374 Burgundia is a typical main belt asteroid that was discovered by Auguste Charlois on 18 September 1893 in Nice. It was named for the former French region of Burgundy. It is one of seven of Charlois's discoveries that was expressly named by the Astromomisches Rechen-Institut (Astronomical Calculation Institute).[4]
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 18 September 1893 |
Designations | |
(374) Burgundia | |
Pronunciation | /bɜːrˈɡʌndiə/[1] |
Named after | Burgundy |
1893 AK | |
Main belt | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 112.39 yr (41051 d) |
Aphelion | 3.00578 AU (449.658 Gm) |
Perihelion | 2.5566 AU (382.46 Gm) |
2.7812 AU (416.06 Gm) | |
Eccentricity | 0.080763 |
4.64 yr (1694.1 d) | |
295.379° | |
0° 12m 45s / day | |
Inclination | 8.9881° |
219.030° | |
25.153° | |
Physical characteristics | |
Dimensions | 44.67±1.3 km |
6.972 h (0.2905 d) | |
0.3014±0.018 | |
S | |
8.67,[2] 8.68[3] | |
Burgundia was long thought to be a member of the now defunct Ceres asteroid family, but it was found to be an unrelated interloper in that group based on its non-matching composition.[5]
References
edit- ^ "Burgundian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ a b Yeomans, Donald K., "374 Burgundia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016.
- ^ Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, vol. 34, pp. 113–119, Bibcode:2007MPBu...34..113W.
- ^ Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. ISBN 3-540-00238-3.
- ^ Cellino, A . et al. "Spectroscopic Properties of Asteroid Families", in Asteroids III, University of Arizona Press, pp. 633-643 (2002).
External links
edit- 374 Burgundia at AstDyS-2, Asteroids—Dynamic Site
- 374 Burgundia at the JPL Small-Body Database