193 Ambrosia
|
A three-dimensional model of 193 Ambrosia based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | J. Coggia, 1879 |
| Discovery date | 28 February 1879 |
| Designations | |
| Main belt | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 100.12 yr (36569 d) |
| Aphelion | 3.3720 AU (504.44 Gm) |
| Perihelion | 1.8302 AU (273.79 Gm) |
| 2.6011 AU (389.12 Gm) | |
| Eccentricity | 0.29638 |
| 4.20 yr (1532.2 d) | |
| 331.40° | |
| 0° 14m 5.82s / day | |
| Inclination | 12.010° |
| 349.97° | |
| 81.365° | |
| Earth MOID | 0.887123 AU (132.7117 Gm) |
| Jupiter MOID | 2.13939 AU (320.048 Gm) |
| Jupiter Tisserand parameter | 3.321 |
| Physical characteristics | |
|
6.580 hours[2] 6.581 h (0.2742 d)[1] | |
| 0.10 | |
| 9.68 | |
|
| |
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193 Ambrosia is a main belt asteroid that was discovered by the French (Corsican) astronomer J. Coggia on February 28, 1879, and named after Ambrosia, the food of the gods in Greek mythology.[3]
In 2009, Photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting light curve shows a synodic rotation period of 6.580 ± 0.001 hours with a brightness variation of 0.11 ± 0.02 in magnitude. This result is consistent with an independent study performed in 1996.[2]
References
- 1 2 Yeomans, Donald K., "193 Ambrosia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 6 May 2016.
- 1 2 Warner, Brian D. (October 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 March-June", The Minor Planet Bulletin, 36 (4), pp. 172–176, Bibcode:2009MPBu...36..172W, doi:10.1016/j.pss.2012.03.009.
- ↑ http://markandrewholmes.com/ambrosia.html
External links
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