Discovery | |
---|---|
Discovered by | LINEAR |
Discovery site | Lincoln Lab's ETS |
Discovery date | 4 January 2000 |
Designations | |
MPC designation | (19738) Calinger |
Named after | Manetta Calinger (DCYSC mentor) |
Alternative designations | 2000 AS97 · 1991 RZ36 |
Minor planet category | main-belt · inner background |
Orbital characteristics | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 26.88 yr (9,819 days) |
Aphelion | 2.7043 AU |
Perihelion | 1.8606 AU |
Semi-major axis | 2.2824 AU |
Eccentricity | 0.1848 |
Orbital period (sidereal) | 3.45 yr (1,260 days) |
Mean anomaly | 165.65° |
Mean motion | 0° 17 8.88 / day |
Inclination | 7.7356° |
Longitude of ascending node | 90.753° |
Argument of perihelion | 280.16° |
Physical characteristics | |
Dimensions | 3.272±0.082 |
Geometric albedo | 0.314±0.056 |
Absolute magnitude (H) | 14.1 |
19738 Calinger (provisional designation 2000 AS97) is a background asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter.
It was discovered on 4 January 2000, by members of the Lincoln Near-Earth Asteroid Research team at Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico, and named after DCYSC-mentor Manetta Calinger.
Classification and orbit
Calinger is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,260 days). Its orbit has an eccentricity of 0.18 and an inclination of 8° with respect to the ecliptic.
The body's observation arc begins almost 10 years prior to its official discovery observation, with a precovery from the Digitized Sky Survey taken at Palomar Observatory in May 1990.
Physical characteristics
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Calinger measures 3.272 kilometers in diameter and its surface has a high albedo of 0.314. It has an absolute magnitude of 14.1.
Lightcurves
As of 2017, Calinger's rotation period and shape remain unknown.
Naming
This minor planet was named after Manetta Calinger who mentored a finalist in the 2003 Discovery Channel Youth Science Challenge, DCYSC. The approved naming citation was published by the Minor Planet Center on 10 October 2003 (M.P.C. 49772).
References
- ^ "JPL Small-Body Database Browser: 19738 Calinger (2000 AS97)" (2017-03-31 last obs.). Jet Propulsion Laboratory. Retrieved 26 June 2017.
- ^ Schmadel, Lutz D. (2006). "(19738) Calinger ". Dictionary of Minor Planet Names – (19738) Calinger, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 142. doi:10.1007/978-3-540-34361-5_1596. ISBN 978-3-540-34361-5.
- ^ 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. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 9 March 2017.
- ^ "19738 Calinger (2000 AS97)". Minor Planet Center. Retrieved 9 March 2017.
- "LCDB Data for (19738) Calinger". Asteroid Lightcurve Database (LCDB). Retrieved 26 June 2017.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 9 March 2017.
External links
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (15001)-(20000) – Minor Planet Center
- 19738 Calinger at AstDyS-2, Asteroids—Dynamic Site
- 19738 Calinger at the JPL Small-Body Database
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