374 Burgundia
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Discovery A | |
---|---|
Discoverer | Auguste Charlois |
Discovery date | September 18, 1893 |
Alternate designations B |
1893 AK |
Category | Main belt |
Orbital elements C | |
|
|
Eccentricity (e) | 0.079 |
Semi-major axis (a) | 415.966 Gm (2.781 AU) |
Perihelion (q) | 382.91 Gm (2.56 AU) |
Aphelion (Q) | 449.021 Gm (3.002 AU) |
Orbital period (P) | 1693.512 d (4.64 a) |
Mean orbital speed | 17.86 km/s |
Inclination (i) | 8.986° |
Longitude of the ascending node (Ω) |
219.238° |
Argument of perihelion (ω) |
27.587° |
Mean anomaly (M) | 119.563° |
Physical characteristics D | |
Dimensions | 45.0 km |
Mass | unknown |
Density | unknown |
Surface gravity | unknown |
Escape velocity | unknown |
Rotation period | unknown |
Spectral class | S |
Absolute magnitude | 8.67 |
Albedo (geometric) | unknown |
Mean surface temperature |
unknown |
374 Burgundia is a typical Main belt asteroid. It is classified as an S-type asteroid.
It was discovered by Auguste Charlois on September 18, 1893 in Nice.
Burgundia was long thought to be a member of the now defunct Ceres asteroid family, but was found to be an unrelated interloper on the basis of its non-matching composition (A Cellino et al "Spectroscopic Properties of Asteroid Families", in Asteroids III, University of Arizona Press p. 633-643 (2002) ).
Minor planets | ||
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Previous minor planet | 374 Burgundia | Next minor planet |
List of asteroids |
Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Comets · Trans-Neptunians (Kuiper belt • Scattered disc • Oort cloud)
For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons and the Solar System.
For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names.