152 Atala
A three-dimensional model of 152 Atala based on its light curve. | |
Discovery[1] | |
---|---|
Discovered by | P. P. Henry |
Discovery site | discovery_site |
Discovery date | 1875 |
Designations | |
Named after | Atala |
Main belt | |
Orbital characteristics[2][3] | |
Aphelion | 3.374 AU |
Perihelion | 2.918 AU |
3.146 AU | |
Eccentricity | 0.072 |
5.582 years | |
Physical characteristics | |
Dimensions |
65 ± 8 km[4] 71–122 km[5] |
Mass | (5.43 ± 1.24) × 1018[6] kg |
Sidereal rotation period | 5.28-6.25 hours |
Albedo | 0.054 |
Spectral type | D[7] |
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.[8] The Henry brothers also named the last of their discoveries, 186 Celuta, after another Chateaubriand heroine.[9] Both Atala and Céluta are American Indian fictional characters.[10]
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.[11]
References
- ↑ Hardard's Numbered MPs
- ↑ Lowell Astorb
- ↑ Yeomans, Donald K., "152 Atala", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-30.
- ↑ Ďurech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanuš, Josef; Frappa, Eric; Talbot, John; Hayamizu, Tsutomu; Warner, Brian D.; Pilcher, Frederick; Galád, Adrián (2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes". Icarus 214 (2): 652–670. arXiv:1104.4227. Bibcode:2011Icar..214..652D. doi:10.1016/j.icarus.2011.03.016.
- ↑ Asterodoccultation.com
- ↑ Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ↑ SPIFF LCSUMPUB
- ↑ Schmadel, Lutz D.; International Astronomical Union (2003). Dictionary of minor planet names. Berlin; New York: Springer-Verlag. p. 29. ISBN 978-3-540-00238-3. Retrieved 9 September 2011.
- ↑ Schmadel, Lutz D.; International Astronomical Union (2012). Dictionary of minor planet names (6 ed.). Berlin; New York: Springer-Verlag. p. 29. ISBN 9783642297182. Retrieved 4 April 2014.
- ↑ Chateaubriand, François-René (1801). Atala.; Chateaubriand, François-René (1802). René.
- ↑ Schober, H. J. (July 1983), "The large C-type asteroids 146 Lucina and 410 Chloris, and the small S-type asteroids 152 Atala and 631 Philippina - Rotation periods and lightcurves", Astronomy and Astrophysics Supplement Series 53: 71–75, Bibcode:1983A&AS...53...71S.
External links
- Orbital simulation from JPL (Java) / Ephemeris
- Occultation of TYC 5558-01048-1 by (152) Atala on 2006 May 7 UT
- (152) Atala near opposition July 5, 2007 (2.38AU from Earth)
|
|