Chryse Planitia
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 28°24′N 319°42′E / 28.4°N 319.7°E . [1] Chryse Planitia lies partially in the Lunae Palus quadrangle , partially in the Oxia Palus quadrangle , partially in the Mare Acidalium quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
85580 characters 3 sections 9 paragraphs 8 images 661 internal links 10 external links |
chryse 0.646 valles 0.342 planitia 0.246 319 0.177 lunae 0.176 maja 0.170 maumee 0.146 vedra 0.146 viking 0.137 kasei 0.124 outflow 0.107 palus 0.102 tharsis 0.102 elevation 0.101 basin 0.096 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 28°24′N 319°42′E / 28.4°N 319.7°E . [1] Chryse Planitia lies partially in the Lunae Palus quadrangle , partially in the Oxia Palus quadrangle , partially in the Mare Acidalium quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2017 |
44089 characters 3 sections 9 paragraphs 11 images 179 internal links 10 external links |
chryse 0.646 valles 0.342 planitia 0.246 319 0.177 lunae 0.176 maja 0.170 maumee 0.146 vedra 0.146 viking 0.137 kasei 0.124 outflow 0.107 palus 0.102 tharsis 0.102 elevation 0.101 basin 0.096 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 28°24′N 319°42′E / 28.4°N 319.7°E . [1] Chryse Planitia lies partially in the Lunae Palus quadrangle , partially in the Oxia Palus quadrangle , partially in the Mare Acidalium quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2016 |
41152 characters 3 sections 8 paragraphs 10 images 177 internal links 9 external links |
chryse 0.664 valles 0.301 planitia 0.243 319 0.192 lunae 0.191 maja 0.138 kasei 0.135 viking 0.124 outflow 0.116 palus 0.111 tharsis 0.110 maumee 0.105 vedra 0.105 basin 0.104 ares 0.103 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 28°24′N 319°42′E / 28.4°N 319.7°E . [1] Chryse Planitia lies partially in the Lunae Palus quadrangle , partially in the Oxia Palus quadrangle , partially in the Mare Acidalium quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2015 |
41000 characters 3 sections 8 paragraphs 10 images 176 internal links 9 external links |
chryse 0.663 valles 0.301 planitia 0.242 319 0.192 lunae 0.191 maja 0.138 kasei 0.135 viking 0.124 outflow 0.116 palus 0.111 tharsis 0.110 maumee 0.105 vedra 0.105 basin 0.104 ares 0.103 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 28°24′N 319°42′E / 28.4°N 319.7°E . [1] Chryse Planitia lies partially in the Lunae Palus quadrangle , partially in the Oxia Palus quadrangle , partially in the Mare Acidalium quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2014 |
34733 characters 3 sections 7 paragraphs 8 images 167 internal links 3 external links |
chryse 0.660 valles 0.317 planitia 0.230 lunae 0.201 maja 0.145 kasei 0.142 320 0.131 viking 0.130 outflow 0.122 palus 0.117 tharsis 0.116 maumee 0.111 vedra 0.111 basin 0.110 ares 0.108 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2013 |
34824 characters 3 sections 7 paragraphs 9 images 168 internal links 3 external links |
chryse 0.669 planitia 0.233 vallis 0.211 lunae 0.204 valles 0.198 maja 0.147 kasei 0.144 320 0.133 viking 0.132 outflow 0.124 palus 0.118 tharsis 0.118 maumee 0.112 vedra 0.112 basin 0.111 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2012 |
13455 characters 3 sections 7 paragraphs 5 images 31 internal links 3 external links |
chryse 0.672 planitia 0.234 vallis 0.212 lunae 0.205 valles 0.199 maja 0.148 kasei 0.144 320 0.133 viking 0.133 outflow 0.124 palus 0.119 tharsis 0.118 maumee 0.113 vedra 0.113 basin 0.112 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 to 2,000 metres (330 to 6,560 ft) range is close to half the average for lunar maria. |
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| 2011 |
