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Contents

   



(Top)
 


1 Notes  





2 References  





3 External links  














Bergelmir (moon)






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Bergelmir
Bergelmir imaged by the Cassini spacecraft in September 2014
Discovery
Discovered byS. Sheppard, D. Jewitt,
J. Kleyna, and B. Marsden
Discovery dateMay 4, 2005
Designations

Designation

Saturn XXXVIII
Pronunciation/ˈbɛərjɛlmɪər/or/ˈbɜːrɡəlmɪər/[a]

Named after

Bergelmir

Alternative names

S/2004 S 15
AdjectivesBergelmian[b]
Orbital characteristics[1]

Semi-major axis

19338000 km
Eccentricity0.142

Orbital period (sidereal)

1006.659 d[2]
Inclination158.5°
Satellite ofSaturn
GroupNorse group
Physical characteristics[2][3]

Mean diameter

5+50%
−30%
 km

Synodic rotation period

8.13±0.09 h
Albedo0.06 (assumed)

Apparent magnitude

24.2

Absolute magnitude (H)

15.2

BergelmirorSaturn XXXVIII (provisional designation S/2004 S 15) is a natural satelliteofSaturn. 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 kilometers (4 miles) in diameter,[3] 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 8.13±0.09 hours.[2]

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[edit]

  1. ^ The 'g' has a 'y' sound in Norse (indeed gelmir sounds like what it means in English, 'yeller'), but a spelling pronunciation would have it as 'g', as 'Aurgelmir' does in Merriam-Webster's Encyclopedia of Literature (1995).
  • ^ The oblique stem of the name is Bergelmi, as in Modern Norwegian Bergelme. The -r is the nominative case ending.
  • References[edit]

    1. ^ Ma, Yuehua; et al. (2010). "On the Origin of Retrograde Orbit Satellites around Saturn and Jupiter". Icy Bodies of the Solar System, Proceedings of the International Astronomical Union, IAU Symposium. 263: 157–160. Bibcode:2010IAUS..263..157M. doi:10.1017/S1743921310001687.
  • ^ a b c Denk, T.; Mottola, S. (2019). Cassini Observations of Saturn's Irregular Moons (PDF). 50th Lunar and Planetary Science Conference. Lunar and Planetary Institute.
  • ^ a b Denk, Tilmann; Mottola, Stefano; Tosi, Frederico; Bottke, William F.; Hamilton, Douglas P. (2018). "The Irregular Satellites of Saturn" (PDF). In Schenk, P.M.; Clark, R.N.; Howett, C.J.A.; Verbiscer, A.J.; Waite, J.H. (eds.). Enceladus and the Icy Moons of Saturn. Space Science Series. Vol. 322. Tucson, AZ: The University of Arizona Press. pp. 409–434. Bibcode:2018eims.book..409D. doi:10.2458/azu_uapress_9780816537075-ch020. ISBN 9780816537075.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Bergelmir_(moon)&oldid=1218164519"

    Categories: 
    Norse group
    Moons of Saturn
    Irregular satellites
    Discoveries by Scott S. Sheppard
    Astronomical objects discovered in 2005
    Moons with a retrograde orbit
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    This page was last edited on 10 April 2024, at 03:06 (UTC).

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