Discovery [1] | |
---|---|
Discovered by | W. Liller |
Discovery site | Cerro Tololo |
Discovery date | 8 April 1978 |
Designations | |
(2449) Kenos | |
Named after | Kenos (Selknam mythology)[2] |
1978 GC | |
Mars-crosser [1] · Hungaria [3] · binary | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 38.93 yr (14,220 days) |
Aphelion | 2.2303 AU |
Perihelion | 1.5872 AU |
1.9088 AU | |
Eccentricity | 0.1685 |
2.64 yr (963 days) | |
258.57° | |
0° 22m 25.32s / day | |
Inclination | 24.986° |
179.86° | |
102.25° | |
Physical characteristics | |
Dimensions | 2.95 km (calculated)[4] |
3.846±0.001 h[5] 3.8481±0.0003 h[6] 3.8492±0.0008 h[7] 4.188±0.007 h[8] | |
0.4 (assumed)[4] | |
Tholen = E [1] · CX [9] · E [4] B–V = 0.684[1] U–B = 0.356[1] | |
14.07±0.09[8] · 14.26[1][4] · 14.46±0.48[9] | |
2449 Kenos, provisional designation 1978 GC, is a bright Hungaria asteroid and medium-sized Mars-crosser from the inner regions of the asteroid belt, approximately 3 kilometers in diameter. It was discovered by American astronomer William Liller at Cerro Tololo Inter-American Observatory in Chile, on 8 April 1978, and named after Kenos from Selknam mythology.[2][3] A minor-planet moon was discovered around the asteroid on 27 February 2015.[10]
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