Discovery [1] | |
---|---|
Discovered by | E. F. Helin M. Barucci |
Discovery site | CERGA Obs. |
Discovery date | 15 August 1985 |
Designations | |
(3752) Camillo | |
Pronunciation | /kəˈmɪloʊ/ |
Named after | Camillo (son of King Turno and son of discoverer)[2] |
1985 PA | |
NEO · Apollo [1][3] | |
Orbital characteristics [3] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 42.26 yr (15,436 d) |
Aphelion | 1.8400 AU |
Perihelion | 0.9871 AU |
1.4135 AU | |
Eccentricity | 0.3017 |
1.68 yr (614 d) | |
41.249° | |
0° 35m 11.4s / day | |
Inclination | 55.555° |
147.98° | |
312.22° | |
Earth MOID | 0.0780 AU (30.3871 LD) |
Physical characteristics | |
2.3 km (approx.)[4] 2.306±0.088 km[5][6] 2.328 km[7] 2.33 km (taken)[8] | |
37.846 h[9] 37.881±0.005 h[10] | |
0.210±0.036[5][6] 0.22[4] 0.2234[7] | |
S (assumed)[8] | |
15.3[3] · 15.41[8][9] · 15.41±0.13[7] · 15.5[5] | |
3752 Camillo is an inclined contact-binary asteroid, classified as near-Earth object of the Apollo group, approximately 2.3 kilometers (1.4 miles) in diameter. It was discovered on 15 August 1985, by astronomers Eleanor Helin and Maria Barucci using a 0.9-metre (35 in) telescope at the CERGA Observatory in Caussols, France. Lightcurve studies by Petr Pravec in 1998 suggest that the assumed S-type asteroid has an elongated shape and a longer-than average rotation period of 38 hours.[1][4]
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