Discovery[1] | |
---|---|
Discovered by | C. J. van Houten I. van Houten G. T. Gehrels |
Discovery site | Palomar Obs. |
Discovery date | 24 September 1960 |
Designations | |
(1923) Osiris | |
Pronunciation | /əˈsaɪrɪs/[2] |
Named after | Osiris (Egyptian mythology)[3] |
4011 P-L · 1964 TO2 1966 FR · 1974 KN 1974 KP · 1974 LE | |
main-belt[4][1] · (inner) Sulamitis | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 62.70 yr (22,900 days) |
Aphelion | 2.5900 AU |
Perihelion | 2.2813 AU |
2.4356 AU | |
Eccentricity | 0.0634 |
3.80 yr (1,388 days) | |
269.38° | |
0° 15m 33.48s / day | |
Inclination | 4.9580° |
353.07° | |
106.04° | |
Physical characteristics | |
Dimensions | 13.1 km 13.461±0.206[5] |
0.031±0.006[5] 0.0591 ± 0.008 | |
SMASS = C[1] | |
13.6[1] | |
1923 Osiris, provisional designation 4011 P-L, is a dark asteroid from the inner regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 24 September 1960, by Ingrid and Cornelis Johannes van Houten at Leiden, on photographic plates taken by Tom Gehrels at Palomar Observatory in the United States.[4][6] It was named after the Egyptian god Osiris.[3]
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