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110 Lydia
Orbital characteristics 1
Orbit type Main belt ( Lydia )
Semimajor axis 2.732 AU
Perihelion distance 2.514 AU
Aphelion distance 2.950 AU
Orbital period 4.52 years
Inclination 5.97°
Eccentricity 0.080
Physical characteristics 1
Diameter 86.1 km
Rotation period 10.927 hours
Spectral class MM-type asteroids are metallic asteroids; they are moderately bright ( albedo. 18) and made of nickel- iron, either pure or mixed with stone. They are thought to be samples of the metallic core of differentiated asteroids and originate in the inner portion
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 7.80
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 0.181
History 2
Discoverer A. Borrelly, 1870Events January 6 The inauguration of the Musikverein ( Vienna). January 10 John D. Rockefeller incorporates Standard Oil January 15 A political cartoon for the first time symbolizes the United States Democratic Party with a donkey ("A Live Jackass Kicking


110 Lydia is a quite 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 composed of fairly pure nickel- iron. Lydia asteroid family is named after it.

It was discovered by A. Borrelly on April 19, 1870. It was his second asteroid discovery.

Lydia occulted a dim star on September 18, 1999.


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Main Belt asteroids



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