145 Adeona
Discovery[1] | |
---|---|
Discovered by | Christian Heinrich Friedrich Peters |
Discovery date | June 3, 1875 |
Designations | |
Named after
|
Adeona |
Main belt, adeona family | |
Orbital characteristics[2] | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 457.677 Gm (3.059 AU) |
Perihelion | 341.958 Gm (2.286 AU) |
399.817 Gm (2.673 AU) | |
Eccentricity | 0.145 |
1595.888 d (4.37 a) | |
Average orbital speed
|
18.12 km/s |
163.291° | |
Inclination | 12.637° |
77.454° | |
44.899° | |
Physical characteristics | |
Dimensions | 149.50 ± 5.45[1] km |
Mass | (2.08 ± 0.57) × 1018[1] kg |
Mean density
|
1.18 ± 0.34[1] g/cm3 |
Equatorial surface gravity
|
0.0422 m/s² |
Equatorial escape velocity
|
0.0799 km/s |
0.0467 ± 0.0116[2] | |
Temperature | ~170 K |
C (Tholen)[2] | |
8.050[2] | |
145 Adeona is a rather large main-belt asteroid. Its surface is very dark,[2] and, based upon its classification as a C-type asteroid, is probably composed of primitive carbonaceous material. 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.[3]
During 2001, 145 Adeona was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 151 ± 18 km. This is consistent with the asteroid dimensions computed through other means.[4]
Adeona has been observed to occult a star once, on July 9, 2002.[citation needed]
References
- ↑ 1.0 1.1 1.2 Lua error in package.lua at line 80: module 'strict' not found. See Table 1.
- ↑ 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found. See Table 4.
- ↑ Lutz D. Schmadel, Dictionary of Minor Planet Names, p.28.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
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