1159 Granada
Discovery | |
---|---|
Discovered by | Reinmuth, K. |
Discovery date | 2 September 1929 |
Orbital characteristics [1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 86.62 yr (31638 days) |
Aphelion | 2.5181146 AU (376.70458 Gm) |
Perihelion | 2.2411377 AU (335.26943 Gm) |
2.3796261 AU (355.98700 Gm) | |
Eccentricity | 0.0581976 |
3.67 yr (1340.8 d) | |
287.94963° | |
0° 16m 6.593s / day | |
Inclination | 13.03125° |
347.89028° | |
313.13819° | |
Earth MOID | 1.24452 AU (186.178 Gm) |
Jupiter MOID | 2.65658 AU (397.419 Gm) |
Jupiter Tisserand parameter | 3.502 |
Physical characteristics | |
Mean radius | ±0.45 14.99km |
31 h (1.3 d) | |
±0.003 0.0471 | |
11.55 | |
|
1159 Granada is a main belt asteroid orbiting the Sun. Approximately 30 kilometers in diameter, it makes a revolution around the Sun once every 4 years. It completes one rotation once every 31 hours. It was discovered by Karl Wilhelm Reinmuth at Heidelberg, Germany on September 2, 1929. Its provisional designation was 1929 RD.[1] It is named after the Spanish province of Granada.[2]
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