Difference between revisions of "Rosalind"
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!bgcolor="lightsteelblue" colspan="2" align="center" |Rosalind | !bgcolor="lightsteelblue" colspan="2" align="center" |Rosalind | ||
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− | |colspan="2" align="center"|[[Image:Rosalind- | + | |colspan="2" align="center"|[[Image:Rosalind-outerplanets060929basezip-Orbiter2006P1.jpg|240px]] |
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− | |colspan="2" align="center"|<center>'''Rosalind from ''outerplanets- | + | |colspan="2" align="center"|<center>'''Rosalind from ''outerplanets-060929-base.zip'' in Orbiter 2006P1'''</center> |
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!bgcolor="lightsteelblue" colspan="2"|Designation | !bgcolor="lightsteelblue" colspan="2"|Designation | ||
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!bgcolor="lightsteelblue" colspan="2"|Planetary mean orbits | !bgcolor="lightsteelblue" colspan="2"|Planetary mean orbits | ||
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− | |width="30%"|Epoch||align="right" width="50%"| | + | |width="30%"|Epoch||align="right" width="50%"|2006.64792344792 |
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− | |width="30%"|Semimajor axis (a)||align="right" width="50%"| | + | |width="30%"|Semimajor axis (a)||align="right" width="50%"|70011150.6873456 m |
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− | |width="30%"|Eccentricity (e)||align="right" width="30%"|0. | + | |width="30%"|Eccentricity (e)||align="right" width="30%"|0.00105548039257262 |
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− | |width="30%"|Inclination (i)||align="right" width="30%"|97. | + | |width="30%"|Inclination (i)||align="right" width="30%"|97.4426833884616° <br> (1.70069565710704 radian) |
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− | |width="30%"|Longitude of the ascending node (LAN, ☊)||align="right" width="30%"|167. | + | |width="30%"|Longitude of the ascending node (LAN, ☊)||align="right" width="30%"|167.645177174286° <br> (2.92596031678053 radian) |
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− | |width="30%"|Longitude of periapsis (ϖ)||align="right" width="30%"| | + | |width="30%"|Longitude of periapsis (ϖ)||align="right" width="30%"|186.570247247043° <br> (3.25626510072078 radian) |
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− | |width="30%"|Mean longitude (L)||align="right" width="30%"| | + | |width="30%"|Mean longitude (L)||align="right" width="30%"|546.030572819725° <br> (9.53003131225485 radian) |
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!bgcolor="lightsteelblue" colspan="2"|Selected physical parameters | !bgcolor="lightsteelblue" colspan="2"|Selected physical parameters | ||
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|width="30%"|LAN||align="right" width="30%"|2.9255 | |width="30%"|LAN||align="right" width="30%"|2.9255 | ||
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− | |width="30%"|Note||align="right" width="30%"|*Elements given are from Rosalind.cfg ( | + | |width="30%"|Note||align="right" width="30%"|*Elements given are from Rosalind.cfg (outer_planets-060929.zip) |
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!Add-on!!Source!!Version!!Author!!Type!!Release Date!!Compatibility!!Wiki article | !Add-on!!Source!!Version!!Author!!Type!!Release Date!!Compatibility!!Wiki article | ||
+ | |- | ||
+ | |[https://library.avsim.net/esearch.php?DLID=&Name=&FileName=outer_planets-060929-base.zip&Author=&CatID=root The Outer Planets 060929 Base]||AVSIM||||Rolf Keibel<br>Carl Romanik<br>Tony Dunn||Scenery||30 September 2006||Orbiter 2006-P1|| | ||
