Astronomy:3169 Ostro
_Ostro.gif) Ostro imaged by the 0.7-m telescope at Heidelberg Observatory | |
| Discovery [1] | |
|---|---|
| Discovered by | E. Bowell |
| Discovery site | Anderson Mesa Stn. |
| Discovery date | 4 June 1981 |
| Designations | |
| (3169) Ostro | |
| Named after | Steven J. Ostro (planetary scientist)[2] |
| 1981 LA | |
| Minor planet category | main-belt · (inner) [1] · Hungaria [3][4] |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 63.43 yr (23,166 days) |
| |{{{apsis}}}|helion}} | 2.0184 AU |
| |{{{apsis}}}|helion}} | 1.7652 AU |
| 1.8918 AU | |
| Eccentricity | 0.0669 |
| Orbital period | 2.60 yr (950 days) |
| Mean anomaly | 120.41° |
| Mean motion | 0° 22m 43.68s / day |
| Inclination | 24.906° |
| Longitude of ascending node | 96.376° |
| 32.622° | |
| Physical characteristics | |
| Dimensions | 4.662±0.118[5] 5.27 km (derived)[4] |
| Rotation period | 6.503±0.003[6] |
| Geometric albedo | 0.5152 (derived)[4] 0.960±0.023[5] |
| TS (Tholen)[1] Xe (SMASS)[1] B–V = 0.771[1] U–B = 0.306[1] | |
| Absolute magnitude (H) | 12.73[1][4] |
3169 Ostro, provisional designation 1981 LA, is a Hungaria family asteroid from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter.
The asteroid was discovered on 4 June 1981, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona,[3] and named after planetary scientist Steven J. Ostro at JPL.[2]
Orbit and classification
Ostro is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.8–2.0 AU once every 2 years and 7 months (950 days). Its orbit has an eccentricity of 0.07 and an inclination of 25° with respect to the ecliptic.[1]
Physical characteristics
In the Tholen and SMASS taxonomy, Ostro is classified as a TS-type and Xe-type asteroid, respectively.[1] It has also been characterized as an E-type asteroid.[4]
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Ostro measures 4.662 kilometers in diameter and its surface has an outstandingly high albedo of 0.960.[5] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.5152 and a diameter of 5.27 kilometers with an absolute magnitude of 12.73.[4]
In May 2012, a rotational lightcurve of Ostro was obtained from photometric observations by American astronomer Brian Warner. Lightcurve analysis gave a well-defined rotation period of 6.503 hours with a brightness amplitude of 0.79 magnitude ({{{1}}}).[6]
Naming
This minor planet was named after American planetary scientist Steven J. Ostro at the Jet Propulsion Laboratory of the California Institute of Technology.[2] The approved naming citation was published by the Minor Planet Center on 14 April 1987 (M.P.C. 11749).[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 "JPL Small-Body Database Browser: 3169 Ostro (1981 LA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003169.
- ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(3169) Ostro". Dictionary of Minor Planet Names – (3169) Ostro. Springer Berlin Heidelberg. p. 262. doi:10.1007/978-3-540-29925-7_3170. ISBN 978-3-540-00238-3.
- ↑ 3.0 3.1 "3169 Ostro (1981 LA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=3169.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 "LCDB Data for (3169) Ostro". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=3169%7COstro.
- ↑ 5.0 5.1 5.2 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J. et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal 741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 15 June 2017.
- ↑ 6.0 6.1 Warner, Brian D. (October 2012). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2012 March - June". The Minor Planet Bulletin 39 (4): 245–252. ISSN 1052-8091. Bibcode: 2012MPBu...39..245W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012MPBu...39..245W. Retrieved 15 June 2017.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
External links
- Lightcurve plot of 3169 Ostro, Palmer Divide Observatory, B. D. Warner (2012)
- Asteroid Lightcurve Database (LCDB), query form (info )
- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- 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
- 3169 Ostro at AstDyS-2, Asteroids—Dynamic Site
- 3169 Ostro at the JPL Small-Body Database
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