Five-planet Nice model
The five-planet Nice model is a recent variation of the Nice model that begins with five giant planets , the current four plus an additional ice giant , in a chain of mean-motion resonances. After the resonance chain is broken, the five giant planets undergo a period of planetesimal-driven migration, followed by a gravitational instability similar to that in the original Nice model. During the instability the additional giant planet is scattered inward onto a Jupiter-crossing orbit and is ejected from the Solar System following an encounter with Jupiter. An early Solar System with five giant planets was proposed in 2011 after numerical models indicated that this is more likely to reproduce the current Solar System. [1]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
244619 characters 10 sections 27 paragraphs 2 images 251 internal links 263 external links |
planets 0.255 migration 0.240 disk 0.228 resonance 0.227 giant 0.227 instability 0.218 nice 0.214 jupiter 0.210 planetesimals 0.207 planetesimal 0.200 neptune 0.195 encounters 0.188 eccentricities 0.156 reproducing 0.149 bombardment 0.148 |
The five-planet Nice model is a recent variation of the Nice model that begins with five giant planets , the current four plus an additional ice giant , in a chain of mean-motion resonances. After the resonance chain is broken, the five giant planets undergo a period of planetesimal-driven migration, followed by a gravitational instability similar to that in the original Nice model. During the instability the additional giant planet is scattered inward onto a Jupiter-crossing orbit and is ejected from the Solar System following an encounter with Jupiter. An early Solar System with five giant planets was proposed in 2011 after numerical models indicated that this is more likely to reproduce the current Solar System. [1] |
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| 2017 |
237805 characters 10 sections 24 paragraphs 2 images 247 internal links 263 external links |
migration 0.269 planets 0.262 resonance 0.237 giant 0.232 nice 0.224 planetesimals 0.216 jupiter 0.214 neptune 0.198 disk 0.192 encounters 0.188 reproducing 0.171 planetesimal 0.165 eccentricities 0.164 instability 0.162 bombardment 0.155 |
The five-planet Nice model is a recent variation of the Nice model that begins with five giant planets , the current four plus an additional ice giant , in a chain of mean-motion resonances. After the resonance chain is broken, the five giant planets undergo a period of planetesimal-driven migration, followed by a gravitational instability similar to that in the original Nice model. During the instability the additional giant planet is scattered inward onto a Jupiter-crossing orbit and is ejected from the Solar System following an encounter with Jupiter. An early Solar System with five giant planets was proposed in 2011 after numerical models indicated that this is more likely to reproduce the current Solar System. [1] |
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| 2016 |
144094 characters 6 sections 14 paragraphs 2 images 218 internal links 145 external links |
planetesimals 0.289 giant 0.275 planets 0.259 jupiter 0.251 migration 0.226 eccentricities 0.212 saturn 0.185 neptune 0.175 planetesimal 0.173 resonance 0.160 disk 0.156 orbits 0.151 encounters 0.148 reproducing 0.147 nice 0.134 |
The five-planet Nice model is a recent variation of the Nice model that begins with five giant planets, the current four plus an additional ice giant, in a chain of mean-motion resonances. After the resonance chain is broken, the five giant planets undergo a period of planetesimal-driven migration, followed by a gravitational instability similar to that in the original Nice model. During the instability the additional giant planet is scattered inward onto a Jupiter-crossing orbit and is ejected from the Solar System following an encounter with Jupiter. An early Solar System with five giant planets was proposed in 2011 after numerical models indicated that this is more likely to reproduce the current Solar System. [1] |
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| 2015 |
67350 characters 4 sections 11 paragraphs 0 images 53 internal links 90 external links |
migration 0.313 eccentricities 0.258 reproducing 0.250 jupiter 0.240 giant 0.221 planetesimal 0.206 planets 0.204 neptune 0.199 resonance 0.164 saturn 0.157 simulations 0.154 inclinations 0.150 planetesimals 0.145 nice 0.143 belt 0.135 |
The hypothetical fifth giant planet is an additional planet added by some theorists to recent versions of the Nice model . The fifth giant planet is ejected from the Solar System following gravitational encounters with Saturn and Jupiter . The inclusion of five giant planets in numerical models of the early Solar System has been shown to increase the likelihood of their reproducing the current Solar System. [1] |
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| 2014 |
64856 characters 4 sections 9 paragraphs 0 images 51 internal links 88 external links |
reproducing 0.291 migration 0.252 jupiter 0.249 eccentricities 0.240 planets 0.238 giant 0.209 planetesimal 0.206 saturn 0.184 nice 0.166 resonance 0.148 outer 0.139 secular 0.135 planetesimals 0.135 neptune 0.135 simulations 0.134 |
The hypothetical fifth gas giant is an additional planet added by some theorists to recent versions of the Nice model . The fifth giant planet is ejected from the Solar System following gravitational encounters with Saturn and Jupiter . The inclusion of five giant planets in numerical models of the early Solar System has been shown to increase the likelihood of their reproducing the current Solar System. [1] |
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| 2013 |
14414 characters 5 sections 8 paragraphs 2 images 40 internal links 2 external links |
2. Hypothetical additional trans-Saturnian ice giant |
nesvorny 0.381 giant 0.284 uranus 0.161 solar 0.150 gas 0.140 intensive 0.140 hypothetical 0.139 expelled 0.129 jupiter 0.122 neptune 0.113 formation 0.108 survival 0.107 hypothesis 0.106 osaka 0.105 inconsistencies 0.105 |
The fifth gas giant hypothesis is an attempt to explain apparent inconsistencies in the formation of the Solar System . Apart from Jupiter , Saturn , Uranus and Neptune , theorists argue that there was once a fifth gas giant, which was expelled from the Solar System in its formative period. |
| 2012 |
14416 characters 5 sections 8 paragraphs 2 images 40 internal links 2 external links |
2. Hypothetical additional trans-Saturnian ice giant |
nesvorny 0.381 giant 0.284 uranus 0.161 solar 0.150 gas 0.140 intensive 0.140 hypothetical 0.139 expelled 0.129 jupiter 0.122 neptune 0.113 formation 0.108 survival 0.107 hypothesis 0.106 osaka 0.105 inconsistencies 0.105 |
The fifth gas giant hypothesis is an attempt to explain apparent inconsistencies in the formation of the Solar System . Apart from Jupiter , Saturn , Uranus and Neptune , theorists argue that there was once a fifth gas giant, which was expelled from the Solar System in its formative period. |
| 2011 |
14443 characters 5 sections 8 paragraphs 2 images 40 internal links 2 external links |
2. Hypothetical additional trans-Saturnian ice giant |
nesvorny 0.382 giant 0.284 uranus 0.162 solar 0.150 gas 0.140 intensive 0.140 hypothetical 0.140 expelled 0.129 jupiter 0.122 neptune 0.114 formation 0.109 survival 0.107 hypothesis 0.106 osaka 0.106 inconsistencies 0.106 |
The fifth gas giant hypothesis is an attempt to explain apparent inconsistencies in the formation of the Solar System . Apart from Jupiter , Saturn , Uranus and Neptune , theorists argue that there was once a fifth gas giant, which was expelled from the Solar System in its formative period. |