Miranda , also designated Uranus V , is the smallest and innermost of Uranus 's five round satellites . It was discovered by Gerard Kuiper on 16 February 1948 at McDonald Observatory , and named after Miranda from William Shakespeare 's play The Tempest . [5] Like the other large moons of Uranus , Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle.
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
115601 characters 7 sections 11 paragraphs 12 images 208 internal links 51 external links |
miranda 0.841 uranus 0.248 coronae 0.143 uranian 0.118 satellites 0.096 shakespeare 0.095 tidal 0.093 umbriel 0.092 resonance 0.067 extensional 0.066 elsinore 0.056 inverness 0.056 ariel 0.053 moons 0.053 verona 0.051 |
Miranda , also designated Uranus V , is the smallest and innermost of Uranus 's five round satellites . It was discovered by Gerard Kuiper on 16 February 1948 at McDonald Observatory , and named after Miranda from William Shakespeare 's play The Tempest . [5] Like the other large moons of Uranus , Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. |
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2017 |
89166 characters 7 sections 14 paragraphs 10 images 199 internal links 42 external links |
miranda 0.827 uranus 0.267 shakespeare 0.139 umbriel 0.107 uranian 0.099 resonance 0.097 moons 0.088 satellites 0.075 verona 0.074 1948 0.073 extensional 0.072 tempest 0.069 tidal 0.068 fairies 0.066 mcdonald 0.064 |
Miranda , also designated Uranus V , is the smallest and innermost of Uranus 's five round satellites . It was discovered by Gerard Kuiper on 16 February 1948 at McDonald Observatory , and named after Miranda from William Shakespeare 's play The Tempest . [5] Like the other large moons of Uranus , Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. |
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2016 |
84886 characters 7 sections 15 paragraphs 10 images 195 internal links 41 external links |
miranda 0.836 uranus 0.246 shakespeare 0.116 umbriel 0.112 resonance 0.101 satellites 0.079 verona 0.077 uranian 0.077 1948 0.076 extensional 0.075 tempest 0.073 tidal 0.071 fairies 0.069 mcdonald 0.066 diapirs 0.064 |
Miranda or Uranus V is the smallest and innermost of Uranus 's five round satellites . Like the other large moons of Uranus , Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. At just 470 km in diameter, Miranda is one of the smallest objects in the Solar System known to be spherical under its own gravity . Of the bodies that are known to be in hydrostatic equilibrium, only Saturn 's moon Mimas is smaller. |
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2015 |
79871 characters 7 sections 15 paragraphs 9 images 197 internal links 37 external links |
miranda 0.821 uranus 0.258 shakespeare 0.121 umbriel 0.117 resonance 0.106 satellites 0.082 verona 0.081 uranian 0.081 1948 0.080 extensional 0.079 tempest 0.076 tidal 0.074 fairies 0.072 mcdonald 0.069 diapirs 0.067 |
Miranda or Uranus V is the smallest and innermost of Uranus 's five round satellites . Like the other large moons of Uranus , Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. At just 470 km in diameter, Miranda is one of the smallest objects in the Solar System known to be spherical under its own gravity . Of the bodies that are known to be in hydrostatic equilibrium, only Saturn 's moon Mimas is smaller. |
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2014 |
71173 characters 7 sections 13 paragraphs 9 images 196 internal links 17 external links |
miranda 0.813 uranus 0.264 shakespeare 0.124 umbriel 0.120 resonance 0.109 satellites 0.084 verona 0.083 uranian 0.083 1948 0.082 extensional 0.081 tempest 0.078 tidal 0.076 fairies 0.074 mcdonald 0.071 diapirs 0.069 |
Miranda or Uranus V is the smallest and innermost of Uranus 's five round satellites . Like the 27 other moons of Uranus , Miranda orbits in its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. At just 470 km in diameter, Miranda is one of the smallest objects in the Solar System known to be spherical under its own gravity . Of the bodies that are known to be in hydrostatic equilibrium, only Saturn 's moon Mimas is smaller. |
