Universe GuideSearchTwitterComments

(11397) 1998 XX93 Asteroid

1998 XX93 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 10.2 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 261.21315 degrees. The Argument of Perihelion is 151.5011. 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 299.72658, is the angular distance of the planet from the perihelion or aphelion. Ref:Dictionary.The Semi-Major Axis of the orbit is 5.2503220, which is the furthest point from the centre to the edge of an elliptical point.

The orbital inclination, the angle at which 1998 XX93 orbits in relation to the orbital plane is 20.99479 degrees. The orbital eccentricity is 0.0611824, it is the degree at which 1998 XX93 orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.

1998 XX93 Facts


TypeAsteroid
Asteroid TypeJupiter Trojan
Absolute Magnitude10.2
Longitude Of Ascending Node261.21315
Argument of Perihelion151.5011
Mean Anomoly299.72658
Semi-Major Axis 5.2503220
Orbital Inclination20.99479
Orbital Eccentricity0.0611824
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