1101 Clematis
| Discovery | |
|---|---|
| Discovered by | Karl Wilhelm Reinmuth |
| Discovery date | 22 September 1928 |
| Designations | |
Named after | Clematis |
| 1928 SJ | |
| Main belt | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 87.28 yr (31878 days) |
| Aphelion | 3.4838 AU (521.17 Gm) |
| Perihelion | 2.97902 AU (445.655 Gm) |
| 3.23141 AU (483.412 Gm) | |
| Eccentricity | 0.078104 |
| 5.81 yr (2121.7 d) | |
Average orbital speed | 16.54 km/s |
| 83.0012° | |
| 0° 10m 10.826s / day | |
| Inclination | 21.424° |
| 201.981° | |
| 107.762° | |
| Earth MOID | 2.04443 AU (305.842 Gm) |
| Jupiter MOID | 1.79483 AU (268.503 Gm) |
| Jupiter Tisserand parameter | 3.073 |
| Physical characteristics | |
Mean radius | 18.93±0.7 km |
| Mass | 5.7×1016 kg |
Equatorial surface gravity | 0.0106 m/s² |
Equatorial escape velocity | 0.0200 km/s |
| 34.3 h (1.43 d) | |
| 0.1124±0.009 | |
| Temperature | ~155 K |
| 10.6 | |
|
| |
1101 Clematis is a minor planet orbiting the Sun that was discovered by German astronomer Karl Wilhelm Reinmuth on September 22, 1928, in Heidelberg.[2] Initially it received the designation 1928 SJ. It was named for the clematis flower.
Photometric observations made in 2003 at the Santana Observatory in Rancho Cucamonga, California, give a synodic rotation period of 12.68 ± 0.01 hours. The light curve shows a brightness variation of 0.40 ± 0.05 in magnitude.[2]
This object is the namesake of a dynamic family of 5–16 asteroids that share similar spectral properties and orbital elements; hence they may have arisen from the same collisional event. All members have a relatively high orbital inclination.[3]
See also
References
- ↑ Yeomans, Donald K., "1101 Clematis", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 2 May 2016.
- 1 2 Stephens, Robert D. (March 2004), "Photometry of 683 Lanzia, 1101 Clematis, 1499 Pori, 1507 Vaasa, and 3893 DeLaeter", The Minor Planet Bulletin, 31 (1), pp. 4–6, Bibcode:2004MPBu...31....4S.
- ↑ Novaković, Bojan; et al. (November 2011), "Families among high-inclination asteroids", Icarus, 216 (1), pp. 69–81, arXiv:1108.3740
, Bibcode:2011Icar..216...69N, doi:10.1016/j.icarus.2011.08.016.
External links
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