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(11200) 1999 CV121 Asteroid

1999 CV121 is an asteroid, a large rock that orbits the Sun mainly between the orbits of Mars and Jupiter. They tend to be an irregular shaped but Ceres asteroid is known to be spherical in shape but because it doesn't clear its path round the Sun, it is only a dwarf planet.

The absolute magnitude of the object is 12.2 which is the brightness of the object. A higher absolute magnitude means that the object is faint whereas a very low number means it is very bright.

The Longitude of Ascending Node of the object is 50.77739 degrees. The Argument of Perihelion is 215.661. It is the angle along the orbit of a planet or other Solar System object as measured from the ascending node (analogous to right ascension and longitude) Ref:Hawaii.

The mean anomoly is 47.03303, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.7366512, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1999 CV121 orbits in relation to the orbital plane is 18.8368 degrees. The orbital eccentricity is 0.2148925, it is the degree at which 1999 CV121 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1999 CV121 Facts


TypeAsteroid
Absolute Magnitude12.2
Longitude Of Ascending Node 50.77739
Argument of Perihelion215.661
Mean Anomoly 47.03303
Semi-Major Axis 2.7366512
Orbital Inclination18.8368
Orbital Eccentricity0.2148925
Sourcehttps://minorplanetcenter.net/


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