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(10338) 1991 RB11 Asteroid

1991 RB11 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 158.13631 degrees. The Argument of Perihelion is 244.1619. 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 340.90712, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 3.1131572, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1991 RB11 orbits in relation to the orbital plane is 1.55046 degrees. The orbital eccentricity is 0.1543897, it is the degree at which 1991 RB11 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1991 RB11 Facts


TypeAsteroid
Absolute Magnitude13.2
Longitude Of Ascending Node158.13631
Argument of Perihelion244.1619
Mean Anomoly340.90712
Semi-Major Axis 3.1131572
Orbital Inclination1.55046
Orbital Eccentricity0.1543897
Sourcehttps://minorplanetcenter.net/


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