Bergelmir is a Moon that orbits round Saturn rather than the Sun which our Earth orbits round. Its orbit circumference, the total distance it travels round its planetary parent is 120,893,879.74 km. The furthest it gets from its orbital parent (apoasis) is 22,078,537 km. Its density has been calculated at being 2.3 g/cm3. Its volume is 2.3 g/cm3. It was discovered on 12 December 2004 by Scott S. Sheppard, David C. Jewitt and Jan T. Kleyna.
The Semi-Major Axis of the orbit is 19,338,300 km, which is the furthest point from the centre to the edge of an elliptical point.
The equatorial circumference of Bergelmir is 18.8 km. The mean radius of Bergelmir is 3.0 (assuming an albedo of 0.04) km. The surface area of Bergelmir is 113.10 km2. The average orbit velocity, that is the speed at which it orbits is 5,008.3 km/h.
The orbital inclination, the angle at which Bergelmir orbits in relation to the orbital plane is 158.919 degrees. The orbital eccentricity is 0.1417, it is the degree at which Bergelmir orbits close to a circular (0) orbit as opposed to an elliptical (1) orbit.
|Orbital Circumference||120,893,879.74 km|
|Furthest from parent (Apoasis)||22,078,537 km|
|Date of Discovery||12 December 2004|
|Discoverer||Scott S. Sheppard, David C. Jewitt and Jan T. Kleyna|
|Semi-Major Axis||19,338,300 km|
|Equatorial Circumference||18.8 km|
|Mean Radius||3.0 (assuming an albedo of 0.04) km|
|Surface Area||113.10 km2|
|Average Orbit Velocity||5,008.3 km/h|