160 Una
A three-dimensional model of 160 Una based on its light curve. | |
Discovery | |
---|---|
Discovered by | C. H. F. Peters |
Discovery date | February 20, 1876 |
Designations | |
Main belt | |
Orbital characteristics[1] | |
Epoch January 30, 2005 (JD 2453400.5) | |
Aphelion | 435.556 Gm (2.912 AU) |
Perihelion | 380.561 Gm (2.544 AU) |
408.058 Gm (2.728 AU) | |
Eccentricity | 0.067 |
1645.485 d (4.51 a) | |
Average orbital speed | 18.01 km/s |
308.565° | |
Inclination | 3.824° |
8.856° | |
49.974° | |
Physical characteristics | |
Dimensions | 81.2 km |
Mass | 5.6×1017 kg (assumed) |
Mean density | 2.0? g/cm³ |
0.0227 m/s² | |
0.0429 km/s | |
0.234 d (5.61[2] h) 1 | |
Albedo | 0.063 3 |
Temperature | ~170 K |
Spectral type | C 2 |
8.95[3] | |
|
160 Una is a fairly large and dark, primitive Main belt asteroid that was discovered by German-American astronomer C. H. F. Peters on February 20, 1876, in Clinton, New York.[4] It is named after a character in Edmund Spenser's epic poem The Faerie Queene (1590).
In the Tholen classification system it is categorized as a CX-type, while the Bus asteroid taxonomy system lists it as an Xk asteroid.[5] Photometric observations of this asteroid made at the Torino Observatory in Italy during 1990–1991 were used to determine a synodic rotation period of 5.61 ± 0.01 hours.[2]
References
- ↑ Yeomans, Donald K., "160 Una", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-25.
- 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.
- ↑ Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers 34, pp. 113–119, Bibcode:2007MPBu...34..113W.
- ↑ "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), retrieved 2013-04-07.
- ↑ DeMeo, Francesca E.; et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus 202 (1), pp. 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.2009.02.005, retrieved 2013-04-08. See appendix A.
External links
- Orbital simulation from JPL (Java) / Ephemeris
- 2011-Jan-24 Occultation / (2011 Asteroidal Occultation Results for North America)
- 160 Una at the JPL Small-Body Database
|
|
This article is issued from Wikipedia - version of the Friday, January 29, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.