1252 Celestia

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°
 13m 22.08s / day
Inclination 33.838°
140.92°
63.622°
Physical characteristics
Dimensions 17.4 km
19.037±0.304[5]
10.636 h (0.4432 d)
0.215±0.022[5]
0.2573±0.053
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. 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.
    2. 1 2 "Discovery Circumstances: Numbered Minor Planets (1)-(5000)". Minor Planet Center. Retrieved 22 August 2016.
    3. 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.
    4. "Small Bodies Data Ferret". Nesvorny HCM Asteroid Families V3.0. Retrieved 4 September 2017.
    5. 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.
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