 h (1.9587 d) | |
Sidereal rotation period | 23.82 hours[5] |
| 0.0535±0.003 | |
| C | |
| 7.94 | |
|
| |
168 Sibylla is a large main-belt asteroid, discovered by Canadian-American astronomer J. C. Watson on September 28, 1876. Based upon its spectrum this object is classified as a C-type asteroid, which indicates it is very dark and composed of primitive carbonaceous materials. 168 Sibylla is a Cybele asteroid, orbiting beyond most of the main-belt asteroids.
Photometric observations of this asteroid made at the Torino Observatory in Italy during 1990–1991 were used to determine a synodic rotation period of 23.82 ± 0.004 hours.[5]
References
- ↑ "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". Retrieved August 14, 2012.
- 1 2 Yeomans, Donald K., "168 Sibylla", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
- ↑ "The Asteroid Orbital Elements Database". astorb. Lowell Observatory. Retrieved August 14, 2012.
- 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 di Martino, M.; et al. (February 1994), "Lightcurves and rotational periods of nine main belt asteroids", Icarus, 107 (2), pp. 269–275, Bibcode:1994Icar..107..269D, doi:10.1006/icar.1994.1022.
External links
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