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(418) Alemannia Asteroid

Alemannia 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 9.77 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 248.82796 degrees. The Argument of Perihelion is 126.5228. 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 108.88811, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.5924927, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which Alemannia orbits in relation to the orbital plane is 6.81837 degrees. The orbital eccentricity is 0.1196748, it is the degree at which Alemannia orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

Alemannia Facts


TypeAsteroid
Absolute Magnitude9.77
Longitude Of Ascending Node248.82796
Argument of Perihelion126.5228
Mean Anomoly108.88811
Semi-Major Axis 2.5924927
Orbital Inclination (degrees)6.81837
Orbital Eccentricity0.1196748
Source(s)https://minorplanetcenter.net/


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