Astronomy:81 Terpsichore
Orbital diagram | |
Discovery | |
---|---|
Discovered by | Ernst Wilhelm Tempel |
Discovery date | September 30, 1864 |
Designations | |
(81) Terpsichore | |
Pronunciation | /tɜːrpˈsɪxərɛ/[1] |
Named after | Terpsichore |
Minor planet category | Main belt |
Adjectives | Terpsichorean /tɜːrpsɪxəˈriːən/[1] |
Orbital characteristics | |
Epoch December 31, 2006 (JD 2454100.5) | |
|{{{apsis}}}|helion}} | 516.955 Gm (3.456 AU) |
|{{{apsis}}}|helion}} | 337.132 Gm (2.254 AU) |
427.044 Gm (2.855 AU) | |
Eccentricity | 0.211 |
Orbital period | 1761.647 d (4.82 a) |
Average Orbital speed | 17.43 km/s |
Mean anomaly | 149.581° |
Inclination | 7.809° |
Longitude of ascending node | 1.497° |
50.234° | |
Physical characteristics | |
Dimensions | 121.77 ± 2.34 km[2] |
Mass | (6.19 ± 5.31) × 1018 kg[2] |
Mean density | 6.54 ± 5.62 g/cm3[2] |
Rotation period | 10.943 hr |
Geometric albedo | 0.051 [3] |
C | |
Absolute magnitude (H) | 8.48 |
Terpsichore (minor planet designation: 81 Terpsichore) is a large and very dark main-belt asteroid. It has most probably a very primitive carbonaceous composition. It was found by the prolific comet discoverer Ernst Tempel on September 30, 1864.[4] It is named after Terpsichore, the Muse of dance in Greek mythology.
Photometric observations of the minor planet in 2011 gave a rotation period of 10.945±0.001 h with an amplitude of 0.09±0.01 in magnitude. This result is consistent with previous determinations.[5] Two stellar occultation events involving this asteroid were observed from multiple sites in 2009. The resulting chords matched a smooth elliptical cross-section with dimensions of 134.0±4.0 km × 108.9±0.7 km.[6]
In popular culture
A space station orbiting 81 Terpsichore is the main setting in the science fiction story The Dark Colony (Asteroid Police Book 1) by Richard Penn.
References
- ↑ 1.0 1.1 Terpsichore (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Terpsichore (Subscription or UK public library membership required.)
- ↑ 2.0 2.1 2.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode: 2012P&SS...73...98C. See Table 1.
- ↑ Asteroid Data Sets
- ↑ Tempel, M. (November 1864), "Minor Planet 81 Terpsichore discovered", Monthly Notices of the Royal Astronomical Society 25: 31, Bibcode: 1864MNRAS..25...31T.
- ↑ 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.
- ↑ Timerson, Brad; Durech, J.; Pilcher, F. et al. (October 2010), "Occultations by 81 Terpsichore and 694 Ekard in 2009 at Different Rotational Phase Angles", The Minor Planet Bulletin 37 (4): 140−142, Bibcode: 2010MPBu...37..140T.
External links
- 81 Terpsichore at AstDyS-2, Asteroids—Dynamic Site
- 81 Terpsichore at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/81 Terpsichore.
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