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(12122) 1999 NV55 Asteroid

1999 NV55 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 12.6 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 245.06639 degrees. The Argument of Perihelion is 308.6855. 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 61.66588, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.9939582, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1999 NV55 orbits in relation to the orbital plane is 11.23612 degrees. The orbital eccentricity is 0.0249245, it is the degree at which 1999 NV55 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1999 NV55 Facts


TypeAsteroid
Absolute Magnitude12.6
Longitude Of Ascending Node245.06639
Argument of Perihelion308.6855
Mean Anomoly 61.66588
Semi-Major Axis 2.9939582
Orbital Inclination11.23612
Orbital Eccentricity0.0249245
Sourcehttps://minorplanetcenter.net/


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