161 Athor
.png) A three-dimensional model of 161 Athor based on its light curve. | |
| Discovery[1] | |
|---|---|
| Discovered by | James Craig Watson |
| Discovery site | Detroit Observatory |
| Discovery date | 19 April 1876 |
| Designations | |
| (161) Athor | |
| Pronunciation | /ˈæθər/,[2] /ˈɑːθər/[3] |
Named after | Hathor |
| Main belt[4] | |
| Orbital characteristics[4][5] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 116.50 yr (42551 d) |
| Aphelion | 2.70593 AU (404.801 Gm) |
| Perihelion | 2.05285 AU (307.102 Gm) |
| 2.37939 AU (355.952 Gm) | |
| Eccentricity | 0.137237 |
| 3.67 yr (1340.6 d) | |
| 348.807° | |
| 0° 16m 6.737s / day | |
| Inclination | 9.05986° |
| 18.6090° | |
| 295.007° | |
| Physical characteristics | |
| Dimensions | 44.19±3.3 km[4] Mean diameter[6] 47.0±0.2 km circular fit[7] |
| 7.280 h (0.3033 d)[4] 7.281 ± 0.001 hours[8] 7.288 ± 0.007 hours[9] | |
| 0.1980±0.033[4][6] | |
| M[10] | |
| 9.15[4][11] | |
161 Athor is an M-type Main belt asteroid that was discovered by James Craig Watson on April 19, 1876, at the Detroit Observatory[1] and named after Hathor, an Egyptian fertility goddess. An occultation by Athor was observed, on October 15, 2002, resulting in an estimated diameter of 47.0 kilometres (29.2 mi).[7]
Photometric observations of the minor planet in 2010 gave a rotation period of 7.2798±0.0001 h with an amplitude of 0.19±0.02 in magnitude. This result is consistent with previous determinations.[12] The spectra is similar to that of carbonaceous chondrites, with characteristics of ferric oxides and little or no hydrated minerals.[13]
References
- ^ a b "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". IAU: Minor Planet Center. Archived from the original on 2 February 2009. Retrieved 20 December 2008.
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ "Hathor, Athor". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ a b c d e f "161 Athor". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
- ^ "(161) Athor". AstDyS. Italy: University of Pisa. Retrieved 20 December 2008.
- ^ a b Tedesco; et al. (2004). "Supplemental IRAS Minor Planet Survey (SIMPS)". IRAS-A-FPA-3-RDR-IMPS-V6.0. Planetary Data System. Archived from the original on August 17, 2009. Retrieved December 27, 2008.
- ^ a b Dunham & Herald (2008). "Asteroid Occultations". EAR-A-3-RDR-OCCULTATIONS-V6.0. Planetary Data System. Retrieved 27 December 2008.
- ^ Pilcher & Higgins (2008). "Period Determination for 161 Athor". The Minor Planet Bulletin. 35 (4): 147. Bibcode:2008MPBu...35..147P.
- ^ Debehogne & Zappala (1980). "Photoelectric lightcurves of the asteroids 139 Juewa and 161 Athor, obtained with the 50 CM photometric telescope at ESO, La Silla". Astronomy and Astrophysics Supplement Series. 42: 85–89. Bibcode:1980A&AS...42...85D.
- ^ Neese (2005). "Asteroid Taxonomy". EAR-A-5-DDR-TAXONOMY-V5.0. Planetary Data System. Archived from the original on August 5, 2009. Retrieved December 27, 2008.
- ^ Tholen (2007). "Asteroid Absolute Magnitudes". EAR-A-5-DDR-ASTERMAG-V11.0. Planetary Data System. Archived from the original on August 16, 2009. Retrieved December 27, 2008.
- ^ Pilcher, Frederick (July 2011), "Rotation Period Determinations for 28 Bellona, 81 Terpsichore, 126 Velleda 150 Nuwa, 161 Athor, 419 Aurelia, and 632 Pyrrha", The Minor Planet Bulletin, 38 (3): 156−158, Bibcode:2011MPBu...38..156P.
- ^ Busarev, V. V.; Taran, M. N. (November 2002), "On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids", Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed. Barbara Warmbein. ESA SP-500., Noordwijk, Netherlands: ESA Publications Division, pp. 933−936, Bibcode:2002ESASP.500..933B, ISBN 92-9092-810-7.
External links
- 161 Athor at AstDyS-2, Asteroids—Dynamic Site
- 161 Athor at the JPL Small-Body Database
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