Deuteronilus Mensae
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae, [2] south is Deuteronilus Colles . Other features are the large Lyot crater to the north and Sinton in the southeast, west is Mamers Valles and further north is the plain-basin of Vastitas Borealis . [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
125556 characters 7 sections 41 paragraphs 31 images 658 internal links 11 external links |
deuteronilus 0.472 mensae 0.400 ice 0.226 hiwish 0.208 ribbed 0.207 cracks 0.174 tilt 0.174 plains 0.162 hirise 0.162 terrain 0.138 upper 0.126 polygons 0.124 sublimation 0.122 unit 0.121 program 0.110 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae, [2] south is Deuteronilus Colles . Other features are the large Lyot crater to the north and Sinton in the southeast, west is Mamers Valles and further north is the plain-basin of Vastitas Borealis . [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2017 |
84008 characters 7 sections 41 paragraphs 34 images 168 internal links 10 external links |
deuteronilus 0.472 mensae 0.400 ice 0.226 hiwish 0.208 ribbed 0.207 cracks 0.174 tilt 0.174 plains 0.162 hirise 0.162 terrain 0.138 upper 0.126 polygons 0.124 sublimation 0.122 unit 0.121 program 0.110 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae, [2] south is Deuteronilus Colles . Other features are the large Lyot crater to the north and Sinton in the southeast, west is Mamers Valles and further north is the plain-basin of Vastitas Borealis . [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2016 |
81547 characters 7 sections 39 paragraphs 32 images 164 internal links 10 external links |
deuteronilus 0.439 mensae 0.392 ice 0.233 hiwish 0.215 ribbed 0.214 cracks 0.180 tilt 0.180 plains 0.168 hirise 0.167 terrain 0.143 upper 0.131 polygons 0.128 sublimation 0.126 unit 0.125 program 0.114 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2015 |
71185 characters 6 sections 31 paragraphs 27 images 161 internal links 9 external links |
deuteronilus 0.452 mensae 0.403 ribbed 0.233 ice 0.222 cracks 0.196 tilt 0.196 plains 0.182 hiwish 0.161 terrain 0.156 upper 0.142 unit 0.136 hirise 0.134 brain 0.118 dipping 0.115 sublimation 0.098 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2014 |
54041 characters 5 sections 17 paragraphs 18 images 157 internal links 8 external links |
deuteronilus 0.605 mensae 0.540 tilt 0.233 337 0.139 ice 0.136 hiwish 0.125 ismenius 0.100 hirise 0.096 degrees 0.088 lacus 0.087 terrain 0.085 43 0.081 photo 0.076 lag 0.071 rich 0.067 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2013 |
53222 characters 5 sections 17 paragraphs 17 images 157 internal links 8 external links |
deuteronilus 0.605 mensae 0.540 tilt 0.233 337 0.139 ice 0.136 hiwish 0.125 ismenius 0.100 hirise 0.096 degrees 0.088 lacus 0.087 terrain 0.085 43 0.081 photo 0.076 lag 0.071 rich 0.067 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] [7] |
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| 2012 |
26639 characters 5 sections 15 paragraphs 13 images 17 internal links 8 external links |
deuteronilus 0.625 mensae 0.557 337 0.153 hiwish 0.138 ismenius 0.111 hirise 0.105 tilt 0.103 lacus 0.096 terrain 0.094 43 0.089 photo 0.084 moisture 0.074 ismeniae 0.074 image 0.073 program 0.073 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] |
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| 2011 |
24429 characters 4 sections 13 paragraphs 11 images 17 internal links 8 external links |
deuteronilus 0.622 mensae 0.554 337 0.163 ismenius 0.118 tilt 0.109 lacus 0.102 hiwish 0.098 43 0.095 photo 0.089 terrain 0.080 hirise 0.080 moisture 0.079 ismeniae 0.079 image 0.078 glacier 0.072 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae. [2] [3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [5] [6] |
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| 2010 |
18646 characters 3 sections 13 paragraphs 12 images 17 internal links 7 external links |
deuteronilus 0.644 mensae 0.526 337 0.197 ismenius 0.142 lacus 0.123 hiwish 0.118 43 0.114 photo 0.108 terrain 0.097 hirise 0.097 image 0.094 glacier 0.087 location 0.086 showing 0.082 mound 0.081 |
Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W . It covers 344° -325° West and 40°-48° North. [1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle . It is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. [2] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [3] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [4] [5] |
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| 2009 |
8668 characters 2 sections 5 paragraphs 4 images 7 internal links 6 external links |
deuteronilus 0.618 mensae 0.459 337 0.378 43 0.220 937 0.136 glaciers 0.135 themis 0.121 region 0.119 knobby 0.117 persist 0.110 topped 0.106 glacier 0.084 highlands 0.081 arabia 0.076 cratered 0.075 |
Deuteronilus Mensae is a region on Mars 937 km across and located at 43°54′N 337°24′W / 43.9°N 337.4°W . Deuteronilus region lies just to the north of Arabia Terra. It is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. [1] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [2] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [3] |
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| 2008 |
6163 characters 2 sections 1 paragraphs 1 images 6 internal links 6 external links |
337 0.534 deuteronilus 0.437 43 0.311 mensae 0.260 937 0.193 glaciers 0.191 region 0.167 knobby 0.165 persist 0.155 topped 0.149 glacier 0.118 highlands 0.115 arabia 0.108 cratered 0.106 heavily 0.101 |
Deuteronilus Mensae is a region on Mars 937 km across and located at 43°54′N 337°24′W / 43.9°N 337.4°W . Deuteronilus region lies just to the north of Arabia Terra. It is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. [1] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [2] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice. [3] |
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| 2007 |
2763 characters 1 sections 1 paragraphs 0 images 1 internal links 2 external links |
337 0.654 43 0.380 937 0.236 glaciers 0.234 knobby 0.202 persist 0.190 topped 0.182 deuteronilus 0.178 mensae 0.159 region 0.154 glacier 0.144 54 0.122 000 0.110 flat 0.101 modern 0.099 |
Deuteronilus Mensae is a region on Mars 937 km across and located at 43°54′N 337°24′W / 43.9°N 337.4°W . The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago. [1] |