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2013 |
57104 characters 4 sections 10 paragraphs 9 images 188 internal links 12 external links |
miranda 0.727 resonance 0.235 umbriel 0.166 uranus 0.163 uranian 0.154 extensional 0.150 diapirs 0.127 tidal 0.106 moon 0.100 escaped 0.099 heating 0.094 flyby 0.080 incarnation 0.077 racetrack 0.077 patchwork 0.077 |
It was discovered by Gerard Kuiper on February 16, 1948 at McDonald Observatory . It was named after Miranda from William Shakespeare 's play The Tempest by Kuiper in his report of the discovery. [5] The adjectival form of the name is Mirandan . It is also designated Uranus V . |
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2012 |
57270 characters 4 sections 10 paragraphs 9 images 189 internal links 12 external links |
miranda 0.749 resonance 0.226 umbriel 0.160 uranus 0.157 uranian 0.148 extensional 0.144 diapirs 0.123 tidal 0.102 moon 0.097 escaped 0.095 heating 0.090 flyby 0.076 incarnation 0.074 racetrack 0.074 patchwork 0.074 |
It was discovered by Gerard Kuiper on February 16, 1948 at McDonald Observatory . It was named after Miranda from William Shakespeare 's play The Tempest by Kuiper in his report of the discovery. [5] The adjectival form of the name is Mirandan . It is also designated Uranus V . |
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2011 |
62259 characters 4 sections 10 paragraphs 9 images 190 internal links 23 external links |
miranda 0.728 resonance 0.220 umbriel 0.155 uranus 0.152 uranian 0.144 extensional 0.140 invalid 0.135 diapirs 0.119 circumference 0.110 tidal 0.099 moon 0.094 escaped 0.092 input 0.090 heating 0.088 icon 0.080 |
Miranda ( / [invalid input: 'icon'] m [invalid input: 'ɨ'] ˈ r æ n d ə / ) [5] is the smallest and innermost of Uranus 's five major moons . |
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2010 |
59329 characters 4 sections 9 paragraphs 9 images 189 internal links 17 external links |
miranda 0.740 uranus 0.199 resonance 0.171 extensional 0.152 diapirs 0.130 circumference 0.120 umbriel 0.113 tidal 0.108 uranian 0.104 moon 0.102 escaped 0.100 satellites 0.091 activity 0.081 flyby 0.081 incarnation 0.078 |
Miranda ( pronounced /mɨˈrændə/ (deprecated template) [4] ) is the smallest and innermost of Uranus ' five major moons . |
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2009 |
60860 characters 5 sections 8 paragraphs 8 images 199 internal links 17 external links |
miranda 0.740 uranus 0.199 resonance 0.171 extensional 0.152 diapirs 0.130 circumference 0.120 umbriel 0.113 tidal 0.108 uranian 0.104 moon 0.102 escaped 0.100 satellites 0.091 activity 0.081 flyby 0.081 incarnation 0.078 |
Miranda ( pronounced /mɨˈrændə/ (deprecated template) [4] ) is the smallest and innermost of Uranus ' five major moons . |
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2008 |
56639 characters 5 sections 8 paragraphs 8 images 193 internal links 15 external links |
miranda 0.720 uranus 0.209 resonance 0.179 extensional 0.159 diapirs 0.136 circumference 0.125 umbriel 0.118 tidal 0.113 uranian 0.109 moon 0.107 escaped 0.105 flyby 0.085 geologically 0.084 incarnation 0.082 racetrack 0.082 |
It was discovered by Gerard Kuiper on 1948-02-16 at McDonald Observatory . It was named after Miranda from William Shakespeare 's play The Tempest by Kuiper in his report of the discovery. [1] The adjectival form of the name is Mirandan . It is also designated Uranus V . |
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2007 |
40759 characters 5 sections 9 paragraphs 4 images 128 internal links 14 external links |
miranda 0.676 uranus 0.247 resonance 0.182 extensional 0.162 template 0.156 diapirs 0.138 circumference 0.128 umbriel 0.120 tidal 0.115 uranian 0.111 moon 0.109 escaped 0.107 flyby 0.086 geologically 0.085 incarnation 0.083 |
It was discovered by Gerard Kuiper on 1948-02-16 at McDonald Observatory . It was named after Prospero 's daughter in William Shakespeare 's play The Tempest by Kuiper in his report of the discovery. [1] The adjectival form of the name is Mirandan . It is also designated Uranus V . |
