Discovery | |
---|---|
Discovered by | R. H. McNaught |
Discovery site | Siding Spring Obs. |
Discovery date | 18 February 1991 |
Designations | |
(5335) Damocles | |
Pronunciation | /ˈdæməkliːz/[1] |
Named after | Damocles (Greek mythology)[2] |
1991 DA | |
distant [3] centaur [4] · damocloid [5] | |
Adjectives | Damoclean (/dæməˈkliːən/)[6] |
Symbol | (astrological) |
Orbital characteristics [4] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 4 | |
Observation arc | 1.51 yr (551 days) |
Aphelion | 22.078 AU |
Perihelion | 1.5741 AU |
11.826 AU | |
Eccentricity | 0.8669 |
40.67 Jyr (14,854 days) | |
236.35° | |
0° 1m 27.12s / day | |
Inclination | 61.875° |
314.14° | |
191.26° | |
Mars MOID | 0.05787 AU[3] |
TJupiter | 1.149 |
Physical characteristics | |
Dimensions | ~ 10 km[7] |
26.56[8] | |
13.3[4][8] | |
(5335) Damocles /ˈdæməkliːz/, provisional designation 1991 DA, is a centaur and the namesake of the damocloids, a group of minor planets which may be inactive nuclei of the Halley-type and long-period comets. It was discovered on 18 February 1991, by Australian astronomer Robert McNaught at Siding Spring Observatory in Australia. It is named after Damocles, a figure of Greek mythology.[2]
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