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1995 UB Asteroid

1995 UB 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. A close approach will occur on 1995 Oct 17 when it will get to within 0.005 A.U. Its orbit takes 1.66 years to travel round the Sun.

The absolute magnitude of the object is 27.3 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 Semi-Major Axis of the orbit is 1.4, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1995 UB orbits in relation to the orbital plane is 9 degrees. The orbital eccentricity is 0.413, it is the degree at which 1995 UB orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1995 UB Facts


TypeAsteroid
Asteroid TypeApollo
Date of Closest Approach1995 Oct 17
Distance on Closest Approach0.005 A.U.
Orbital Period1.66
Absolute Magnitude27.3
Semi-Major Axis1.4
Orbital Inclination9
Orbital Eccentricity0.413
Sourcehttps://minorplanetcenter.net/


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