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2006 |
21657 characters 5 sections 12 paragraphs 3 images 65 internal links 7 external links |
miranda 0.625 uranus 0.294 earths 0.181 moon 0.176 resettled 0.128 culprit 0.128 geologically 0.118 incarnation 0.116 prospero 0.116 patchwork 0.116 template 0.108 upwellings 0.108 tempest 0.108 tidal 0.106 ipa 0.103 |
It was discovered by Gerard Kuiper on 1948-02-16 at McDonald Observatory . It is named after Prospero 's daughter in William Shakespeare 's play The Tempest . It is also designated Uranus V . |
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2005 |
11498 characters 3 sections 7 paragraphs 3 images 56 internal links 3 external links |
miranda 0.611 uranus 0.329 moon 0.169 resettled 0.143 culprit 0.143 prospero 0.129 patchwork 0.129 template 0.121 tempest 0.121 tidal 0.119 criss 0.115 mcdonald 0.111 geological 0.107 voyager 0.107 coronae 0.104 |
It was discovered by Gerard Kuiper on 1948-02-16 at McDonald Observatory . It is named after Prospero 's daughter in William Shakespeare 's play The Tempest . It is also designated Uranus V . |
|
2004 |
7287 characters 1 sections 5 paragraphs 2 images 43 internal links 3 external links |
miranda 0.722 uranus 0.227 prospero 0.178 patchwork 0.178 template 0.167 tempest 0.167 criss 0.159 geological 0.148 shakespeare 0.133 daughter 0.126 shattered 0.124 recognize 0.120 innermost 0.112 crossed 0.109 silicate 0.101 |
Miranda is the smallest and innermost of Uranus ' major moons . It is named after Prospero 's daughter in William Shakespeare 's play The Tempest . |
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2003 |
5417 characters 1 sections 1 paragraphs 2 images 30 internal links 1 external links |
miranda 0.540 patchwork 0.267 criss 0.238 uranus 0.226 shattered 0.186 gerard 0.183 1948 0.175 innermost 0.167 crossed 0.163 silicate 0.151 remainder 0.149 struck 0.145 activity 0.138 canyons 0.127 smallest 0.124 |
Miranda is the smallest and innermost of Uranus ' major moons . Discovered in 1948 by Gerard Kuiper , it roughly half water ice with the remainder being divided between silicate rock and methane -related organic compounds . Miranda's surface is criss-crossed by huge canyons up to 12 miles deep, with patchwork regions of broken terrain indicating intense geological activity in the moon's past. It is thought that this activity is likely powered by tidal forces from Uranus, but another theory suggests that Miranda was at some point struck by a massive object that partially shattered the moon. |
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2002 |
2734 characters 1 sections 3 paragraphs 0 images 9 internal links 2 external links |
miranda 0.754 uranus 0.237 disambiguation 0.206 patchwork 0.186 criss 0.166 shattered 0.129 gerard 0.127 1948 0.122 moon 0.121 innermost 0.116 crossed 0.114 silicate 0.105 remainder 0.104 struck 0.101 activity 0.096 |
This is about Miranda, the moon of Uranus. For other uses of the word, see Miranda (disambiguation) . |
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2001 |
1973 characters 0 sections 6 paragraphs 0 images 8 internal links 0 external links |
miranda 0.486 prospero 0.240 patchwork 0.240 tempest 0.225 criss 0.214 uranus 0.204 shakespeare 0.180 daughter 0.170 shattered 0.167 gerard 0.165 1948 0.158 innermost 0.150 crossed 0.147 silicate 0.136 remainder 0.134 |
2. The smallest and innermost of Uranus ' major moons . Discovered in 1948 by Gerard Kuiper , it roughly half water ice with the remainder being divided between silicate rock and methane -related organic compounds . Miranda's surface is criss-crossed by huge canyons up to 12 miles deep, with patchwork regions of broken terrain indicating intense geological activity in the moon's past. It is thought that this activity is likely powered by tidal stresses from Uranus, but another theory suggests that Miranda was at some point struck by a massive object that partially shattered the moon. |