3255 Tholen
Discovery [1] | |
---|---|
Discovered by | E. Bowell |
Discovery site | Anderson Mesa Stn. |
Discovery date | 2 September 1980 |
Designations | |
MPC designation | 3255 Tholen |
Named after |
David J. Tholen (astronomer)[2] |
1980 RA · 1969 SD | |
Mars-crosser [1][3][4] | |
Orbital characteristics [1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 45.63 yr (16,667 days) |
Aphelion | 3.2355 AU |
Perihelion | 1.5086 AU |
2.3720 AU | |
Eccentricity | 0.3640 |
3.65 yr (1,334 days) | |
257.34° | |
0° 16m 11.28s / day | |
Inclination | 21.355° |
337.22° | |
79.171° | |
Earth MOID | 0.6644 AU |
Physical characteristics | |
Dimensions |
5.07 km (derived)[4] ±0.17 km 6.76[5] |
±0.001 h 2.947[6] ±0.02 2.95h[lower-alpha 1] ±0.01 h 2.95[lower-alpha 1] ±1 h 3[7] h 6[8] | |
±0.008 0.142[5] 0.20 (assumed)[4] | |
SMASS = S [1] · S [4] | |
13.4[1] 13.60[5] ±0.04 13.84[4][7][9] | |
|
3255 Tholen, provisional designation 1980 RA, is a stony and relatively fast rotating asteroid and Mars-crosser, approximately 6 kilometers in diameter. It was discovered on 2 September 1980, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona.[3]
The S-type asteroid orbits the Sun at a distance of 1.5–3.2 AU once every 3 years and 8 months (1,334 days). Its orbit has an eccentricity of 0.36 and an inclination of 21° with respect to the ecliptic.[1] The first observation was made at the Argentinian El Leoncito site in 1969, extending the asteroid's observation arc by 11 years prior to its discovery.[3]
According to the space-based survey carried out by the Japanese Akari satellite, the asteroid measures 6.8 kilometers in diameter and its surface has an albedo of 0.14,[5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.1 kilometers, based on an absolute magnitude of 13.84.[4]
Several rotational light-curves were obtained for this asteroid from photometric observations. In September 2013, Italian astronomer Andrea Ferrero at the Bigmuskie Observatory (B88) in Mombercelli, Italy, derived a rotation period of ±0.001 hours with a brightness variation of 0.11 in 2.947magnitude (U=2), while two month later, in November 2013, astronomer Brian A. Skiff obtained two light-curves that both gave a period of 2.95 and an amplitude of 0.24 and 0.28 in magnitude, respectively (U=3-/3-).[lower-alpha 1] The results supersede two older light-curves from 1991 and 2002, that gave a period of ±1 and 6 hours, respectively ( 3U=1/1).[7][8]
The minor planet was named after David J. Tholen (b. 1955), a discoverer of minor planets and planetary scientist at the Institute for Astronomy of the University of Hawaii, known for his eight-color taxonomic scheme on minor planets.[2] Naming citation was published on 14 April 1987 (M.P.C. 11749).[10]
References
- 1 2 3 Skiff (2013) web: rotation period ±0.01 and 2.95±0.02 hours with a brightness amplitude of 2.95 and 0.24 mag, respectively. Summary figures at 0.28Collaborative Asteroid Lightcurve Link (CALL) for (3255) Tholen, Skiff, B.A. (2013) Posting on CALL web site.
- 1 2 3 4 5 6 "JPL Small-Body Database Browser: 3255 Tholen (1980 RA)" (2015-05-08 last obs.). Jet Propulsion Laboratory. Retrieved 13 August 2016.
- 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (3255) Tholen. Springer Berlin Heidelberg. p. 271. ISBN 978-3-540-00238-3. Retrieved 13 August 2016.
- 1 2 3 "3255 Tholen (1980 RA)". Minor Planet Center. Retrieved 13 August 2016.
- 1 2 3 4 5 6 "LCDB Data for (3255) Tholen". Asteroid Lightcurve Database (LCDB). Retrieved 13 August 2016.
- 1 2 3 4 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey" (PDF). Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 13 August 2016.
- ↑ Ferrero, Andrea (January 2014). "Period Determination of Four Main-belt Asteroids in Mid-2013". The Minor Planet Bulletin. 41 (1): 24–25. Bibcode:2014MPBu...41...24F. ISSN 1052-8091. Retrieved 13 August 2016.
- 1 2 3 Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids". Abstracts of the Lunar and Planetary Science Conference. Bibcode:1995LPI....26.1511W. Retrieved 13 August 2016.
- 1 2 Behrend, Raoul. "Asteroids and comets rotation curves – (3255) Tholen". Geneva Observatory. Retrieved 13 August 2016.
- ↑ Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. Retrieved 13 August 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 13 August 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 3255 Tholen at the JPL Small-Body Database