Universe GuideSearchTwitterComments

(7185) 1991 VN1 Asteroid

1991 VN1 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 13.7 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 115.09844 degrees. The Argument of Perihelion is 137.986. 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 300.70376, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 2.1951409, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1991 VN1 orbits in relation to the orbital plane is 5.70746 degrees. The orbital eccentricity is 0.0964789, it is the degree at which 1991 VN1 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1991 VN1 Facts


TypeAsteroid
Absolute Magnitude13.7
Longitude Of Ascending Node115.09844
Argument of Perihelion137.986
Mean Anomoly300.70376
Semi-Major Axis 2.1951409
Orbital Inclination5.70746
Orbital Eccentricity0.0964789
Sourcehttps://minorplanetcenter.net/


Comments and Questions

There's no register feature and no need to give an email address if you don't need to. All messages will be reviewed before being displayed. Comments may be merged or altered slightly such as if an email address is given in the main body of the comment.

   
x
This website is using cookies. More info. That's Fine