![]() Orbits ofSerpe (blue), theinner planets andJupiter (outermost) | |
Discovery [1] | |
---|---|
Discovered by | H. Debehogne |
Discovery site | La Silla Obs. |
Discovery date | 4 May 1992 |
Designations | |
(9968) Serpe | |
Named after | Jean Serpe (Belgian physicist)[2] |
1992 JS2 · 1977 VT 1985 SC2 · 1988 KR1 | |
main-belt · (middle) | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 39.56 yr (14,451 days) |
Aphelion | 2.6974AU |
Perihelion | 2.4354 AU |
2.5664 AU | |
Eccentricity | 0.0510 |
4.11yr (1,502 days) | |
346.96° | |
0° 14m 22.92s / day | |
Inclination | 12.993° |
213.10° | |
78.256° | |
Physical characteristics | |
Dimensions | 12.355±0.453 km[3] |
0.088±0.011[3] | |
13.0[1] | |
9968 Serpe, provisional designation1992 JS2, is anasteroid from the middle regions of theasteroid belt, approximately 12 kilometers in diameter. This asteroid was discovered on 4 May 1992, by Belgian astronomerHenri Debehogne at ESO'sLa Silla Observatory in northern Chile. It was named after Belgian theoretical-physicistJean Serpe,[2] professor atUniversity of Liège and member of theRASAB.[2] The official naming citation was published by theMinor Planet Center on 17 May 2011 (M.P.C. 75102).[4]
Serpe orbits the Sun in themiddle main-belt at a distance of 2.4–2.7 AU once every 4 years and 1 month (1,502 days). Its orbit has aneccentricity of 0.05 and aninclination of 13° with respect to theecliptic.[1] In 1977, it was first observed as1977 VT atCerro El Roble Station in Argentina, extending the body'sobservation arc by 15 years prior to its official discovery at La Silla.[2]
According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures 12.355 kilometers in diameter and its surface has analbedo of 0.088.[3] As of 2017, no rotationallightcurve has been obtained ofSerpe. The body'srotation period and shape, as well as itsspectral type remain unknown.[1][5]