Editing 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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#REDIRECT [[Fenrir]]
!bgcolor="lightsteelblue" colspan="2" align="center" |136199 Eris
 
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|colspan="2" align="center"|[[Image:136199Eris-ErisAndDysnomia-Orbiter2006P1.jpg|Eris|240px]]
 
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|colspan="2" align="center"|'''136199 Eris from ''ErisAndDysnomia.zip'' in Orbiter 2006P1'''
 
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!bgcolor="lightsteelblue" colspan="2"|Designation
 
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|Name||align="right"|136199 Eris
 
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|width="30%"|Reference body||align="right" width="30%"|Sun
 
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|width="30%"|Number of satellites||align="right" width="30%"|5
 
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!bgcolor="lightsteelblue" colspan="2"|Planetary mean orbits
 
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|width="30%"|Epoch||align="right" width="50%"|2005.71598173516
 
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|width="30%"|Semimajor axis (a)||align="right" width="50%"|10148508382333.42 m
 
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|width="30%"|Eccentricity (e)||align="right" width="30%"|0.4374901
 
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|width="30%"|Inclination (i)||align="right" width="30%"|44.07902° <br> (0.769324030052431 radian)
 
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|width="30%"|Longitude of the ascending node (LAN, ☊)||align="right" width="30%"|35.9276° <br> (0.627054912339515 radian)
 
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|width="30%"|Longitude of periapsis (ϖ)||align="right" width="30%"|187.50013° <br> (3.27249461641740 radian)
 
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|width="30%"|Mean longitude (L)||align="right" width="30%"|25.98231° <br> (0.453476856773848 radian)
 
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!bgcolor="lightsteelblue" colspan="2"|Selected physical parameters
 
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|width="30%"|Mean radius||align="right" width="30%"|1356407.61 m
 
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|width="30%"|Mass||align="right" width="30%"|4.28625×10<sup>22</sup> kg
 
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|width="30%"|Sidereal rotation period||align="right" width="30%"|138240 sec (38.4 hours)
 
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|width="30%"|SidRotOffset||align="right" width="30%"|0
 
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|width="30%"|Obliquity||align="right" width="30%"|30.68° (0.535467015 radian)
 
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|width="30%"|LAN||align="right" width="30%"|0
 
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|width="30%"|Note||align="right" width="30%"|*Elements given are from 136199 Eris.cfg (ErisAndDysnomia.zip)
 
|}
 
 
 
'''136199 Eris (2003 UB<sub>313</sub>)''' is the second largest after [[134340 Pluto]] and the most massive [[Dwarf planet]] in the solar system, and is a trans-Neptunian object in the scattered disc. Eris was discovered by [[w:Michael E. Brown|Mike Brown]] at the [[w:Palomar Observatory|Palomar Observatory]] in January 2005. There is a pre-discovery image from October 2003, but, it was not recognized due to its slow orbital motion.
 
 
 
Eris is named for [[w:Eris (mythology)|Eris]] the Greek goddess of strife and discord.
 
 
 
Eris has one satellite, [[Dysnomia]].
 
 
 
== Eris in Orbiter ==
 
Eris was first introduced with the release of ''ErisAndDysnomia.zip'' in May 2008.
 
 
 
{| class="wikitable" style="text-align: center"
 
|colspan="8"|<center>'''Orbiter versions and add-ons which include Pluto'''</center>
 
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!Add-on!!Source!!Version!!Author!!Type!!Release Date!!Compatibility!!Wiki article
 
|-
 
|[https://www.orbiter-forum.com/resources/celestial-bodies-motion-part-2-4-v2-0-0.295/ Celestial Bodies Motion - Part 2/4 - v2.0.0]||O-F Resources||v2.0.0||cristiapi||Scenery||2 July 2015||*module only||
 
|-
 
|[https://www.orbiter-forum.com/resources/eris-and-dysnomia.521/ Eris and Dysnomia]||O-F Resources||2008-05-10||Piper||Scenery||11 May 2008||||
 
|}
 
 
 
== Gallery ==
 
<gallery widths="100" heights="100">
 
136199Eris-ErisAndDysnomia-Orbiter2006P1.jpg|136199 Eris from ''ErisAndDysnomia.zip'' in Orbiter 2006P1</center>
 
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>
 
</gallery>
 
 
 
==References==
 
 
 
[[Category:Articles|Eris]]
 
[[Category:Celestial bodies|Eris]]
 
[[Category:Solar System|Eris]]
 
[[Category:Dwarf planets|Eris]]
 
[[Category:Trans-Neptunian objects|Eris]]
 
 
 
{{SolarSystem}}
 

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