Classical Kuiper belt object
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune's orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
100657 characters 11 sections 23 paragraphs 7 images 220 internal links 53 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.365 objects 0.285 classical 0.278 cubewano 0.275 neptune 0.213 kbo 0.199 plutinos 0.195 orbits 0.174 belt 0.174 inclinations 0.173 au 0.153 inclination 0.147 kuiper 0.142 resonance 0.126 population 0.123 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune's orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2017 |
96329 characters 10 sections 22 paragraphs 6 images 217 internal links 49 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.379 objects 0.296 cubewano 0.285 classical 0.273 neptune 0.221 plutinos 0.203 orbits 0.181 inclinations 0.180 belt 0.153 inclination 0.153 au 0.142 kbo 0.138 resonance 0.131 population 0.127 populations 0.126 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2016 |
92209 characters 10 sections 22 paragraphs 6 images 222 internal links 38 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.383 objects 0.299 cubewano 0.288 classical 0.261 neptune 0.224 plutinos 0.205 orbits 0.183 inclinations 0.182 inclination 0.154 au 0.143 belt 0.140 kbo 0.139 resonance 0.132 population 0.129 populations 0.127 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2015 |
92150 characters 10 sections 22 paragraphs 6 images 221 internal links 37 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.417 cubewano 0.287 objects 0.285 classical 0.245 neptune 0.223 plutinos 0.204 orbits 0.182 inclinations 0.181 inclination 0.154 au 0.143 kbo 0.139 resonance 0.132 population 0.128 populations 0.127 belt 0.126 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2014 |
92975 characters 11 sections 24 paragraphs 6 images 224 internal links 37 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.417 cubewano 0.287 objects 0.285 classical 0.245 neptune 0.223 plutinos 0.204 orbits 0.182 inclinations 0.181 inclination 0.154 au 0.143 kbo 0.139 resonance 0.132 population 0.128 populations 0.127 belt 0.126 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o"), [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2013 |
84295 characters 10 sections 23 paragraphs 6 images 206 internal links 37 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.393 cubewano 0.295 objects 0.281 classical 0.252 neptune 0.229 plutinos 0.210 orbits 0.187 inclinations 0.186 inclination 0.158 kbo 0.143 resonance 0.136 population 0.132 populations 0.130 belt 0.129 hot 0.128 |
A classical Kuiper belt object , also called a cubewano ( / ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o") [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2012 |
83358 characters 10 sections 23 paragraphs 6 images 206 internal links 36 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.395 cubewano 0.296 objects 0.282 classical 0.237 neptune 0.230 plutinos 0.211 orbits 0.188 inclinations 0.187 inclination 0.159 kbo 0.143 resonance 0.136 population 0.132 populations 0.131 hot 0.128 qb1 0.119 |
A classical Kuiper belt object , also called a cubewano ( / [invalid input: 'icon'] ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o") [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2011 |
76373 characters 10 sections 23 paragraphs 6 images 205 internal links 23 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.395 cubewano 0.297 objects 0.282 classical 0.237 neptune 0.230 plutinos 0.211 orbits 0.188 inclinations 0.187 inclination 0.159 kbo 0.144 resonance 0.136 population 0.132 populations 0.131 hot 0.128 qb1 0.119 |
A classical Kuiper belt object , also called a cubewano ( / [invalid input: 'icon'] ˌ k juː b iː ˈ w ʌ n oʊ / "QB1-o") [1] is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune . Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto , do not cross Neptune’s orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. |
| 2010 |
72552 characters 9 sections 22 paragraphs 6 images 206 internal links 13 external links |
1. Orbits: 'hot' and 'cold' populations |
cubewanos 0.407 cubewano 0.306 objects 0.291 neptune 0.219 plutinos 0.218 classical 0.212 inclinations 0.193 orbits 0.168 kbo 0.148 inclination 0.146 resonance 0.141 population 0.137 populations 0.135 hot 0.132 belt 0.119 |
In astronomy a classical Kuiper belt object , also called a cubewano , [1] is a Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with the gas giant . Cubewanos have semi-major axes in the 40-50 AU range and, unlike Pluto , do not cross Neptune’s orbit. |
