1252 Celestia
Discovery [1] | |
---|---|
Discovered by | F. L. Whipple |
Discovery site |
Oak Ridge Obs. [2] (Harvard) |
Discovery date | 19 February 1933 |
Designations | |
MPC designation | (1252) Celestia |
Named after |
Celestia Whipple (mother of the discoverer)[3] |
1933 DG · 1934 PA1 | |
main-belt · (middle) Pallas [4] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 84.09 yr (30,714 days) |
Aphelion | 3.2552 AU |
Perihelion | 2.1346 AU |
2.6949 AU | |
Eccentricity | 0.2079 |
4.42 yr (1,616 days) | |
3.3646° | |
0° 13m 22.08s / day | |
Inclination | 33.838° |
140.92° | |
63.622° | |
Physical characteristics | |
Dimensions |
17.4 km ±0.304 19.037[5] |
10.636 h (0.4432 d) | |
±0.022 0.215[5] ±0.053 0.2573 | |
S (Tholen)[1] S (SMASS)[1] B–V = 0.890[1] U–B = 0.425[1] | |
10.89[1] | |
|
1252 Celestia, provisional designation 1933 DG, is a stony Palladian asteroid from the central region of the asteroid belt, discovered on 19 February 1933, by American astronomer Fred Whipple at Oak Ridge Observatory[2] operated by the Harvard-Smithsonian Center for Astrophysics at Massachusetts, United States. The S-type asteroid measures about 17 kilometers in diameter, rotates once every 10.6 hours and is heavily tilted towards the ecliptic by almost 34 degrees.[1]
This minor planet was named after the mother of the discoverer, Celestia MacFarland Whipple.[3]
References
- 1 2 3 4 5 6 7 8 "JPL Small-Body Database Browser: 1252 Celestia (1933 DG)" (2017-04-30 last obs.). Jet Propulsion Laboratory. Retrieved 15 June 2017.
- 1 2 "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". Minor Planet Center. Retrieved 22 August 2016.
- 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1252) Celestia. Springer Berlin Heidelberg. p. 104. ISBN 978-3-540-29925-7. Retrieved 22 August 2016.
- ↑ "Small Bodies Data Ferret". Nesvorny HCM Asteroid Families V3.0. Retrieved 4 September 2017.
- 1 2 Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. Retrieved 15 June 2017.
External links
- Dictionary of Minor Planet Names, Google books
- 1252 Celestia at the JPL Small-Body Database
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