978 Aidamina
| Discovery [1] | |
|---|---|
| Discovered by | S. Belyavskyj |
| Discovery site | Simeiz Observatory |
| Discovery date | 18 May 1922 |
| Designations | |
| 978 Aidamina | |
Named after | Aida Minaevna (friend of discoverer)[2] |
| 1922 LY · 1929 YA 1946 QD · 1966 BD A906 VB · A923 YA | |
| main-belt · (outer) [3] | |
| Orbital characteristics [1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 109.41 yr (39963 days) |
| Aphelion | 3.9467 AU (590.42 Gm) |
| Perihelion | 2.4490 AU (366.37 Gm) |
| 3.1979 AU (478.40 Gm) | |
| Eccentricity | 0.23418 |
| 5.72 yr (2088.8 d) | |
| 84.794° | |
| 0° 10m 20.46s / day | |
| Inclination | 21.645° |
| 216.64° | |
| 132.96° | |
| Earth MOID | 1.49407 AU (223.510 Gm) |
| Jupiter MOID | 1.76555 AU (264.123 Gm) |
| TJupiter | 3.044 |
| Physical characteristics | |
| Dimensions | 78.73±2.3 km (IRAS:17)[4] 82.28±2.71 km[5] 92.10±0.76 km[6] |
| 39.365±1.15 km | |
| 10.099±0.004 h[7] 10.100±0.003 h[8] 9.5 h[9] 10.098±0.001 h[10] 10.099 h (0.4208 d)[1] | |
| 0.0365±0.002 (IRAS:17)[1][4] 0.035±0.002[5] 0.027±0.004[6] | |
| B–V = 0.677 U–B = 0.252 Tholen = PF[1] P [3] | |
| 9.73[1] | |
978 Aidamina, provisional designation 1922 LY, is a large, rare-type asteroid from the outer region of the asteroid belt, about 80 kilometers in diameter. It was discovered by Soviet–Russian astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula, on 18 May 1922.[11] Twelve nights later, the body was independently discovered by astronomer Max Wolf at Heidelberg, southern Germany.[2]
The asteroid is the only body classified as a PF-type asteroid in the Tholen taxonomy,[12] a subtype of the dark and reddish P-type asteroids, of which only a few dozens bodies are currently known.[13] It orbits the Sun at a distance of 2.4–3.9 AU once every 5 years and 9 months (2,090 days). Its orbit is tilted by 22 degrees to the plane of the ecliptic and shows an eccentricity of 0.23.
According to the surveys carried out by the Infrared Astronomical Satellite, IRAS, the Japanese Akari satellite, and the U.S. Wide-field Infrared Survey Explorer with its NEOWISE mission, the body has a very low albedo between 0.027 and 0.037.[4][5][6] Several photometric light-curve analysis rendered a concurring, well-defined rotation period of 10.1 hours,[7][8][10] while another observation resulted in an alternative period of 9.5 hours.[9]
The minor planet was named after a friend of the discoverer's family, Aida Minaevna.[2]
References
- ^ a b c d e f "JPL Small-Body Database Browser: 978 Aidamina (1922 LY)" (2015-11-17 last obs.). Jet Propulsion Laboratory. Retrieved 2 May 2016.
- ^ a b c Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (978) Aidamina. Springer Berlin Heidelberg. p. 85. ISBN 978-3-540-29925-7. Retrieved January 2016.
{{cite book}}: Check date values in:|accessdate=(help) - ^ a b "LCDB Data for (978) Aidamina". Asteroid Lightcurve Database (LCDB). Retrieved January 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. Bibcode:2004PDSS...12.....T. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b c 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". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b c 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. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Lecrone, Crystal; Duncan, Allison; Kirkpatrick, Elaine (December 2004). "Lightcurves and periods for asteroids 105 Artemis, 978 Aidamina, and 1103 Sequoia". The Minor Planet Bulletin. 31 (4): 77–78. Bibcode:2004MPBu...31...77L. ISSN 1052-8091. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (978) Aidamina". Geneva Observatory. Retrieved January 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b Clark, Maurice (September 2006). "Lightcurve results for 383 Janina, 899 Jokaste, 1825 Klare, 2525 O'Steen 5064 Tanchozuru, and (17939) 1999 HH8". The Minor Planet Bulletin. 33 (3): 53–56. Bibcode:2006MPBu...33...53C. ISSN 1052-8091. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Pilcher, Frederick; Ferrero, Andrea (January 2015). "Rotation Period Determination for 978 Aidamina". The Minor Planet Bulletin. 42 (1): 28. Bibcode:2015MPBu...42...28P. ISSN 1052-8091. Retrieved January 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ "978 Aidamina (1922 LY)". Minor Planet Center. Retrieved January 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ "JPL Small-Body Database Search Engine: spec. type = PF (Tholen)". JPL Solar System Dynamics. Retrieved January 2016.
{{cite web}}: Check date values in:|accessdate=(help); Missing pipe in:|title=(help) - ^ "JPL Small-Body Database Search Engine: spec. type = P (Tholen)". JPL Solar System Dynamics. Retrieved January 2016.
{{cite web}}: Check date values in:|accessdate=(help); Missing pipe in:|title=(help)
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
- 978 Aidamina at the JPL Small-Body Database
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