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(10751) 1989 UV1 Asteroid

1989 UV1 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 13.6 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 19.57279 degrees. The Argument of Perihelion is 320.2614. 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 159.84168, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 3.0966022, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1989 UV1 orbits in relation to the orbital plane is 0.73426 degrees. The orbital eccentricity is 0.2327600, it is the degree at which 1989 UV1 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1989 UV1 Facts


TypeAsteroid
Absolute Magnitude13.6
Longitude Of Ascending Node 19.57279
Argument of Perihelion320.2614
Mean Anomoly159.84168
Semi-Major Axis 3.0966022
Orbital Inclination (degrees)0.73426
Orbital Eccentricity0.2327600
Source(s)https://minorplanetcenter.net/


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