Damocloid
Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter of 2 or less ( T J ≤ 2 ), [1] while Akimasa Nakamura defines this group with the following orbital criterion: [2]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
216433 characters 5 sections 8 paragraphs 2 images 111 internal links 299 external links |
damocloids 0.483 damocloid 0.294 akimasa 0.245 nakamura 0.245 tjupiter 0.221 tisserand 0.173 objects 0.169 halley 0.167 retrograde 0.162 parameter 0.135 comets 0.124 2002 0.117 coma 0.095 jupiter 0.094 criteria 0.090 |
Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter of 2 or less ( T J ≤ 2 ), [1] while Akimasa Nakamura defines this group with the following orbital criterion: [2] |
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| 2017 |
26782 characters 4 sections 5 paragraphs 0 images 71 internal links 11 external links |
damocloids 0.572 damocloid 0.262 objects 0.200 halley 0.198 comets 0.147 retrograde 0.144 2002 0.139 tisserand 0.137 coma 0.113 parameter 0.107 defines 0.104 cometary 0.099 127546 0.097 20461 0.097 343158 0.097 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter of 2 or less ( T J ≤ 2 ), [1] while Akimasa Nakamura defines this group with the following orbital criterion: [2] |
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| 2016 |
26866 characters 4 sections 4 paragraphs 0 images 71 internal links 11 external links |
damocloids 0.577 damocloid 0.264 objects 0.202 halley 0.200 comets 0.149 retrograde 0.145 2002 0.140 tisserand 0.138 coma 0.114 parameter 0.108 cometary 0.100 127546 0.097 20461 0.097 343158 0.097 65407 0.097 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter T J ≤ 2. [1] This can also loosely be defined as ( q < 5.2 AU , a > 8.0 AU, and e > 0.75) or i > 90 deg, [2] but this definition that does not focus on Jupiter excludes objects such as (127546) 2002 XU 93 , 2003 WG 166 , and 2004 DA 62 . [3] |
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| 2015 |
26852 characters 4 sections 4 paragraphs 0 images 71 internal links 11 external links |
damocloids 0.577 damocloid 0.264 objects 0.202 halley 0.200 comets 0.149 retrograde 0.145 2002 0.140 tisserand 0.138 coma 0.114 parameter 0.108 cometary 0.100 127546 0.097 20461 0.097 343158 0.097 65407 0.097 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter T J ≤ 2. [1] This can also loosely be defined as ( q < 5.2 AU , a > 8.0 AU, and e > 0.75) or i > 90 deg, [2] but this definition that does not focus on Jupiter excludes objects such as (127546) 2002 XU 93 , 2003 WG 166 , and 2004 DA 62 . [3] |
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| 2014 |
26861 characters 4 sections 4 paragraphs 0 images 71 internal links 11 external links |
damocloids 0.576 damocloid 0.264 objects 0.202 halley 0.199 comets 0.148 retrograde 0.145 2002 0.140 tisserand 0.138 coma 0.114 parameter 0.108 cometary 0.100 127546 0.097 20461 0.097 343158 0.097 65407 0.097 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet , but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Tisserand's parameter relative to Jupiter T J ≤ 2. [1] This can also loosely be defined as ( q < 5.2 AU , a > 8.0 AU, and e > 0.75) or i > 90 deg, [2] but this definition that does not focus on Jupiter excludes objects such as (127546) 2002 XU 93 , 2003 WG 166 , and 2004 DA 62 . [3] |
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| 2013 |
23113 characters 3 sections 5 paragraphs 0 images 66 internal links 10 external links |
damocloids 0.562 objects 0.230 damocloid 0.200 halley 0.170 comets 0.169 tisserand 0.157 coma 0.130 au 0.124 parameter 0.122 2002 0.120 cometary 0.113 orbits 0.112 127546 0.111 ce10 0.111 da62 0.111 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley-family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2012 |
23291 characters 3 sections 5 paragraphs 0 images 67 internal links 10 external links |
damocloids 0.561 objects 0.230 damocloid 0.200 halley 0.170 comets 0.169 tisserand 0.157 coma 0.130 au 0.124 parameter 0.122 2002 0.120 cometary 0.113 orbits 0.112 127546 0.111 ce10 0.111 da62 0.111 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2011 |
22634 characters 3 sections 5 paragraphs 0 images 67 internal links 9 external links |
damocloids 0.561 objects 0.229 damocloid 0.200 halley 0.170 comets 0.169 tisserand 0.156 coma 0.129 au 0.124 parameter 0.122 2002 0.119 cometary 0.113 orbits 0.112 127546 0.111 ce10 0.111 da62 0.111 |
Damocloids are minor planets such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2010 |
10769 characters 2 sections 3 paragraphs 0 images 52 internal links 3 external links |
damocloids 0.761 halley 0.198 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.104 loneos 0.104 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2009 |
10383 characters 1 sections 3 paragraphs 0 images 52 internal links 3 external links |
damocloids 0.761 halley 0.198 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.104 loneos 0.104 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2008 |
10420 characters 1 sections 3 paragraphs 0 images 52 internal links 3 external links |
damocloids 0.761 halley 0.198 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.104 loneos 0.104 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2007 |
10414 characters 1 sections 3 paragraphs 0 images 52 internal links 3 external links |
damocloids 0.761 halley 0.198 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.104 loneos 0.104 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2006 |
10217 characters 1 sections 3 paragraphs 0 images 51 internal links 3 external links |
damocloids 0.761 halley 0.197 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.103 loneos 0.103 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
|
| 2005 |
10139 characters 1 sections 4 paragraphs 0 images 50 internal links 3 external links |
damocloids 0.761 halley 0.197 comets 0.196 coma 0.151 cometary 0.132 ce10 0.129 hv60 0.129 vq94 0.129 5335 0.116 damocles 0.116 og108 0.116 spacewatch 0.103 loneos 0.103 objects 0.100 linear 0.100 |
Damocloids are asteroids such as 5335 Damocles and 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley , but without showing a cometary coma or tail. |
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| 2004 |
9141 characters 1 sections 3 paragraphs 0 images 45 internal links 1 external links |
og108 0.486 cometary 0.276 1p 0.269 5335 0.243 damocles 0.243 damocloid 0.243 damocloids 0.228 loneos 0.217 pw 0.201 coma 0.158 2001 0.155 renamed 0.147 tail 0.140 oort 0.140 halley 0.138 |
Damocloids are asteroids such as 5335 Damocles and (16746) 1996 PW that have long-period highly eccentric orbits typical of periodic comets such as 1P/Halley , but without showing a cometary coma or tail. |