(230) Athamantis
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Asteroid (230) Athamantis |
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| Properties of the orbit ( animation ) | |
| Orbit type | Inner main belt |
| Major semi-axis | 2.382 AU |
| eccentricity | 0.062 |
| Perihelion - aphelion | 2.235 AU - 2.529 AU |
| Inclination of the orbit plane | 9.4 ° |
| Length of the ascending node | 239.9 ° |
| Argument of the periapsis | 140.2 ° |
| Time of passage of the perihelion | September 23, 2011 |
| Sidereal period | 3 a 247 d |
| Mean orbital velocity | 19.3 km / s |
| Physical Properties | |
| Medium diameter | 109 km |
| Albedo | 0.1708 |
| Rotation period | 24 h 0 min |
| Absolute brightness | 7.35 likes |
| Spectral class | S. |
| history | |
| Explorer | LAC de Ball |
| Date of discovery | September 3, 1882 |
| Another name | 1949 flat share |
| 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. | |
(230) Athamantis is an asteroid of the asteroid belt that was discovered on September 3, 1882 by Leo Anton Carl de Ball at the Bothkamp observatory near Kiel . De Ball had actually wanted to observe the asteroid (12) Victoria that night .
The celestial body was named after Athamantis (or Helle ), the daughter of Athamas, king of Thebes , from Greek mythology . Since Athamantis was very "bright" at the time, this could have inspired de Ball to give the name.
Athamantis moves 2.2353 ( perihelion ) to 2.5293 ( aphelion ) astronomical units around the Sun in 3.6771 years . The orbit is inclined 9.4344 ° to the ecliptic , the orbital eccentricity is 0.0617.
Athamantis has a diameter of 109 kilometers. The asteroid has a relatively bright, silicate-rich surface with an albedo of 0.171. It rotates around its own axis in around 23 hours and 59 minutes.
See also
- List of asteroids with references and web links (see also infobox)