Hecates Tholus
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
41360 characters 5 sections 7 paragraphs 11 images 171 internal links 7 external links |
hecates 0.588 tholus 0.538 eruption 0.216 elysium 0.165 caldera 0.143 nightly 0.123 hecate 0.123 sorcery 0.123 domical 0.115 ghost 0.102 glaciers 0.101 volcano 0.097 albor 0.090 182 0.090 ridges 0.087 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2017 |
41207 characters 5 sections 6 paragraphs 11 images 171 internal links 7 external links |
hecates 0.588 tholus 0.538 eruption 0.216 elysium 0.165 caldera 0.143 nightly 0.123 hecate 0.123 sorcery 0.123 domical 0.115 ghost 0.102 glaciers 0.101 volcano 0.097 albor 0.090 182 0.090 ridges 0.087 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2016 |
38126 characters 4 sections 6 paragraphs 11 images 168 internal links 6 external links |
tholus 0.565 hecates 0.504 eruption 0.260 elysium 0.198 caldera 0.171 domical 0.138 glaciers 0.121 volcano 0.116 albor 0.108 182 0.108 ridges 0.105 northernmost 0.099 counts 0.094 ago 0.094 climate 0.088 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2015 |
38372 characters 5 sections 8 paragraphs 11 images 168 internal links 6 external links |
tholus 0.558 hecates 0.523 elysium 0.171 eruption 0.149 caldera 0.148 ridges 0.136 theorize 0.127 abducted 0.127 domical 0.119 tribe 0.119 theorists 0.113 imprisoned 0.105 glaciers 0.104 aliens 0.102 volcano 0.101 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2014 |
36497 characters 3 sections 6 paragraphs 11 images 168 internal links 6 external links |
tholus 0.582 hecates 0.519 elysium 0.204 eruption 0.178 caldera 0.176 domical 0.142 glaciers 0.124 volcano 0.120 albor 0.111 182 0.111 ridges 0.108 northernmost 0.102 counts 0.097 ago 0.097 climate 0.090 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2013 |
35945 characters 3 sections 6 paragraphs 10 images 169 internal links 6 external links |
tholus 0.582 hecates 0.519 elysium 0.204 eruption 0.178 caldera 0.176 domical 0.142 glaciers 0.124 volcano 0.120 albor 0.111 182 0.111 ridges 0.108 northernmost 0.102 counts 0.097 ago 0.097 climate 0.090 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2012 |
35128 characters 3 sections 7 paragraphs 9 images 169 internal links 6 external links |
tholus 0.583 hecates 0.521 elysium 0.205 eruption 0.179 caldera 0.177 domical 0.142 glaciers 0.125 volcano 0.120 albor 0.111 182 0.111 ridges 0.108 northernmost 0.103 counts 0.097 ago 0.097 climate 0.090 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis. [1] |
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| 2011 |
34073 characters 3 sections 6 paragraphs 8 images 165 internal links 6 external links |
tholus 0.586 hecates 0.523 elysium 0.206 eruption 0.179 caldera 0.178 domical 0.143 glaciers 0.125 volcano 0.121 albor 0.112 183 0.110 ridges 0.108 northernmost 0.103 counts 0.098 ago 0.098 climate 0.091 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis [1] . |
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| 2010 |
33851 characters 3 sections 6 paragraphs 8 images 164 internal links 5 external links |
tholus 0.586 hecates 0.523 elysium 0.206 eruption 0.179 caldera 0.178 domical 0.143 glaciers 0.125 volcano 0.121 albor 0.112 183 0.110 ridges 0.108 northernmost 0.103 counts 0.098 ago 0.098 climate 0.091 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis [1] . |
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| 2009 |
34132 characters 3 sections 6 paragraphs 8 images 164 internal links 5 external links |
tholus 0.556 hecates 0.496 32 0.227 150 0.198 elysium 0.195 eruption 0.170 caldera 0.169 domical 0.136 glaciers 0.119 volcano 0.114 albor 0.106 183 0.104 ridges 0.103 northernmost 0.098 counts 0.093 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10 km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis [1] . |
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| 2008 |
31644 characters 3 sections 4 paragraphs 6 images 162 internal links 4 external links |
tholus 0.453 hecates 0.283 elysium 0.278 eruption 0.243 caldera 0.240 10km 0.229 domical 0.193 glaciers 0.170 volcano 0.163 albor 0.151 183 0.149 northernmost 0.139 counts 0.132 ago 0.132 climate 0.123 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis [1] . |
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| 2007 |
11076 characters 3 sections 5 paragraphs 3 images 20 internal links 3 external links |
tholus 0.445 hecates 0.278 elysium 0.273 eruption 0.238 caldera 0.236 10km 0.225 template 0.190 domical 0.190 glaciers 0.166 volcano 0.160 albor 0.149 183 0.146 northernmost 0.137 counts 0.130 ago 0.130 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. The eruption created a caldera 10km in diameter. It has been suggested that glacial deposits later partly filled the caldera and an adjacent depression. Crater counts indicate this happened as recently as 5 to 20 million years ago. However climate models show that ice is not stable at Hecates Tholus today, pointing to climate change since the glaciers were active. It has been shown that the age of the glaciers correspond to a period of increased obliquity of Mars' rotational axis [1] . |
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| 2006 |
6237 characters 2 sections 4 paragraphs 2 images 17 internal links 2 external links |
tholus 0.459 elysium 0.376 eruption 0.328 domical 0.261 volcano 0.221 albor 0.205 183 0.201 hecates 0.191 northernmost 0.188 caldera 0.162 glacial 0.144 350 0.129 depressions 0.129 hill 0.127 notable 0.119 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. |
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| 2005 |
4087 characters 1 sections 3 paragraphs 1 images 14 internal links 1 external links |
tholus 0.459 elysium 0.376 eruption 0.328 domical 0.261 volcano 0.221 albor 0.205 183 0.201 hecates 0.191 northernmost 0.188 caldera 0.162 glacial 0.144 350 0.129 depressions 0.129 hill 0.127 notable 0.119 |
Hecates Tholus is a Martian volcano , notable for results from the European Space Agency 's Mars Express mission which indicate a major eruption took place 350 million years ago. |