Concentric crater fill
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
87039 characters 3 sections 17 paragraphs 15 images 653 internal links 2 external links |
fill 0.544 concentric 0.528 casius 0.216 hiwish 0.184 phaethontis 0.174 crater 0.164 hirise 0.151 brain 0.149 cracks 0.140 location 0.134 cell 0.130 program 0.097 closed 0.095 believed 0.095 quadrangle 0.091 |
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2017 |
47113 characters 3 sections 15 paragraphs 16 images 167 internal links 5 external links |
concentric 0.517 fill 0.502 casius 0.226 crater 0.179 snow 0.169 brain 0.156 cracks 0.146 hiwish 0.144 cell 0.135 ice 0.130 hirise 0.126 debris 0.113 closed 0.100 believed 0.099 location 0.098 |
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2015 |
47111 characters 3 sections 15 paragraphs 16 images 167 internal links 5 external links |
concentric 0.517 fill 0.502 casius 0.226 crater 0.179 snow 0.169 brain 0.156 cracks 0.146 hiwish 0.144 cell 0.135 ice 0.130 hirise 0.126 debris 0.113 closed 0.100 believed 0.099 location 0.098 |
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2014 |
44183 characters 3 sections 12 paragraphs 13 images 165 internal links 5 external links |
fill 0.477 concentric 0.450 casius 0.215 snow 0.201 brain 0.185 cracks 0.174 cell 0.161 crater 0.157 ice 0.155 hiwish 0.143 debris 0.134 hirise 0.131 closed 0.118 believed 0.117 pits 0.105 |
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2013 |
43470 characters 3 sections 13 paragraphs 13 images 164 internal links 5 external links |
fill 0.476 concentric 0.401 casius 0.292 brain 0.201 cracks 0.189 cell 0.175 hirise 0.163 hiwish 0.155 ice 0.152 debris 0.146 crater 0.141 closed 0.129 believed 0.128 pits 0.115 lineated 0.108 |
A concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, [2] [3] and is widely believed to be caused by glacial movement. [4] [5] Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2012 |
17434 characters 3 sections 8 paragraphs 6 images 24 internal links 4 external links |
fill 0.493 concentric 0.458 casius 0.334 cracks 0.216 crater 0.161 hirise 0.139 debris 0.133 pits 0.131 movement 0.117 ice 0.115 brain 0.115 mensae 0.115 glacial 0.106 hiwish 0.106 location 0.104 |
Concentric crater fill is a landform where the floor of a crater is mostly covered with a large number of parallel ridges. [1] It is common in the mid-latitudes of Mars, and is widely believed to be caused by glacial movement. Areas on Mars called Deuteronilus Mensae and Protonilus Mensae contain many examples of concentric crater fill. |
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| 2011 |
18510 characters 3 sections 9 paragraphs 7 images 26 internal links 4 external links |
fill 0.495 concentric 0.459 casius 0.334 cracks 0.217 crater 0.161 hirise 0.140 debris 0.133 pits 0.131 movement 0.117 ice 0.116 brain 0.115 mensae 0.115 glacial 0.107 hiwish 0.107 location 0.104 |
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| 2010 |
13780 characters 2 sections 5 paragraphs 4 images 11 internal links 4 external links |
fill 0.541 concentric 0.488 debris 0.182 ice 0.158 brain 0.157 crater 0.157 erratics 0.141 cell 0.137 hirise 0.127 cracks 0.118 snowfall 0.108 movement 0.107 surfaces 0.100 believed 0.100 wall 0.097 |
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