1109 Tata
| Discovery | |
|---|---|
| Discovered by | Reinmuth, K. at Heidelberg (024) |
| Discovery date | 5 February 1929 |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 87.20 yr (31850 days) |
| Aphelion | 3.5415339 AU (529.80593 Gm) |
| Perihelion | 2.907934 AU (435.0207 Gm) |
| 3.224734 AU (482.4133 Gm) | |
| Eccentricity | 0.09824065 |
| 5.79 yr (2115.1 d) | |
| 355.09839° | |
| 0° 10m 12.725s / day | |
| Inclination | 4.120524° |
| 268.09963° | |
| 359.13943° | |
| Earth MOID | 1.89178 AU (283.006 Gm) |
| Jupiter MOID | 1.53613 AU (229.802 Gm) |
| TJupiter | 3.176 |
| Physical characteristics | |
Mean radius | 33.265±0.7 km |
| 8.277 h (0.3449 d) | |
| 0.0378±0.002 | |
| 10.06 | |
1109 Tata is a main belt asteroid orbiting the Sun. It was discovered by Karl Wilhelm Reinmuth on February 5, 1929, at Heidelberg, Germany. Its provisional designation was 1929 CU. The origin of its name is unknown.[2]
References
- ^ a b "1109 Tata (1929 CU)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 2 May 2016.
- ^ Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names. Springer. ISBN 3-540-00238-3.
External links
- 1109 Tata at the JPL Small-Body Database
