584 Semiramis
A three-dimensional model of 584 Semiramis based on its light curve. | |
Discovery | |
---|---|
Discovered by | A. Kopff |
Discovery site | Heidelberg |
Discovery date | 15 January 1906 |
Designations | |
1906 SY | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 110.26 yr (40272 d) |
Aphelion | 2.9282 AU (438.05 Gm) |
Perihelion | 1.8224 AU (272.63 Gm) |
2.3753 AU (355.34 Gm) | |
Eccentricity | 0.23276 |
3.66 yr (1337.1 d) | |
166.35° | |
0° 16m 9.228s / day | |
Inclination | 10.718° |
282.159° | |
85.121° | |
Earth MOID | 0.857216 AU (128.2377 Gm) |
Jupiter MOID | 2.65382 AU (397.006 Gm) |
Jupiter Tisserand parameter | 3.482 |
Physical characteristics | |
Mean radius |
±0.7 27.005km[1] 25.89 ± 1.075 km[2] |
Mass | (8.23 ± 5.77) × 1017 kg[2] |
5.068 h (0.2112 d) | |
±0.011 0.1987 | |
8.71 | |
|
584 Semiramis is a minor planet orbiting the Sun within the main asteroid belt. Photometric observations at the Mark Evans Observatory during 2014 gave a rotation period of 5.0689 ± 0.0001 hours. This value is in close agreement with previous studies.[3] The spectrum shows it to be a stony S(IV)-type asteroid.[4]
References
- 1 2 "584 Semiramis (1906 SY)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 7 May 2016.
- 1 2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ↑ Connour, Kyle; Wright, Tyler; French, Linda M. (April 2011), "Upon Further Review: VI. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory", The Minor Planet Bulletin, 42 (1): 4, Bibcode:2015MPBu...42....4C
- ↑ Sasaki, Takanori; et al. (November 2004), "Mature and Fresh Surfaces on the Newborn Asteroid Karin", The Astrophysical Journal, 615 (2): L161–L164, Bibcode:2004ApJ...615L.161S, doi:10.1086/426431
External links
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