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(8905) Bankakuko Asteroid

Bankakuko 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 14.2 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 70.94147 degrees. The Argument of Perihelion is 279.6833. 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 245.70357, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.6074994, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which Bankakuko orbits in relation to the orbital plane is 5.69774 degrees. The orbital eccentricity is 0.2701190, it is the degree at which Bankakuko orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

Bankakuko Facts


TypeAsteroid
Absolute Magnitude14.2
Longitude Of Ascending Node 70.94147
Argument of Perihelion279.6833
Mean Anomoly245.70357
Semi-Major Axis 2.6074994
Orbital Inclination5.69774
Orbital Eccentricity0.2701190
Sourcehttps://minorplanetcenter.net/


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