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(5487) 1991 UM4 Asteroid

1991 UM4 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 13.9 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 355.84595 degrees. The Argument of Perihelion is 241.7255. 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 272.71706, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.4117254, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1991 UM4 orbits in relation to the orbital plane is 2.30676 degrees. The orbital eccentricity is 0.1609211, it is the degree at which 1991 UM4 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1991 UM4 Facts

Absolute Magnitude13.9
Longitude Of Ascending Node355.84595
Argument of Perihelion241.7255
Mean Anomoly272.71706
Semi-Major Axis 2.4117254
Orbital Inclination (degrees)2.30676
Orbital Eccentricity0.1609211

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