152 Atala
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A three-dimensional model of 152 Atala based on its light curve.
|
|
| Discovery | |
|---|---|
| Discovered by | P. P. Henry |
| Discovery site | discovery_site |
| Discovery date | 2 November 1875 |
| Designations | |
| MPC designation | (152) Atala |
|
Named after
|
Atala |
| Main belt | |
| Orbital characteristics | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 130.69 yr (47735 d) |
| Aphelion | 3.3855 AU (506.46 Gm) |
| Perihelion | 2.8984 AU (433.59 Gm) |
| 3.1420 AU (470.04 Gm) | |
| Eccentricity | 0.077507 |
| 5.57 yr (2034.2 d) | |
| 52.593° | |
| 0° 10m 37.092s / day | |
| Inclination | 12.114° |
| 39.945° | |
| 59.807° | |
| Earth MOID | 1.93567 AU (289.572 Gm) |
| Jupiter MOID | 1.85235 AU (277.108 Gm) |
| Jupiter Tisserand parameter | 3.171 |
| Physical characteristics | |
| Dimensions | 65 ± 8 km 71–122 km |
| Mass | (5.43 ± 1.24) × 1018 kg |
| 6.246 h (0.2603 d) | |
|
Sidereal rotation period
|
5.28-6.25 hours |
| 0.054 | |
| D | |
| 8.33 | |
152 Atala is a large main belt asteroid that was discovered by brothers Paul Henry and Prosper Henry on November 2, 1875, but the discovery was credited to Paul. It is a type D asteroid, meaning that it is composed of carbon, organic rich silicates and possibly water ice.
The asteroid is named for the eponymous heroine of the 1801 novella Atala by François-René de Chateaubriand. The Henry brothers also named the last of their discoveries, 186 Celuta, after another Chateaubriand heroine. Both Atala and Céluta are American Indian fictional characters.
An occultation of a star by Atala was observed from Japan on March 11, 1994. Subsequent occultations have been observed as recently as 2006.
Photometric of this asteroid made in 1981 gave a light curve with a period of 5.282 ± 0.004 hours with a brightness variation of 0.50 in magnitude.
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