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Home > 117 Lomia


117 Lomia
Orbital characteristics 1
Orbit type Main belt
Semimajor axis 2.990 AU
Perihelion distance 2.905 AU
Aphelion distance 3.074 AU
Orbital period 5.17 years
Inclination 14.93°
Eccentricity 0.028
Physical characteristics 1
Diameter 148.7 km
Rotation period 9.127 hours
Spectral class CC-type asteroids are carbonaceous asteroids. They form 75% of known asteroids, and are extremely dark ( albedo 0. 03), similar to carbonaceous chondrite meteorites (types CI and CM). They dominate the outer belt beyond 2. These asteroids have approximatel
Abs. magnitudeIn astronomy, absolute magnitude is the apparent magnitude, m an object would have if it were at a standardized distance away. It allows the overall brightnesses of objects to be compared without regards to distance. Absolute Magnitude for stars M In stel 7.95
AlbedoNote: This article discusses the physical or planetological property of albedo. For other usage, see Albedo (disambiguation). The albedo is a measure of reflectivity of a surface or body. It is the ratio of electromagnetic radiation reflected to the amoun 4 0.053
History 2
Discoverer A. Borrelly, 1871Events January January 18 The member-states of the North German Confederation unite into a single nation-state known as the German Empire. The King of Prussia is declared the first German Emperor as Wilhelm I of Germany. January 28 France surrenders to en


117 Lomia is a rather large Main belt asteroidAn asteroid is a small, solid object in our Solar System, orbiting the Sun. An asteroid is an example of a minor planet (or planetoid , which are much smaller than planets. The asteroids are believed to be remnants of the protoplanetary disc which were no. It has a very dark surface and primitive carbonaceous composition.

It was discovered by A. Borrelly on September 12, 1871.

Occultations by Lomia have so far been observed twice, in 2000 and 2003.

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Main Belt asteroids

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