Astronomy:(9942) 1989 TM1
| Discovery[1] | |
|---|---|
| Discovered by | T. Hioki N. Kawasato |
| Discovery site | Okutama Obs. |
| Discovery date | 8 October 1989 |
| Designations | |
| (9942) 1989 TM1 | |
| 1989 TM1 | |
| Minor planet category | main-belt[1][2] · (middle)[3] background |
| Orbital characteristics[2] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 26.64 yr (9,732 days) |
| |{{{apsis}}}|helion}} | 3.0287 AU |
| |{{{apsis}}}|helion}} | 2.1619 AU |
| 2.5953 AU | |
| Eccentricity | 0.1670 |
| Orbital period | 4.18 yr (1,527 days) |
| Mean anomaly | 217.94° |
| Mean motion | 0° 14m 8.52s / day |
| Inclination | 9.9393° |
| Longitude of ascending node | 21.747° |
| 38.492° | |
| Physical characteristics | |
| Mean diameter | 4.12±0.45 km[4] 4.73 km (calculated)[3] |
| Rotation period | 3.0706±0.0004 h[5] |
| Geometric albedo | 0.20 (assumed)[3] 0.454±0.106[4] |
| S (assumed)[3] | |
| Absolute magnitude (H) | 13.40[4] · 13.541[5] 13.6[2] · 13.99[3] |
(9942) 1989 TM1 (provisional designation 1989 TM1) is a background asteroid from the central region of the asteroid belt, approximately 4.5 kilometers (2.8 miles) in diameter. It was discovered on 8 October 1989, by Japanese astronomers Nobuhiro Kawasato and Tsutomu Hioki at the Okutama Observatory (877) in Japan.[1] The asteroid has a tentative rotation period of 3.1 hours.[3]
Orbit and classification
The assumed stony S-type is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 2.2–3.0 AU once every 4 years and 2 months (1,527 days; semi-major axis of 2.6 AU). Its orbit has an eccentricity of 0.17 and an inclination of 10° with respect to the ecliptic.[2]
Its first observation was a precovery taken at the Palomar Observatory on 30 September 1989, extending the asteroid's observation arc by just 9 days prior to its official discovery observation.[1]
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 2 February 1999.[6] As of 2018, it has not been named.[1]
Physical characteristics
Diameter and albedo
The asteroid was predicted to cross the focal plane array of the Infrared Astronomical Satellite (IRAS). However, it was missed on each of its seven planned observation and was never detected. According to the "missed predictions file" of the supplemental IRAS minor planet survey (SIMPS), the body was expected to have a diameter of 13.5 kilometers and an absolute magnitude of 13.20.[7]
Based on an absolute magnitude of 13.99, and an assumed standard albedo for stony asteroids of 0.20, the Collaborative Asteroid Lightcurve Link calculated a much smaller diameter of 4.7 kilometers,[3] which agrees with a diameter of 4.1 kilometers, found by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission.[4]
Rotation period
In October 2010, a rotational lightcurve for this asteroid was obtained from photometric observations at the Palomar Transient Factory in California. It rendered a tentative rotation period of 3.0706±0.0004 hours with a brightness variation of 0.08 in magnitude ({{{1}}}).[5]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 "9942 (1989 TM1)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=9942. Retrieved 13 September 2018.
- ↑ 2.0 2.1 2.2 2.3 "JPL Small-Body Database Browser: 9942 (1989 TM1)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2009942. Retrieved 13 September 2018.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 "LCDB Data for (9942)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=9942%7C. Retrieved 4 July 2016.
- ↑ 4.0 4.1 4.2 4.3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C. et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M.
- ↑ 5.0 5.1 5.2 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal 150 (3): 35. doi:10.1088/0004-6256/150/3/75. Bibcode: 2015AJ....150...75W.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 13 September 2018.
- ↑ Tedesco E.F.; Noah P.V.. "The supplemental IRAS minor planet survey (SIMPS) – Missed-Predictions". http://iopscience.iop.org/1538-3881/123/2/1056/fulltext/FP206.txt.
External links
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
- (9942) 1989 TM1 at AstDyS-2, Asteroids—Dynamic Site
- (9942) 1989 TM1 at the JPL Small-Body Database
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