.png) A three-dimensional model of 572 Rebekka based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | Paul Götz |
| Discovery site | Heidelberg |
| Discovery date | 19 September 1905 |
| Designations | |
| (572) Rebekka | |
| Pronunciation | /rɪˈbɛkə/[1] German: [ʁeːˈbɛkaː][2] |
| 1905 RB | |
| Orbital characteristics[3] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 109.81 yr (40108 d) |
| Aphelion | 2.7789 AU (415.72 Gm) |
| Perihelion | 2.0213 AU (302.38 Gm) |
| 2.4001 AU (359.05 Gm) | |
| Eccentricity | 0.15782 |
| 3.72 yr (1358.1 d) | |
| 272.796° | |
| 0° 15m 54.252s / day | |
| Inclination | 10.580° |
| 194.566° | |
| 192.111° | |
| Physical characteristics | |
| 14.815±0.45 km | |
| 5.6497 h (0.23540 d) | |
| 0.0847±0.005 | |
| 10.94 | |
572 Rebekka is a minor planet orbiting the Sun, which was discovered on September 19, 1905, by a German astronomer Paul Götz in Heidelberg. It was named after a young lady from Heidelberg, and may have been inspired by the asteroid's provisional designation 1905 RB.
Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light curve with a period of 5.656 ± 0.002 hours with a brightness range of 0.40 ± 0.02 in magnitude. This agrees with the 5.65 hour period measured in 1998.[4]
- ^ 'Rebecca' in Noah Webster (1884) A Practical Dictionary of the English Language
- ^ (German Names)
- ^ "572 Rebekka (1905 RB)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- ^ Cite error: The named reference
Warner2007was invoked but never defined (see the help page).