Discovery [1] | |
---|---|
Discovered by | W. Liller |
Discovery site | Cerro Tololo Obs. |
Discovery date | 23 January 1979 |
Designations | |
(3040) Kozai | |
Named after | Yoshihide Kozai (Japanese astronomer)[2] |
1979 BA | |
Mars-crosser [1][3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 38.36 yr (14,011 days) |
Aphelion | 2.2096 AU |
Perihelion | 1.4717 AU |
1.8406 AU | |
Eccentricity | 0.2004 |
2.50 yr (912 days) | |
213.41° | |
Inclination | 46.640° |
143.51° | |
290.19° | |
Physical characteristics | |
Dimensions | 4–11 km (conversion)[4] |
SMASS = S [1] | |
13.8[1] | |
3040 Kozai, provisional designation 1979 BA, is a stony asteroid and Mars-crosser on a tilted orbit from the innermost regions of the asteroid belt, approximately 4 kilometers in diameters.
The asteroid was discovered by American astronomer William Liller at Cerro Tololo Inter-American Observatory in Chile, on 23 January 1979, and named after Japanese astronomer Yoshihide Kozai.[2][3] It is considered a classical example of an object submitted to the Kozai effect, induced by an outer perturber, which in this case is the gas giant Jupiter.[5]
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