151 Abundantia
| Discovery[1] | |
|---|---|
| Discovered by | J. Palisa |
| Discovery date | 1 November 1875 |
| Designations | |
Named after | Abundantia |
| Main belt | |
| Orbital characteristics[2][3] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 131.24 yr (47936 d) |
| Aphelion | 2.6792 AU (400.80 Gm) |
| Perihelion | 2.5049 AU (374.73 Gm) |
| 2.5921 AU (387.77 Gm) | |
| Eccentricity | 0.033623 |
| 4.17 yr (1524.3 d) | |
| 141.90° | |
| 0° 14m 10.212s / day | |
| Inclination | 6.4348° |
| 38.872° | |
| 130.92° | |
| Earth MOID | 1.51246 AU (226.261 Gm) |
| Jupiter MOID | 2.28656 AU (342.065 Gm) |
| Jupiter Tisserand parameter | 3.409 |
| Physical characteristics | |
| Dimensions | 45.37±0.9 km |
| 9.864 h (0.4110 d) | |
|
0.1728±0.007[3] 0.173[4] | |
| S[5] | |
| 9.1 | |
|
| |
151 Abundantia is a stony main belt asteroid. It was discovered by Johann Palisa on November 1, 1875, from the Austrian Naval Observatory in Pula. The name was chosen by Edmund Weiss of the Vienna Observatory; although the name refers to Abundantia, a Roman goddess of luck, it was also chosen to celebrate the increasing numbers of asteroids that were being discovered in the 1870s.[6]
Information from A. Harris as of March 1, 2001: 151 Abundantia is an S class (stony) asteroid with a diameter of 45.37 km and H = 9.24 .1728 and albedo of 0.03.
The light curve collected over 6 nights from 2/16/2002 to 3/10/2002 confirmed the rotational period to be 19.718h.
Data from 2001 shows a diameter of 45.37 km.[7]
References
- ↑ Harvard, Numbured MPs
- ↑ "The Asteroid Orbital Elements Database". astorb. Lowell Observatory.
- 1 2 "151 Abundantia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
- ↑ DSN IRAS
- ↑ LCSUMPUB
- ↑ Lutz D. Schmadel, Dictionary of Minor Planet Names, p.29.
- ↑ "151 Abundantia". Archived from the original on 2009-05-02. Retrieved 2009-03-11.
External links
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