729 Watsonia
Discovery | |
---|---|
Discovered by | Joel Hastings Metcalf |
Discovery site | Winchester, Massachusetts |
Discovery date | 9 February 1912 |
Designations | |
1912 OD | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 98.79 yr (36082 d) |
Aphelion | 3.0270 AU (452.83 Gm) |
Perihelion | 2.4917 AU (372.75 Gm) |
2.7594 AU (412.80 Gm) | |
Eccentricity | 0.096988 |
4.58 yr (1674.2 d) | |
223.02° | |
0° 12m 54.108s / day | |
Inclination | 18.042° |
124.388° | |
88.376° | |
Earth MOID | 1.56567 AU (234.221 Gm) |
Jupiter MOID | 2.17725 AU (325.712 Gm) |
Jupiter Tisserand parameter | 3.264 |
Physical characteristics | |
Mean radius | ±0.75 24.575km |
25.230 h (1.0513 d) | |
±0.009 0.1381 | |
9.31 | |
|
729 Watsonia is a minor planet orbiting the Sun. It was named after the Canadian-American astronomer James C. Watson. Asteroid (729) Watsonia occulted the star HIP 53417 (54 Leonis A/B, 4.3 Magnitude Star) on 2013 Mar 03 at 01:48.
This object is the namesake of a family of 31–139 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.[2]
References
- ↑ Yeomans, Donald K., "729 Watsonia", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 5 May 2016.
- ↑ 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
|
|
This article is issued from Wikipedia - version of the Friday, May 06, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.