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Fornjot (moon)

Moon of saturn


Summary

Moon of saturn

FieldValue
nameFornjot
imageFornjot-cassini.png
captionFornjot imaged by the Cassini spacecraft in March 2014
pronounced
named_afterFornjót
mpc_nameSaturn XLII
alt_namesS/2004 S 8
discoveredDecember 2004
discovererScott S. Sheppard
David C. Jewitt
Jan T. Kleyna
Brian G. Marsden
orbit_ref
semimajor
inclination170.4°
eccentricity0.206
period−1490.9 days
satellite_ofSaturn
groupNorse group
physical_ref
mean_diameter
rotation(6.9 or 9.5) ± 0.4? h
albedo0.06 (assumed)
spectral_typer – i = 0.20 ± 0.09
magnitude24.6
abs_magnitude14.9

David C. Jewitt Jan T. Kleyna Brian G. Marsden

Fornjot or Saturn XLII is the outermost named moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 4 May 2005 from observations taken between 12 December 2004, and 11 March 2005. It had the largest semi-major axis among all the known moons of Saturn until the recovery of Saturn LVIII in 2019.

It is about 6 kilometres in diameter, and it orbits Saturn at an average distance of 23,609 Mm in 1491 d at an inclination of 168° to the ecliptic (160° to Saturn's equator) in a retrograde direction and with an eccentricity of 0.186. It is ambiguous whether the rotation period is 6.9 or hours, but it is known to show very little variation in brightness and is probably very round in shape. It was also the faintest moon that was measured by Cassini–Huygens.{{cite conference

Fornjot was named after Fornjót, a giant in Norse mythology.

References

References

  1. [https://sites.google.com/carnegiescience.edu/sheppard/moons/saturnmoons S.S. Sheppard (2019), Moons of Saturn, ''Carnegie Science'', on line]
  2. (2022-05-17). "Colors of Irregular Satellites of Saturn with the Dark Energy Camera". The Astronomical Journal.
  3. (2018). "Enceladus and the Icy Moons of Saturn". [[The University of Arizona Press]].
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