Discovery [1] | |
---|---|
Discovered by | J. H. Metcalf |
Discovery site | Winchester Obs. |
Discovery date | 23 September 1913 |
Designations | |
(767) Bondia | |
Named after | William Cranch Bond (1789–1859) George Phillips Bond (1825–1865) (American astronomers)[2] |
A913 SD · 1929 OA 1933 FO1 · 1938 DQ2 1957 UR · 1958 XA1 1959 AD · A902 SA 1913 SX | |
main-belt [1][3] · (outer) Themis [4][5][6] | |
Orbital characteristics [3] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 0 | |
Observation arc | 117.59 yr (42,949 d) |
Aphelion | 3.6909 AU |
Perihelion | 2.5531 AU |
3.1220 AU | |
Eccentricity | 0.1822 |
5.52 yr (2,015 d) | |
137.11° | |
0° 10m 43.32s / day | |
Inclination | 2.4118° |
79.324° | |
269.09° | |
Physical characteristics | |
8.3402±0.0007 h[10] | |
SMASS = B [3][11] | |
767 Bondia (prov. designation: A913 SD or 1913 SX) is a Themis asteroid from the outer regions of the asteroid belt, approximately 43 kilometers (27 miles) in diameter. It was discovered on 23 September 1913, by American astronomer Joel Hastings Metcalf at his observatory (799) in Winchester, Massachusetts.[1] The B-type asteroid has a rotation period of 8.3 hours. It was named after William Cranch Bond (1789–1859) and his son George Phillips Bond (1825–1865), both American astronomers and directors of the Harvard College Observatory in Cambridge, Massachusetts.[2]
MPC-object
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