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Bergelmir (moon)

Moon of Saturn


Summary

Moon of Saturn

FieldValue
nameBergelmir
imageBergelmir.png
captionBergelmir imaged by the Cassini spacecraft in September 2014
discovery_ref
discovererS. Sheppard, D. Jewitt,
J. Kleyna, and B. Marsden
discoveredMay 4, 2005
mpc_nameSaturn XXXVIII
alt_namesS/2004 S 15
pronouncedor
adjectiveBergelmian
named_afterBergelmir
orbit_ref
semimajor
eccentricity0.142
period
inclination158.5°
satellite_ofSaturn
groupNorse group
physical_ref
mean_diameter
rotation
albedo0.06 (assumed)
spectral_typeB–R = 1.10 ± 0.15
magnitude24.2
abs_magnitude15.2

J. Kleyna, and B. Marsden

Bergelmir or Saturn XXXVIII (provisional designation S/2004 S 15) is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on May 4, 2005, from observations taken between December 12, 2004, and March 9, 2005.

Bergelmir is about 6 km in diameter, and orbits Saturn at an average distance of 19,338,000 km in 1006.659 days, at an inclination of 157° to the ecliptic (134° to Saturn's equator), in a retrograde direction and with an eccentricity of 0.152. Its rotation period is hours.

It was named in April 2007 after Bergelmir, a giant from Norse mythology and the grandson of Ymir, the primordial giant. Bergelmir and his wife alone among their kind were the only survivors of the enormous deluge of blood from Ymir's wounds when he was killed by Odin and his brothers at the dawn of time. Bergelmir then became the progenitor of a new race of giants.

Notes

References

References

  1. ...
  2. (2018). "Enceladus and the Icy Moons of Saturn". [[The University of Arizona Press]].
  3. Graykowski, Ariel. (2018-04-05). "Colors and Shapes of the Irregular Planetary Satellites". The Astronomical Journal.
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