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::Dysnomia (moon)

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{{#invoke:Hatnote|hatnote}} {{#invoke:Infobox|infobox}}

Dysnomia (Greek: Δυσνομία)—officially (136199) Eris I Dysnomia—is the only known moon of the dwarf planet Eris (the most massive known dwarf planet in the Solar System). It was discovered in 2005 by Mike Brown and the laser guide star adaptive optics team at the W. M. Keck Observatory, and carried the provisional designation of S/2005 (2003 UB313) 1 until officially named Dysnomia<ref name="IAUC 8747"/> (from the Ancient Greek word Δυσνομία{{#invoke:Category handler|main}} meaning "lawlessness") after the daughter of the Greek goddess Eris.


Dysnomia (moon) sections
Intro   Discovery    Properties    Formation    Name    Notes    References   External links  

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Brown::dysnomia    First::title    Journal::planet    Dwarf::pluto    Category::times    Fainter::schaller

{{#invoke:Hatnote|hatnote}} {{#invoke:Infobox|infobox}}

Dysnomia (Greek: Δυσνομία)—officially (136199) Eris I Dysnomia—is the only known moon of the dwarf planet Eris (the most massive known dwarf planet in the Solar System). It was discovered in 2005 by Mike Brown and the laser guide star adaptive optics team at the W. M. Keck Observatory, and carried the provisional designation of S/2005 (2003 UB313) 1 until officially named Dysnomia<ref name="IAUC 8747"/> (from the Ancient Greek word Δυσνομία{{#invoke:Category handler|main}} meaning "lawlessness") after the daughter of the Greek goddess Eris.


Dysnomia (moon) sections
Intro   Discovery    Properties    Formation    Name    Notes    References   External links  

PREVIOUS: IntroNEXT: Discovery
<<>>