| 2009 |
68980 characters 9 sections 22 paragraphs 6 images 201 internal links 14 external links |
cubewanos 0.409 cubewano 0.308 objects 0.279 neptune 0.220 plutinos 0.219 classical 0.213 inclinations 0.194 orbits 0.182 kbo 0.149 inclination 0.146 resonance 0.141 population 0.137 populations 0.136 hot 0.133 belt 0.120 |
In astronomy a classical Kuiper Belt object , also called a cubewano , [1] is a Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with the giant planet. Cubewanos have semi-major axes in the 40-50 AU range and, unlike Pluto , do not cross Neptune’s orbit. |
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| 2008 |
57348 characters 6 sections 17 paragraphs 5 images 199 internal links 11 external links |
cubewanos 0.475 cubewano 0.262 neptune 0.258 objects 0.255 plutinos 0.239 inclinations 0.213 kbo 0.190 orbits 0.166 scatnear 0.131 resonance 0.129 classical 0.126 ecliptic 0.112 eccentricities 0.110 qb1 0.105 haumea 0.102 |
In astronomy a classical Kuiper Belt object , also called a cubewano ( Template:PronEng [ citation needed ] ), is a Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with the giant planet. Cubewanos have semi-major axes in the 40-50 AU range and, unlike Pluto , do not cross Neptune’s orbit. |
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| 2007 |
30958 characters 6 sections 17 paragraphs 3 images 88 internal links 9 external links |
cubewanos 0.433 objects 0.290 plutinos 0.273 neptune 0.267 inclinations 0.242 orbits 0.189 kbo 0.162 cubewano 0.149 resonance 0.147 template 0.126 eccentricities 0.125 el61 0.120 qb1 0.120 definition 0.110 belt 0.109 |
In astronomy a cubewano ( Template:PronEng [ citation needed ] (stress?)) is a Kuiper belt object that orbits beyond Neptune and is not controlled by an orbital resonance with the giant planet. Cubewanos have semi-major axes in the 40-50 AU range and, unlike Pluto , do not cross Neptune’s orbit. They are also called classical Kuiper Belt objects . |
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| 2006 |
28373 characters 5 sections 14 paragraphs 3 images 82 internal links 9 external links |
cubewanos 0.463 plutinos 0.292 neptune 0.286 inclinations 0.259 objects 0.248 orbits 0.182 cubewano 0.160 resonance 0.157 eccentricities 0.134 qb1 0.128 definition 0.118 belt 0.117 kbo 0.116 resonances 0.114 orbital 0.104 |
In astronomy a cubewano ( pronounced /kjuːbiːwənoʊ/ ) is a Kuiper belt object that orbits beyond Neptune and is not controlled by an orbital resonance with the giant planet. Cubewanos have semi-major axes in the 40-50 AU range and, unlike Pluto , do not cross Neptune’s orbit. They are also called classical Kuiper Belt objects. |
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| 2005 |
11136 characters 0 sections 3 paragraphs 0 images 54 internal links 0 external links |
qb1 0.531 cubewanos 0.479 cubewano 0.330 15760 0.240 odd 0.207 object 0.185 objects 0.171 resonances 0.157 neptunian 0.148 trans 0.135 41 0.133 1992 0.131 substantial 0.128 kuiper 0.128 au 0.123 |
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets . |
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| 2004 |
28575 characters 0 sections 4 paragraphs 2 images 185 internal links 0 external links |
qb1 0.436 cubewanos 0.393 os 0.271 cubewano 0.271 local 0.238 15760 0.197 supercluster 0.182 milky 0.171 odd 0.170 belt 0.158 object 0.152 objects 0.140 resonances 0.129 neptunian 0.122 trans 0.110 |
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets . |
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| 2003 |
1309 characters 0 sections 2 paragraphs 0 images 6 internal links 0 external links |
os 0.398 cubewano 0.398 qb1 0.320 smiley 0.289 cubewanos 0.289 odd 0.250 object 0.222 resonances 0.190 nicknamed 0.188 neptunian 0.178 trans 0.162 41 0.160 kuiper 0.154 au 0.148 controlled 0.148 |
A cubewano is a main Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets . |
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| 2002 |
1319 characters 0 sections 2 paragraphs 0 images 6 internal links 0 external links |
cubewano 0.436 qb1 0.351 smiley 0.316 cubewanos 0.316 odd 0.274 object 0.244 resonances 0.208 nicknamed 0.206 neptunian 0.196 trans 0.178 41 0.176 kuiper 0.169 au 0.162 controlled 0.162 belt 0.127 |
A Cubewano is a main Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets . |