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(4490) Bambery Asteroid

Bambery 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 13.2 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 134.80455 degrees. The Argument of Perihelion is 267.9722. 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 79.33607, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 1.9309024, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which Bambery orbits in relation to the orbital plane is 26.11784 degrees. The orbital eccentricity is 0.0924336, it is the degree at which Bambery orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

Bambery Facts


TypeAsteroid
Asteroid TypeHungaria
Absolute Magnitude13.2
Longitude Of Ascending Node134.80455
Argument of Perihelion267.9722
Mean Anomoly 79.33607
Semi-Major Axis 1.9309024
Orbital Inclination (degrees)26.11784
Orbital Eccentricity0.0924336
Source(s)https://minorplanetcenter.net/


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