Difference between revisions of "Dysnomia"

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m (Arvil moved page User:Arvil/Sandbox02 to Dysnomia: Move to article page.)
 
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#REDIRECT [[136199 Eris]]
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{| cellpadding="2" cellspacing="0" style="margin:25px 0 0 10px; border:3px solid lightsteelblue;width:250px; font-size:90%; font-family:'Arial','Helvetica'; float: right; clear: right;"Pluto in Orbiter"
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!bgcolor="lightsteelblue" colspan="2" align="center" |Dysnomia
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|-
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|colspan="2" align="center"|[[Image:Dysnomia-ErisAndDysnomia-Orbiter2006P1.jpg|Eris|240px]]
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|-
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|colspan="2" align="center"|'''Dysnomia from ''ErisAndDysnomia.zip'' in Orbiter 2006P1'''
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|-
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!bgcolor="lightsteelblue" colspan="2"|Designation
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|-
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|Name||align="right"|Dysnomia
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|-
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|width="30%"|Reference body||align="right" width="30%"|Sun
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|-
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|width="30%"|Number of satellites||align="right" width="30%"|0
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|-
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!bgcolor="lightsteelblue" colspan="2"|Planetary mean orbits
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|-
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|width="30%"|Epoch||align="right" width="50%"|2005.71598173516
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|-
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|width="30%"|Semimajor axis (a)||align="right" width="50%"|37370000 m
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|-
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|width="30%"|Eccentricity (e)||align="right" width="30%"|0.013
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|-
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|width="30%"|Inclination (i)||align="right" width="30%"|142° <br> (2.478367537831948 radian)
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|-
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|width="30%"|Longitude of the ascending node (LAN, ☊)||align="right" width="30%"|261.198642253875° <br> (4.55877630906891 radian)
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|-
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|width="30%"|Longitude of periapsis (ϖ)||align="right" width="30%"|175.525689125061° <br> (3.06350119706432 radian)
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|-
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|width="30%"|Mean longitude (L)||align="right" width="30%"|247.512810230255° <br> (4.31991347938186 radian)
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|-
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!bgcolor="lightsteelblue" colspan="2"|Selected physical parameters
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|-
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|width="30%"|Mean radius||align="right" width="30%"|175000 m
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|-
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|width="30%"|Mass||align="right" width="30%"|4.07380803368229×10<sup>19</sup> kg
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|-
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|width="30%"|Sidereal rotation period||align="right" width="30%"|-848746.7853712236 sec (-9.82 days)
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|-
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|width="30%"|SidRotOffset||align="right" width="30%"|0
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|-
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|width="30%"|Obliquity||align="right" width="30%"|30.68° (0.535467015 radian)
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|-
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|width="30%"|LAN||align="right" width="30%"|0
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|-
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|width="30%"|Note||align="right" width="30%"|*Elements given are from Dysnomia.cfg (ErisAndDysnomia.zip)
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|}
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'''Dysnomia (S/2005 (2003 UB<sub>313</sub>))''' is the only known satellite of the [[Dwarf planet]] 136199 Eris, and was discovered by [[w:Michael E. Brown|Mike Brown]] at the [[w:W. M. Keck Observatory|Keck Observatory]] in September 2005.
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Dysnomia was named after [[w:Dysnomia (deity)|Dysnomia]] the daughter of [[w:Eris (mythology)|Eris]].
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== Dysnomia in Orbiter ==
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Dysnomia was first introduced with the release of ''ErisAndDysnomia.zip'' in May 2008.
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{| class="wikitable" style="text-align: center"
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|colspan="8"|<center>'''Orbiter versions and add-ons which include Pluto'''</center>
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|-
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!Add-on!!Source!!Version!!Author!!Type!!Release Date!!Compatibility!!Wiki article
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|-
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|[https://www.orbiter-forum.com/resources/eris-and-dysnomia.521/ Eris and Dysnomia]||O-F Resources||2008-05-10||Piper||Scenery||11 May 2008||||
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|}
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== Gallery ==
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<gallery widths="100" heights="100">
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Dysnomia-ErisAndDysnomia-Orbiter2006P1.jpg|Dysnomia from ''ErisAndDysnomia.zip'' in Orbiter 2006P1</center>
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Hubble Dysnomia orbit overlay.jpg|<center>Image of Eris and Dysnomia by [[w:Hubble Space Telescope|Hubble]] in August 2006<br>from Wikimedia Commons</center>
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</gallery>
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==References==
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[[Category:Articles|Dysnomia]]
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[[Category:Celestial bodies|Dysnomia]]
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[[Category:Solar System|Dysnomia]]
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[[Category:Natural satellites|Dysnomia]]
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[[Category:Trans-Neptunian objects|Dysnomia]]
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{{SolarSystem}}

Latest revision as of 03:36, 23 October 2024

Dysnomia
Eris
Dysnomia from ErisAndDysnomia.zip in Orbiter 2006P1
Designation
Name Dysnomia
Reference body Sun
Number of satellites 0
Planetary mean orbits
Epoch 2005.71598173516
Semimajor axis (a) 37370000 m
Eccentricity (e) 0.013
Inclination (i) 142°
(2.478367537831948 radian)
Longitude of the ascending node (LAN, ☊) 261.198642253875°
(4.55877630906891 radian)
Longitude of periapsis (ϖ) 175.525689125061°
(3.06350119706432 radian)
Mean longitude (L) 247.512810230255°
(4.31991347938186 radian)
Selected physical parameters
Mean radius 175000 m
Mass 4.07380803368229×1019 kg
Sidereal rotation period -848746.7853712236 sec (-9.82 days)
SidRotOffset 0
Obliquity 30.68° (0.535467015 radian)
LAN 0
Note *Elements given are from Dysnomia.cfg (ErisAndDysnomia.zip)

Dysnomia (S/2005 (2003 UB313)) is the only known satellite of the Dwarf planet 136199 Eris, and was discovered by Mike Brown at the Keck Observatory in September 2005.

Dysnomia was named after Dysnomia the daughter of Eris.

Dysnomia in Orbiter[edit]

Dysnomia was first introduced with the release of ErisAndDysnomia.zip in May 2008.

Orbiter versions and add-ons which include Pluto
Add-on Source Version Author Type Release Date Compatibility Wiki article
Eris and Dysnomia O-F Resources 2008-05-10 Piper Scenery 11 May 2008

Gallery[edit]

  • Dysnomia from ErisAndDysnomia.zip in Orbiter 2006P1
  • Image of Eris and Dysnomia by Hubble in August 2006
    from Wikimedia Commons

References[edit]

edit The Solar System
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

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