1175 Margo
Discovery [1] | |
---|---|
Discovered by | Karl Wilhelm Reinmuth |
Discovery site | Heidelberg-Königstuhl State Observatory |
Discovery date | 17 October 1930 |
Designations | |
MPC designation | 1175 |
1930 UD | |
outer main-belt asteroid [2] | |
Orbital characteristics [2][3] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 107.71 yr (39342 days) |
Aphelion | 3.4336 AU (513.66 Gm) |
Perihelion | 2.9982 AU (448.52 Gm) |
3.2159 AU (481.09 Gm) | |
Eccentricity | 0.067691 |
5.77 yr (2106.5 d) | |
352.80° | |
0° 10m 15.24s / day | |
Inclination | 16.305° |
237.195° | |
102.908° | |
Earth MOID | 2.04546 AU (305.996 Gm) |
Jupiter MOID | 1.85791 AU (277.939 Gm) |
Jupiter Tisserand parameter | 3.124 |
Physical characteristics | |
11.99 ± 0.03 hours,[4] 6.01 h (0.250 d) [2] | |
10.2,[5] 10.0 [2] | |
|
1175 Margo (1930 UD) is an outer main-belt asteroid discovered on October 17, 1930, by Karl Wilhelm Reinmuth at Heidelberg-Königstuhl State Observatory.[1] The origin of the name Margo is unknown.[6]
References
- 1 2 "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". IAU: Minor Planet Center. Archived from the original on 2 February 2009. Retrieved December 22, 2008.
- 1 2 3 4 "1175 Margo (1930 UD)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 1 May 2016.
- ↑ "(1175) Margo". AstDyS. Italy: University of Pisa. Retrieved December 22, 2008.
- ↑ Oliver; et al. (2008). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2008 March". The Minor Planet Bulletin 35 (4): 149–150. Bibcode:2008MPBu...35..149O.
- ↑ Tholen (2007). "Asteroid Absolute Magnitudes". EAR-A-5-DDR-ASTERMAG-V11.0. Planetary Data System. Archived from the original on 1 December 2008. Retrieved December 26, 2008.
- ↑ Schmadel, Lutz (2003). Dictionary of minor planet names (fifth ed.). Germany: Springer. p. 99. ISBN 3-540-00238-3. Retrieved 2008-12-26.
External links
|
|
This article is issued from Wikipedia - version of the Sunday, May 01, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.