4055 Magellan
Discovery[1] | |
---|---|
Discovered by | E. Helin |
Discovery site | Palomar |
Discovery date | 24 February 1985 |
Designations | |
MPC designation | 1985 DO2 |
Named after | Ferdinand Magellan |
MPO 337285, 1988 OG | |
Orbital characteristics[2] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 11359 days (31.10 yr) |
Aphelion | 2.4145 AU (361.20 Gm) |
Perihelion | 1.2259 AU (183.39 Gm) |
1.8202 AU (272.30 Gm) | |
Eccentricity | 0.32652 |
2.46 yr (896.95 d) | |
63.101° | |
0° 24m 4.896s / day | |
Inclination | 23.258° |
164.850° | |
154.370° | |
Earth MOID | 0.23734 AU (35.506 Gm) |
Jupiter MOID | 2.99971 AU (448.750 Gm) |
Jupiter Tisserand parameter | 3.886 |
Physical characteristics | |
Dimensions | 3.038 km |
Mean radius | 1.245 km |
7.475 h (0.3115 d) | |
0.31 | |
V | |
14.7 | |
|
4055 Magellan (or 1985 DO2) is an Amor asteroid discovered on February 24, 1985, by E. Helin at Palomar. Based upon the spectrum, it is compositionally similar to 4 Vesta. It has a high albedo of 0.31.[3]
Photometric observations of this asteroid in 2010 show a rotation period of 7.488 ± 0.001 hours, with a brightness variation of 0.8 magnitude. The large variation suggests an elongated shape.[3]
See also
References
- ↑ "(4055) Magellan = 1985 DO2 = 1988 OG". Minor Planet Center. Retrieved 2015-06-04.
- ↑ "4055 Magellan (1985 DO2)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 14 April 2016.
- 1 2 Garcia, Karen; et al. (May 2011), "Rotationally Resolved Photometry of the V-type Near-Earth Asteroid 4055 Magellan (1985 DO2)", Bulletin of the American Astronomical Society 43, Bibcode:2011AAS...21822403G.
External links
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