382 Dodona
|
A three-dimensional model of 382 Dodona based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 29 January 1894 |
| Designations | |
Named after | Dodona |
| 1894 AT | |
| Main belt | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 122.21 yr (44636 d) |
| Aphelion | 3.6577 AU (547.18 Gm) |
| Perihelion | 2.58301 AU (386.413 Gm) |
| 3.1204 AU (466.81 Gm) | |
| Eccentricity | 0.17221 |
| 5.51 yr (2013.3 d) | |
Average orbital speed | 16.87 km/s |
| 6.32892° | |
| 0° 10m 43.716s / day | |
| Inclination | 7.3928° |
| 313.511° | |
| 270.036° | |
| Earth MOID | 1.58765 AU (237.509 Gm) |
| Jupiter MOID | 1.46431 AU (219.058 Gm) |
| Jupiter Tisserand parameter | 3.181 |
| Physical characteristics | |
| Dimensions |
58.37±2.8 km[1] 58.37 km[2] |
| 4.113 h (0.1714 d) | |
|
0.1610±0.017[1] 0.161[2] | |
| M | |
| 8.77[1][2] | |
|
| |
.png)
382 Dodona is a large Main belt asteroid that was discovered by the French astronomer Auguste Charlois on January 29, 1894 in Nice. It is classified as an M-type asteroid.
Measurements of the thermal inertia of 115 Thyra give an estimated range of 15–150 J m−2 K−1 s−1/2, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere.[2]
References
- 1 2 3 4 "382 Dodona (1894 AT)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 10 May 2016.
- 1 2 3 4 Delbo', Marco; Tanga, Paolo (February 2009), "Thermal inertia of main belt asteroids smaller than 100 km from IRAS data", Planetary and Space Science, 57 (2), pp. 259–265, arXiv:0808.0869
, Bibcode:2009P&SS...57..259D, doi:10.1016/j.pss.2008.06.015.
External links
This article is issued from Wikipedia - version of the 9/10/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.