Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is a region called the Martian dichotomy and parts of it contain fretted terrain. This terrain contains a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain shows up in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W, and in Aeolis Mensae , between 10 N and 10 S latitude and 240 W and 210 W longitude. [3] [4] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae .
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
76523 characters 8 sections 37 paragraphs 34 images 174 internal links 10 external links |
fretted 0.404 mensae 0.300 terrain 0.239 ismenius 0.212 debris 0.186 lacus 0.184 lobate 0.172 hirise 0.165 lineated 0.161 mesa 0.153 image 0.147 hiwish 0.146 deuteronilus 0.144 apron 0.131 fill 0.129 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is a region called the Martian dichotomy and parts of it contain fretted terrain. This terrain contains a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain shows up in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W, and in Aeolis Mensae , between 10 N and 10 S latitude and 240 W and 210 W longitude. [3] [4] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2017 |
75749 characters 8 sections 37 paragraphs 34 images 174 internal links 10 external links |
fretted 0.384 mensae 0.304 terrain 0.231 ismenius 0.215 debris 0.189 lacus 0.187 lobate 0.174 hirise 0.167 lineated 0.164 mesa 0.155 image 0.149 hiwish 0.148 deuteronilus 0.146 apron 0.133 fill 0.131 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is a region called the Martian dichotomy and parts of it contain fretted terrain. This terrain contains a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain shows up in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W, and in Aeolis Mensae , between 10 N and 10 S latitude and 240 W and 210 W longitude. [3] [4] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2016 |
70945 characters 8 sections 33 paragraphs 33 images 169 internal links 10 external links |
fretted 0.325 mensae 0.276 ismenius 0.224 terrain 0.216 lacus 0.194 hirise 0.193 lobate 0.179 mesa 0.179 debris 0.174 hiwish 0.171 deuteronilus 0.169 lineated 0.162 image 0.156 ctx 0.150 glaciers 0.148 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2015 |
70416 characters 8 sections 33 paragraphs 33 images 171 internal links 10 external links |
fretted 0.322 mensae 0.273 ismenius 0.222 terrain 0.214 lda 0.208 lacus 0.192 hirise 0.191 lobate 0.177 mesa 0.177 debris 0.173 hiwish 0.169 deuteronilus 0.167 lineated 0.160 image 0.154 ctx 0.149 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2014 |
62870 characters 8 sections 25 paragraphs 25 images 171 internal links 10 external links |
fretted 0.418 mensae 0.355 terrain 0.229 deuteronilus 0.217 hirise 0.196 glaciers 0.166 lineations 0.155 ice 0.141 hiwish 0.139 reull 0.136 ismenius 0.128 image 0.126 mesas 0.121 protonilus 0.117 floors 0.115 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2013 |
62877 characters 8 sections 25 paragraphs 25 images 171 internal links 10 external links |
fretted 0.418 mensae 0.355 terrain 0.229 deuteronilus 0.217 hirise 0.196 glaciers 0.166 lineations 0.155 ice 0.141 hiwish 0.139 reull 0.136 ismenius 0.128 image 0.126 mesas 0.121 protonilus 0.117 floors 0.115 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2012 |
41511 characters 8 sections 25 paragraphs 21 images 38 internal links 9 external links |
fretted 0.418 mensae 0.354 terrain 0.229 deuteronilus 0.217 hirise 0.196 glaciers 0.166 lineations 0.155 ice 0.140 hiwish 0.139 reull 0.136 ismenius 0.128 image 0.126 mesas 0.121 protonilus 0.117 floors 0.115 |
Fretted terrain is a type of surface feature common to certain areas of Mars and was discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , and straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2011 |
38321 characters 8 sections 27 paragraphs 21 images 33 internal links 7 external links |
fretted 0.418 mensae 0.355 terrain 0.229 deuteronilus 0.217 hirise 0.196 glaciers 0.166 lineations 0.155 ice 0.141 hiwish 0.140 reull 0.136 ismenius 0.128 image 0.127 mesas 0.121 protonilus 0.117 floors 0.115 |
Fretted terrain is a type of surface feature common to certain areas of Mars and discovered in Mariner 9 images. It lies between two different types of terrain. The surface of Mars can be divided into two parts : low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Two good examples of fretted terrain are Deuteronilus Mensae and Protonilus Mensae . |
|
2010 |
35420 characters 8 sections 27 paragraphs 21 images 26 internal links 7 external links |
fretted 0.389 mensae 0.363 deuteronilus 0.222 terrain 0.201 hirise 0.200 glaciers 0.170 lineations 0.158 ice 0.144 hiwish 0.143 reull 0.139 ismenius 0.131 image 0.130 mesas 0.124 protonilus 0.120 floors 0.118 |
Fretted Terrain is a type of surface feature common to certain areas of Mars and discovered in Mariner 9 images. It lies between two different surfaces. The surface of Mars can be divided into two parts: low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and a small part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , straight-walled and sinuous canyons . [1] It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [2] Fretted terrain is most common in northern Arabia , between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [3] Parts of the fretted terrain are called Deuteronilus Mensae and Protonilus Mensae. |
|
2009 |
20072 characters 2 sections 15 paragraphs 11 images 16 internal links 6 external links |
fretted 0.496 glaciers 0.217 terrain 0.213 lineations 0.202 reull 0.178 ice 0.155 floors 0.150 cliffs 0.148 lineated 0.136 ismenius 0.125 striations 0.125 debris 0.122 hirise 0.119 aprons 0.119 coloe 0.116 |
Fretted Terrain is a type of surface feature common to certain areas of Mars and discovered in Mariner 9 images. It lies between two different surfaces. The surface of Mars can be divided into two parts: low, young, uncratered plains that cover most of the northern hemisphere, and high-standing, old, heavily cratered areas that cover the southern and part of the northern hemisphere. Between these two zones is the fretted terrain, containing a complicated mix of cliffs, mesas , buttes , straight-walled and sinuous canyons . It contains smooth, flat lowlands along with steep cliffs. The scarps or cliffs are usually 1 to 2 km high. Channels in the area have wide, flat floors and steep walls. [1] Fretted terrain is most common in northern Arabia, between latitudes 30°N and 50°N and longitudes 270°W and 360°W. [2] Parts of the fretted terrain are called Deuteronilus Mensae and Protonilus Mensae. |