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 UB 313 ) 1 until officially named Dysnomia [5] (from the Ancient Greek word Δυσνομία meaning anarchy/lawlessness) after the daughter of the Greek goddess Eris .
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
99821 characters 8 sections 10 paragraphs 6 images 277 internal links 24 external links |
dysnomia 0.620 eris 0.365 xena 0.207 δυσνομία 0.172 brown 0.164 pronounces 0.115 wife 0.106 nickname 0.106 adaptive 0.105 lawlessness 0.103 fainter 0.101 optics 0.097 gabrielle 0.097 keck 0.096 ub313 0.092 |
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 UB 313 ) 1 until officially named Dysnomia [5] (from the Ancient Greek word Δυσνομία meaning anarchy/lawlessness) after the daughter of the Greek goddess Eris . |
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2017 |
97679 characters 7 sections 8 paragraphs 6 images 275 internal links 24 external links |
dysnomia 0.545 eris 0.437 xena 0.212 brown 0.192 δυσνομία 0.176 fainter 0.172 pronounces 0.118 wife 0.109 nickname 0.109 adaptive 0.107 mike 0.107 lawlessness 0.106 optics 0.100 gabrielle 0.099 keck 0.098 |
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 UB 313 ) 1 until officially named Dysnomia [6] (from the Ancient Greek word Δυσνομία meaning anarchy/lawlessness) after the daughter of the Greek goddess Eris . |
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2016 |
89814 characters 7 sections 8 paragraphs 5 images 269 internal links 22 external links |
dysnomia 0.545 eris 0.437 xena 0.212 brown 0.192 δυσνομία 0.176 fainter 0.172 pronounces 0.118 wife 0.109 nickname 0.109 adaptive 0.107 mike 0.107 lawlessness 0.106 optics 0.100 gabrielle 0.099 keck 0.098 |
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 UB 313 ) 1 until officially named Dysnomia [6] (from the Ancient Greek word Δυσνομία meaning anarchy/lawlessness) after the daughter of the Greek goddess Eris . |
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2015 |
89722 characters 7 sections 9 paragraphs 5 images 269 internal links 21 external links |
dysnomia 0.506 eris 0.474 xena 0.215 brown 0.194 δυσνομία 0.179 fainter 0.174 pronounces 0.119 wife 0.110 nickname 0.110 adaptive 0.109 mike 0.109 pluto 0.108 lawlessness 0.107 optics 0.101 gabrielle 0.101 |
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 UB 313 ) 1 until officially named Dysnomia [6] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2014 |
104803 characters 7 sections 10 paragraphs 6 images 314 internal links 21 external links |
dysnomia 0.540 eris 0.464 xena 0.210 brown 0.190 δυσνομία 0.175 fainter 0.170 pronounces 0.117 wife 0.108 nickname 0.108 adaptive 0.106 mike 0.106 pluto 0.106 lawlessness 0.105 optics 0.099 gabrielle 0.098 |
Dysnomia , officially (136199) Eris I Dysnomia ( Greek : Δυσνομία ), 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 UB 313 ) 1 until officially named Dysnomia [7] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2013 |
94084 characters 6 sections 9 paragraphs 4 images 275 internal links 21 external links |
dysnomia 0.508 eris 0.475 xena 0.216 brown 0.195 δυσνομία 0.179 fainter 0.175 pronounces 0.120 wife 0.111 nickname 0.111 adaptive 0.109 mike 0.109 pluto 0.108 lawlessness 0.108 optics 0.101 gabrielle 0.101 |
Dysnomia , officially (136199) Eris I Dysnomia ( Greek : Δυσνομία ), 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 UB 313 ) 1 until officially named Dysnomia [7] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2012 |
82145 characters 6 sections 9 paragraphs 3 images 257 internal links 21 external links |
dysnomia 0.508 eris 0.475 xena 0.216 brown 0.195 δυσνομία 0.179 fainter 0.175 pronounces 0.119 wife 0.111 nickname 0.111 adaptive 0.109 mike 0.109 pluto 0.108 lawlessness 0.108 optics 0.101 gabrielle 0.101 |
