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(284) Amalia Asteroid

Amalia 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 10.05 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 233.71209 degrees. The Argument of Perihelion is 58.06379. 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 272.14680, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.3582353, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which Amalia orbits in relation to the orbital plane is 8.05758 degrees. The orbital eccentricity is 0.2221126, it is the degree at which Amalia orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

Amalia Facts


TypeAsteroid
Absolute Magnitude10.05
Longitude Of Ascending Node233.71209
Argument of Perihelion58.06379
Mean Anomoly272.14680
Semi-Major Axis 2.3582353
Orbital Inclination8.05758
Orbital Eccentricity0.2221126
Sourcehttps://minorplanetcenter.net/


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