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(4424) Arkhipova Asteroid

Arkhipova 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 11.7 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 138.38620 degrees. The Argument of Perihelion is 15.86076. 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 143.39131, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.7571315, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which Arkhipova orbits in relation to the orbital plane is 14.72229 degrees. The orbital eccentricity is 0.0786759, it is the degree at which Arkhipova orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

Arkhipova Facts


TypeAsteroid
Absolute Magnitude11.7
Longitude Of Ascending Node138.38620
Argument of Perihelion15.86076
Mean Anomoly143.39131
Semi-Major Axis 2.7571315
Orbital Inclination (degrees)14.72229
Orbital Eccentricity0.0786759
Source(s)https://minorplanetcenter.net/


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