Discovery

Bergelmir was discovered on Dec. 12, 2004, one of 12 Saturnian moons found that day by Scott S. Sheppard, David C. Jewitt, and Jan T. Kleyna, using wide-field camera on the Subaru 8.3-m reflector telescope on Mauna Kea, Hawaii. Brian Marsden computed the orbital elements.

Overview

Bergelmir has a mean radius of 1.9 miles (3 km), assuming an albedo (a measure of how reflective the surface is) of 0.04. It orbits Saturn at an inclination of about 159 degrees and an eccentricity of about 0.1. At a mean distance of 12 million miles (19.3 million km) from Saturn, the moon takes about 1,006 Earth days to complete one orbit.

Bergelmir is a member of the Norse group of moons. These "irregular" moons have retrograde orbits around Saturn—traveling around in the opposite direction from the planet's rotation. Bergelmir and the other Norse moons also have eccentric orbits, meaning they are more elongated than circular.

Like Saturn's other irregular moons, Bergelmir is thought to be an object that was captured by Saturn's gravity, rather than having accreted from the dusty disk that surrounded the newly formed planet as the regular moons are thought to have done.

How Bergelmir Got its Name

Originally called S/2004 S15, Bergelmir was named for the frost giant who, with his wife, escaped drowning in the flood of Ymir's blood that ensued when Ymir was slain by Odin and his brothers in the Norse tale of creation.​

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