Bamberga Comparison Table

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Bamberga comparison table

Subject has absolute magnitude has mean opposition magnitude has meteorite class is a kind of is an instance of has radiu has inclination has semi-major axi has albedo has definition has rotation period 8^{h< sup>} has asteroid number has eccentricity

asteroid celestial body Also called planetoids or minor planets, the asteroids are tiny planets most of which orbit the Sun between Mars and Jupiter. The largest - and the first discovered - is Ceres, with a diameter of 1,003 km. It is estimated that there may altogether be no fewer than 40000. A few have very elliptical orbits and cross the orbits of several other (major) planets. One or two even have their own satellites (moons).

Bamberga +8.14 +11.41 carbonaceous chondrite asteroid larger than Pallas i = 11°.2 a = 2.80 AU, < 0.05 Asteroid with the darkest known surfaces in the solar system, the only minor planet known to have such a low albedo. -has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press 324 e = 0.36,

Subject	has absolute magnitude	has mean opposition magnitude	has meteorite class	is a kind of	is an instance of	has radiu	has inclination	has semi-major axi	has albedo	has definition	has rotation period 8^{h< sup>}	has asteroid number	has eccentricity
asteroid				celestial body						Also called planetoids or minor planets, the asteroids are tiny planets most of which orbit the Sun between Mars and Jupiter. The largest - and the first discovered - is Ceres, with a diameter of 1,003 km. It is estimated that there may altogether be no fewer than 40000. A few have very elliptical orbits and cross the orbits of several other (major) planets. One or two even have their own satellites (moons).
Bamberga	+8.14	+11.41	carbonaceous chondrite		asteroid	larger than Pallas	i = 11°.2	a = 2.80 AU,	< 0.05	Asteroid with the darkest known surfaces in the solar system, the only minor planet known to have such a low albedo.	-has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press	324	e = 0.36,

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