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Narvi (moon)

Moon of Saturn


Summary

Moon of Saturn

FieldValue
nameNarvi
imageNarvi.jpg
captionNarvi's discovery image
pronounced
named_afterNarfi
alt_namesS/2003 S 1
discovered11 April 2003
discovererScott S. Sheppard et al.
orbit_ref
semimajor
inclination136.803°
eccentricity0.2990
period−995.33 days
satellite_ofSaturn
groupNorse group
albedo0.06 (assumed)
magnitude23.8
physical_ref{{cite conference
titleCassini Observations of Saturn's Irregular Moons
urlhttps://www.hou.usra.edu/meetings/lpsc2019/pdf/2654.pdf
first1T.last1=Denk
first2S.last2=Mottola
conference50th Lunar and Planetary Science Conference
publisherLunar and Planetary Institute
number2132
year2019}}
spectral_typeg – r = 0.24 ± 0.07, r – i = 0.42 ± 0.09
mean_radius
rotationh

Narvi or Saturn XXXI is a natural satellite of Saturn. It was discovered by a team of astronomers led by Scott S. Sheppard in 2003, and given the temporary designation S/2003 S 1.

Description

Narvi is about 7 kilometres in diameter, and orbits Saturn at an average distance of 19,371,000 km in 1006.541 days, at an inclination of 136.8° to the ecliptic (109° to Saturn's equator), in a retrograde direction and with an eccentricity of 0.2990, very similar to Bestla's orbit. Narvi's rotation period is hours, and its light curve has three minima like Siarnaq and Ymir. Unlike the other triangular moons, however, one minimum is much higher than the others, and the maximum that is a half-period ahead is much lower.{{cite conference

Naming

It was named in January 2005 after Narfi, a giant in Norse mythology. The name was approved by the IAU Working Group on Planetary System Nomenclature on 21 January 2005.

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". University of Arizona Press.
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