13356 characters 3 sections 7 paragraphs 5 images 31 internal links 3 external links |
chryse 0.674 planitia 0.235 vallis 0.213 lunae 0.205 valles 0.199 maja 0.148 kasei 0.145 320 0.134 viking 0.133 outflow 0.125 palus 0.119 tharsis 0.119 maumee 0.113 vedra 0.113 basin 0.112 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2010 |
13356 characters 3 sections 7 paragraphs 5 images 31 internal links 3 external links |
chryse 0.674 planitia 0.235 vallis 0.213 lunae 0.205 valles 0.199 maja 0.148 kasei 0.145 320 0.134 viking 0.133 outflow 0.125 palus 0.119 tharsis 0.119 maumee 0.113 vedra 0.113 basin 0.112 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2009 |
13219 characters 3 sections 7 paragraphs 5 images 31 internal links 3 external links |
chryse 0.674 planitia 0.235 vallis 0.213 lunae 0.205 valles 0.199 maja 0.148 kasei 0.145 320 0.134 viking 0.133 outflow 0.125 palus 0.119 tharsis 0.119 maumee 0.113 vedra 0.113 basin 0.112 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . Chryse Planitia lies partially in the Lunae Palus quadrangle and partially in the Oxia Palus quadrangle . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2008 |
6360 characters 2 sections 3 paragraphs 1 images 19 internal links 3 external links |
chryse 0.570 320 0.274 outflow 0.256 basin 0.230 maria 0.214 channels 0.177 planitia 0.161 26 0.136 emptying 0.136 tharsis 0.122 plain 0.121 opens 0.121 lunar 0.110 golden 0.109 shoreline 0.109 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2007 |
5978 characters 2 sections 3 paragraphs 1 images 15 internal links 3 external links |
chryse 0.570 320 0.274 outflow 0.256 basin 0.230 maria 0.214 channels 0.177 planitia 0.161 26 0.136 emptying 0.136 tharsis 0.122 plain 0.121 opens 0.121 lunar 0.110 golden 0.109 shoreline 0.109 |
Chryse Planitia (Greek, " Golden Plain ") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region, centered at 26°42′N 320°00′E / 26.7°N 320.0°E . It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2006 |
4513 characters 2 sections 3 paragraphs 1 images 15 internal links 2 external links |
chryse 0.613 outflow 0.275 basin 0.248 maria 0.230 channels 0.190 planitia 0.173 emptying 0.146 tharsis 0.131 opens 0.130 lunar 0.118 shoreline 0.117 ocean 0.113 wrinkle 0.112 landed 0.112 flanks 0.105 |
Chryse Planitia is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region. It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100 m to 2000 m range is close to half the average for lunar maria. |
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| 2005 |
3738 characters 1 sections 3 paragraphs 1 images 13 internal links 1 external links |
chryse 0.608 outflow 0.273 basin 0.246 maria 0.228 channels 0.188 planitia 0.171 100m 0.151 emptying 0.145 tharsis 0.130 opens 0.129 lunar 0.117 shoreline 0.116 ocean 0.112 wrinkle 0.111 landed 0.111 |
Chryse Planitia is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region. It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100m to 2000m range is close to half the average for lunar maria. |
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| 2004 |
3236 characters 1 sections 3 paragraphs 0 images 12 internal links 1 external links |
chryse 0.608 outflow 0.273 basin 0.246 maria 0.228 channels 0.188 planitia 0.171 100m 0.151 emptying 0.145 tharsis 0.130 opens 0.129 lunar 0.117 shoreline 0.116 ocean 0.112 wrinkle 0.111 landed 0.111 |
Chryse Planitia is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region. It is 1600 km in diameter and with a floor 2.5 km below the average planetary surface altitude, and is thought to be an ancient impact basin ; it has has several features in common with lunar maria , such as wrinkle ridges . The density of impact craters in the 100m to 2000m range is close to half the average for lunar maria. |