145 Adeona
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Discovery[1] and designation
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| Discovered by | Christian Heinrich Friedrich Peters |
| Discovery date | June 3, 1875 |
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Designations
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| Named after | Adeona |
| Alternate name(s) | |
| Minor planet category |
Main belt |
| Epoch December 31, 2006 (JD 2454100.5) | |
| Aphelion | 457.677 Gm (3.059 AU) |
| Perihelion | 341.958 Gm (2.286 AU) |
| Semi-major axis | 399.817 Gm (2.673 AU) |
| Eccentricity | 0.145 |
| Orbital period | 1595.888 d (4.37 a) |
| Average orbital speed | 18.12 km/s |
| Mean anomaly | 163.291° |
| Inclination | 12.637° |
| Longitude of ascending node | 77.454° |
| Argument of perihelion | 44.899° |
| Dimensions | 151.1 km |
| Mass | 3.6×1018 kg |
| Mean density | 2.0 g/cm³ |
| Equatorial surface gravity | 0.0422 m/s² |
| Equatorial escape velocity | 0.0799 km/s |
| Sidereal rotation period |
? d |
| Axial tilt | ?° |
| Pole ecliptic latitude | ? |
| Pole ecliptic longitude | ? |
| Geometric albedo | 0.10 |
| Temperature | ~170 K |
| Spectral type | C |
| Absolute magnitude (H) | 8.13 |
145 Adeona is a rather large main-belt asteroid. Its surface is very dark, and probably composed of primitive carbonaceous material.[citation needed] The Adeona family of asteroids is named after it.
It was discovered by C. H. F. Peters on June 3, 1875, from the observatory at Hamilton College, Clinton, New York. Peters named it after Adeona, the Roman goddess of homecoming, because he had recently returned from a journey across the world to observe the transit of Venus. Peters also discovered 144 Vibilia on the same night.[1]
Adeona has been observed to occult a star once, on July 9, 2002.[citation needed]
[edit] References
- ^ Lutz D. Schmadel, Dictionary of Minor Planet Names, p.28.
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