Discovery [1] | |
---|---|
Discovered by | E. Bowell |
Discovery site | Anderson Mesa Stn. |
Discovery date | 18 December 1985 |
Designations | |
(4205) David Hughes | |
Named after | David Hughes [1] (British astronomer) |
1985 YP · 1986 AF 1986 CF | |
Mars-crosser [1][2][3] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 37.73 yr (13,780 d) |
Aphelion | 1.9843 AU |
Perihelion | 1.4686 AU |
1.7264 AU | |
Eccentricity | 0.1494 |
2.27 yr (829 d) | |
132.52° | |
0° 26m 4.2s / day | |
Inclination | 16.479° |
276.55° | |
109.98° | |
Earth MOID | 0.5525 AU (215 LD) |
Physical characteristics | |
3.92 km (calculated)[3] | |
24 h[4] | |
0.20 (assumed)[3] | |
SMASS = Xe [2][5] | |
14.4[2][3] | |
4205 David Hughes, provisional designation 1985 YP, is a Mars-crossing asteroid from inside the innermost regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 18 December 1985, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station near Flagstaff, Arizona.[1] The transitional X-type asteroid has a longer-than average rotation period of at least 24 hours.[3] It was named for British astronomer David Hughes.[1]
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