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|[https://library.avsim.net/esearch.php?DLID=&Name=&FileName=outerplanets-050329_update.zip&Author=&CatID=root The Outer Planets 050329 Update]||AVSIM||050329||Rolf Keibel<br>Tony Dunn<br>Carl Romanik||Scenery||30 March 2005|||| | |[https://library.avsim.net/esearch.php?DLID=&Name=&FileName=outerplanets-050329_update.zip&Author=&CatID=root The Outer Planets 050329 Update]||AVSIM||050329||Rolf Keibel<br>Tony Dunn<br>Carl Romanik||Scenery||30 March 2005|||| | ||
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Rosalind-UranusMoonszip-Orbiter2003P2.jpg|<center>Rosalind from ''UranusMoons.zip'' in Orbiter 2003P2</center> | Rosalind-UranusMoonszip-Orbiter2003P2.jpg|<center>Rosalind from ''UranusMoons.zip'' in Orbiter 2003P2</center> | ||
Rosalind-outerplanets050125zip-Orbiter2005P1.jpg|<center>Rosalind from ''outerplanets-050125.zip'' in Orbiter 2005P1</center> | Rosalind-outerplanets050125zip-Orbiter2005P1.jpg|<center>Rosalind from ''outerplanets-050125.zip'' in Orbiter 2005P1</center> | ||
+ | Rosalind-outerplanets060929basezip-Orbiter2006P1.jpg|<center>Rosalind from ''outer_planets-0609029-base.zip'' in Orbiter 2006P1</center> | ||
Rosalindmoon.png|<center>Rosalind imaged from the [[w:Hubble Space Telescope|Hubble Space Telescope]] in 1997,<br>from Wikimedia Commons</center> | Rosalindmoon.png|<center>Rosalind imaged from the [[w:Hubble Space Telescope|Hubble Space Telescope]] in 1997,<br>from Wikimedia Commons</center> | ||
</gallery> | </gallery> |
Revision as of 03:02, 17 October 2024
Rosalind (Uranus XIII, S/1986 U 4) is one of the inner satellites of Uranus. It was discovered by the Voyager2 spacecraft in January 1986. It is named after the daughter of the banished Duke in Shakespeare's As You Like It.
Rosalind in Orbiter
Rosalind was first introduced into Orbiter with the add-on uranus.zip in November 2002.
Add-on | Source | Version | Author | Type | Release Date | Compatibility | Wiki article |
---|---|---|---|---|---|---|---|
The Outer Planets 060929 Base | AVSIM | Rolf Keibel Carl Romanik Tony Dunn |
Scenery | 30 September 2006 | Orbiter 2006-P1 | ||
The Outer Planets 050329 Update | AVSIM | 050329 | Rolf Keibel Tony Dunn Carl Romanik |
Scenery | 30 March 2005 | ||
The Outer Planets 050125 | AVSIM | 050125 | Rolf Keibel Tony Dunn |
Scenery | 26 January 2005 | Orbiter 2005-P1 | |
Uranus Minor Moons | O-F Resources | 2004-12-14 | Nighthawke | Scenery | 14 December 2004 | ||
Uranus | AVSIM | Rolf Keibel | Scenery | 5 November 2002 |
Rosalind imaged from the Hubble Space Telescope in 1997,
from Wikimedia Commons
Uranus's natural satellites |
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Named Satellites:
Ariel | Belinda | Bianca | Caliban | Cordelia | Cressida | Cupid | Desdemona | Ferdinand | Francisco | Juliet | Mab | Margaret | Miranda | Oberon | Ophelia | Perdita | Portia | Prospero | Puck | Rosalind | Setebos | Stephano | Sycorax | Titania | Trinculo | Umbriel Numbered Satellites: |
See also: Pronunciation key | rings of Uranus |
edit The Solar System | |
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Central star |
Sun (Sol) |
Planets |
Mercury - Venus - Earth - Mars - Jupiter - Saturn - Uranus - Neptune |
Natural satellites |
Moon - Phobos - Deimos - Io - Europa - Ganymede - Titan - more... |
Add-ons |
Planets - Dwarf Planets - Small objects - Natural satellites - Alternative star systems |
This natural satellite related article is a stub. You can help Orbiterwiki by expanding it.
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