Discovery[1] | |
---|---|
Discovered by | J. Alu |
Discovery site | Palomar Obs. |
Discovery date | 12 March 1988 |
Designations | |
(6037) 1988 EG | |
1988 EG | |
Apollo · NEO · PHA[2] | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 28.24 yr (10,315 days) |
Aphelion | 1.9064 AU |
Perihelion | 0.6359 AU |
1.2711 AU | |
Eccentricity | 0.4997 |
1.43 yr (523 days) | |
261.93° | |
0° 41m 15.72s / day | |
Inclination | 3.4998° |
182.48° | |
242.07° | |
Earth MOID | 0.0243 AU · 9.5 LD |
Physical characteristics | |
0.399±0.027 km[3] 0.54 km (derived)[4] | |
2.760±0.002 h[a] | |
0.20 (assumed)[4] 0.37±0.05[3] | |
S[4] | |
18.7[1][4] · 19.18±0.20[5] | |
(6037) 1988 EG (provisional designation 1988 EG) is an eccentric, stony asteroid, classified as near-Earth object and potentially hazardous asteroid. It belongs to the group of Apollo asteroids and measures approximately half a kilometer in diameter. It was discovered by American astronomer Jeff T. Alu at the U.S. Palomar Observatory, California, on 12 March 1988.[2]
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