Editing Dysnomia

Jump to navigation Jump to search

Warning: You are not logged in. Your IP address will be publicly visible if you make any edits. If you log in or create an account, your edits will be attributed to your username, along with other benefits.

The edit can be undone. Please check the comparison below to verify that this is what you want to do, and then save the changes below to finish undoing the edit.

Latest revision Your text
Line 1: Line 1:
{| 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"
+
#REDIRECT [[136199 Eris]]
!bgcolor="lightsteelblue" colspan="2" align="center" |Dysnomia
 
|-
 
|colspan="2" align="center"|[[Image:Dysnomia-ErisAndDysnomia-Orbiter2006P1.jpg|Eris|240px]]
 
|-
 
|colspan="2" align="center"|'''Dysnomia from ''ErisAndDysnomia.zip'' in Orbiter 2006P1'''
 
|-
 
!bgcolor="lightsteelblue" colspan="2"|Designation
 
|-
 
|Name||align="right"|Dysnomia
 
|-
 
|width="30%"|Reference body||align="right" width="30%"|Sun
 
|-
 
|width="30%"|Number of satellites||align="right" width="30%"|0
 
|-
 
!bgcolor="lightsteelblue" colspan="2"|Planetary mean orbits
 
|-
 
|width="30%"|Epoch||align="right" width="50%"|2005.71598173516
 
|-
 
|width="30%"|Semimajor axis (a)||align="right" width="50%"|37370000 m
 
|-
 
|width="30%"|Eccentricity (e)||align="right" width="30%"|0.013
 
|-
 
|width="30%"|Inclination (i)||align="right" width="30%"|142° <br> (2.478367537831948 radian)
 
|-
 
|width="30%"|Longitude of the ascending node (LAN, ☊)||align="right" width="30%"|261.198642253875° <br> (4.55877630906891 radian)
 
|-
 
|width="30%"|Longitude of periapsis (ϖ)||align="right" width="30%"|175.525689125061° <br> (3.06350119706432 radian)
 
|-
 
|width="30%"|Mean longitude (L)||align="right" width="30%"|247.512810230255° <br> (4.31991347938186 radian)
 
|-
 
!bgcolor="lightsteelblue" colspan="2"|Selected physical parameters
 
|-
 
|width="30%"|Mean radius||align="right" width="30%"|175000 m
 
|-
 
|width="30%"|Mass||align="right" width="30%"|4.07380803368229×10<sup>19</sup> kg
 
|-
 
|width="30%"|Sidereal rotation period||align="right" width="30%"|-848746.7853712236 sec (-9.82 days)
 
|-
 
|width="30%"|SidRotOffset||align="right" width="30%"|0
 
|-
 
|width="30%"|Obliquity||align="right" width="30%"|30.68° (0.535467015 radian)
 
|-
 
|width="30%"|LAN||align="right" width="30%"|0
 
|-
 
|width="30%"|Note||align="right" width="30%"|*Elements given are from Dysnomia.cfg (ErisAndDysnomia.zip)
 
|}
 
 
 
'''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.
 
 
 
Dysnomia was named after [[w:Dysnomia (deity)|Dysnomia]] the daughter of [[w:Eris (mythology)|Eris]].
 
 
 
== Dysnomia in Orbiter ==
 
Dysnomia 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>
 
|-
 
!Add-on!!Source!!Version!!Author!!Type!!Release Date!!Compatibility!!Wiki article
 
|-
 
|[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">
 
Dysnomia-ErisAndDysnomia-Orbiter2006P1.jpg|Dysnomia 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|Dysnomia]]
 
[[Category:Celestial bodies|Dysnomia]]
 
[[Category:Solar System|Dysnomia]]
 
[[Category:Natural satellites|Dysnomia]]
 
[[Category:Trans-Neptunian objects|Dysnomia]]
 
 
 
{{SolarSystem}}
 

Please note that all contributions to OrbiterWiki are considered to be released under the GNU Free Documentation License 1.2 (see OrbiterWiki:Copyrights for details). If you do not want your writing to be edited mercilessly and redistributed at will, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource. Do not submit copyrighted work without permission!

To protect the wiki against automated edit spam, we kindly ask you to solve the following hCaptcha:

Cancel Editing help (opens in new window)

Template used on this page: