(92) Undina
Asteroid (92) Undina |
|
---|---|
Properties of the orbit ( animation ) | |
Orbit type | Outer main belt |
Major semi-axis | 3.19 AU |
eccentricity | 0.102 |
Perihelion - aphelion | 2.864 AU - 3.516 AU |
Inclination of the orbit plane | 9.9 ° |
Length of the ascending node | 101.8 ° |
Argument of the periapsis | 241.9 ° |
Time of passage of the perihelion | October 31, 2010 |
Sidereal period | 5 a 255 d |
Mean orbital velocity | 16.6 km / s |
Physical Properties | |
Medium diameter | 126 km |
Dimensions | (4.43 ± 0.25) 10 17 | kg
Albedo | 0.2509 |
Medium density | 4.39 ± 0.42 g / cm³ |
Rotation period | 15 h 56 min |
Absolute brightness | 6.61 likes |
Spectral class | M (Tholen), Xc (Bus) |
history | |
Explorer | CHF Peters |
Date of discovery | July 7, 1867 |
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items. |
(92) Undina is an asteroid of the main outer belt that was discovered on July 7, 1867 by the German-American astronomer Christian Heinrich Friedrich Peters .
The asteroid was named after Undine , a short story by the German poet Friedrich de la Motte Fouqué .
nature
Undina has a light, silicate-containing surface with an albedo of 0.251. Originally classified as a representative of the spectral class X, a more detailed spectral investigation in 2004-2005 indicated that it should rather be classified as an M-asteroid. Signs of a weak spectral band at 9 microns suggest the presence of orthopyroxene associated with an iron or pallasite composition. For (92) Undina a composition similar to the Esquel meteorite was proposed. In addition to (92) Undine, the asteroids (417) Suevia and (1124) Stroobantia with a similar composition were identified.
See also
Individual evidence
- ↑ a b Benoit Carry Density of Asteriods , Planetary & Space Science, 2012, Volume 73, Issue 1, pp. 98–118, doi: 10.1016 / j.pss.2012.03.009
- ^ Discovery Circumstances: Numbered Minor Planets. The international Astronomical Union - Minor Planet Center, accessed August 7, 2020 .
- ↑ S.Fornasier BEClark E.Dotto Spectroscopic Survey of X-type Asteroids , Icarus 214 (1), pp 131-146, 2011 arXiv: 1105.3380