126 Velleda
Discovery | |
---|---|
Discovered by | Paul Henry and Prosper Henry |
Discovery date | November 5, 1872 |
Designations | |
Named after | Veleda |
Main belt | |
Orbital characteristics | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 403.523 Gm (2.697 AU) |
Perihelion | 326.153 Gm (2.180 AU) |
364.838 Gm (2.438644[1] AU) | |
Eccentricity | 0.1060806[1] |
1391.107 d (3.81 a) | |
Average orbital speed | 19.02 km/s |
117.027° | |
Inclination | 2.92451°[1] |
23.47325°[1] | |
327.94065°[1] | |
Physical characteristics | |
Dimensions | 44.79 ± 1.33 km[2] |
Mass | (0.47 ± 5.79) × 1018 kg[2] |
0.0125 m/s² | |
0.0237 km/s | |
5.364 ± 0.003 d[3] | |
Albedo | 0.1723[1] |
Temperature | ~178 K |
Spectral type | S |
9.27[1] | |
|
126 Velleda is a main-belt asteroid. It is probably a rather typical, albeit sizable, S-type asteroid. Named for Veleda, a priestess and prophet of the Germanic tribe of the Bructeri. It was discovered by Paul Henry on November 5, 1872, in Paris, France. It was his first credited discovery. He and his brother Prosper Henry discovered a total of 14 asteroids.
This asteroid rotates once every 5 days, 8 hours and 44 minutes. During each rotation the light curve varies by 0.22 magnitudes.[3]
References
- 1 2 3 4 5 6 7 "126 Velleda". JPL Small-Body Database Browser. NASA JPL. 2003-08-29. Retrieved 2007-03-12.
- 1 2 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 Dovgopol, A. N.; Kruglyi, Iu. N.; Shevchenko, V. G. (1992). "Asteroid 126 Velleda - Rotation period and magnitude-phase curve". Acta Astronomica. 42 (1): 67–72. Bibcode:1992AcA....42...67D.
External links
This article is issued from Wikipedia - version of the 9/9/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.