Dysnomia , officially (136199) Eris I Dysnomia ( Greek : Δυσνομία ), 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 UB 313 ) 1 until officially named Dysnomia [7] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2011 |
71428 characters 6 sections 8 paragraphs 3 images 253 internal links 11 external links |
dysnomia 0.529 eris 0.429 xena 0.224 brown 0.203 gabrielle 0.158 pronounces 0.124 δυσνομία 0.124 wife 0.115 nickname 0.115 adaptive 0.114 mike 0.114 pluto 0.113 lawlessness 0.112 sidekick 0.112 fainter 0.109 |
Dysnomia , 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 UB 313 ) 1 until officially named Dysnomia [6] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2010 |
70794 characters 6 sections 8 paragraphs 4 images 252 internal links 9 external links |
dysnomia 0.536 eris 0.435 xena 0.228 brown 0.180 gabrielle 0.160 pronounces 0.126 δυσνομία 0.126 wife 0.117 nickname 0.117 adaptive 0.115 pluto 0.114 lawlessness 0.114 sidekick 0.114 optics 0.107 keck 0.106 |
Dysnomia , officially (136199) Eris I Dysnomia , is the only known moon of the dwarf planet Eris (the largest 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 UB 313 ) 1 until officially named Dysnomia [5] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2009 |
70200 characters 6 sections 8 paragraphs 4 images 251 internal links 9 external links |
dysnomia 0.538 eris 0.436 xena 0.228 brown 0.180 gabrielle 0.160 pronounces 0.126 δυσνομία 0.126 wife 0.117 nickname 0.117 adaptive 0.116 pluto 0.115 lawlessness 0.114 sidekick 0.114 optics 0.107 keck 0.106 |
Dysnomia , officially (136199) Eris I Dysnomia , is the only known moon of the dwarf planet Eris . 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 UB 313 ) 1 until officially named Dysnomia [5] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2008 |
68405 characters 5 sections 8 paragraphs 4 images 256 internal links 9 external links |
dysnomia 0.486 eris 0.400 xena 0.227 δυσνομία 0.188 brown 0.179 template 0.159 gabrielle 0.159 pronounces 0.126 wife 0.117 nickname 0.117 adaptive 0.115 pluto 0.114 noh 0.113 lawlessness 0.113 sidekick 0.113 |
Dysnomia ( pronounced /dɪsˈnoʊmiə/ (deprecated template) dis- NOH -mee-ə , Template:IPAlink-en dyes- NOH -mee-ə , or as in Greek Δυσνομία), officially (136199) Eris I Dysnomia , is the only known moon of the dwarf planet Eris . 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 UB 313 ) 1 until officially named Dysnomia [4] (from the Ancient Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2007 |
58986 characters 5 sections 8 paragraphs 4 images 244 internal links 5 external links |
dysnomia 0.516 eris 0.424 xena 0.241 δυσνομία 0.200 gabrielle 0.169 brown 0.136 adaptive 0.122 pluto 0.121 lawlessness 0.120 sidekick 0.120 optics 0.113 keck 0.112 princess 0.107 ub313 0.107 warrior 0.097 |
Dysnomia ( Template:PronEng dis-noe'-mee-ə, Greek Δυσνομία), officially designated (136199) Eris I Dysnomia , is a moon of the dwarf planet Eris . 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 UB 313 ) 1 until officially named Dysnomia [4] (from the Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2006 |
51311 characters 5 sections 7 paragraphs 4 images 234 internal links 4 external links |
dysnomia 0.518 eris 0.391 xena 0.302 lawlessness 0.181 gabrielle 0.170 brown 0.136 δυσνομία 0.134 adaptive 0.122 lawless 0.121 sidekick 0.121 actress 0.121 optics 0.113 keck 0.112 princess 0.108 ub313 0.108 |
Dysnomia ( IPA: [dɪsˈnoʊmiə] ), officially designated (136199) Eris I Dysnomia , is a moon of the dwarf planet Eris . 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 UB 313 ) 1 until officially named Dysnomia [1] (from the Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris . |
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2005 |
865 characters 0 sections 1 paragraphs 0 images 1 internal links 0 external links |
redirect 1.000 |