The atmosphere of the planet Mars is composed mostly of carbon dioxide . The atmospheric pressure on the Martian surface averages 600 pascals (0.087 psi ; 6.0 mbar ), about 0.6% of Earth's mean sea level pressure of 101.3 kilopascals (14.69 psi; 1.013 bar). It ranges from a low of 30 pascals (0.0044 psi; 0.30 mbar) on Olympus Mons 's peak to over 1,155 pascals (0.1675 psi; 11.55 mbar) in the depths of Hellas Planitia . This pressure is well below the Armstrong limit for the unprotected human body. Mars 's atmospheric mass of 25 teratonnes compares to Earth's 5148 teratonnes ; Mars has a scale height of 11.1 kilometres (6.9 mi) [2] versus Earth's 8.5 kilometres (5.3 mi). [3]
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
280077 characters 19 sections 41 paragraphs 31 images 368 internal links 190 external links |
2. Observations and measurement from Earth |
methane 0.532 atmosphere 0.285 dioxide 0.191 carbon 0.165 atmospheric 0.146 ozone 0.131 ppb 0.124 reported 0.105 argon 0.104 ppbv 0.098 psi 0.097 destruction 0.094 co2 0.088 oxygen 0.085 nasa 0.081 |
The atmosphere of the planet Mars is composed mostly of carbon dioxide . The atmospheric pressure on the Martian surface averages 600 pascals (0.087 psi ; 6.0 mbar ), about 0.6% of Earth's mean sea level pressure of 101.3 kilopascals (14.69 psi; 1.013 bar). It ranges from a low of 30 pascals (0.0044 psi; 0.30 mbar) on Olympus Mons 's peak to over 1,155 pascals (0.1675 psi; 11.55 mbar) in the depths of Hellas Planitia . This pressure is well below the Armstrong limit for the unprotected human body. Mars 's atmospheric mass of 25 teratonnes compares to Earth's 5148 teratonnes ; Mars has a scale height of 11.1 kilometres (6.9 mi) [2] versus Earth's 8.5 kilometres (5.3 mi). [3] |
2017 |
239216 characters 18 sections 38 paragraphs 28 images 355 internal links 160 external links |
2. Observations and measurement from Earth |
methane 0.518 atmosphere 0.298 dioxide 0.203 carbon 0.176 ozone 0.139 ppb 0.132 atmospheric 0.131 argon 0.111 ppbv 0.104 psi 0.103 destruction 0.099 reported 0.095 co2 0.094 oxygen 0.091 sulfur 0.083 |
The atmosphere of Mars is the layer of gases surrounding Mars . It is composed mostly of carbon dioxide . The atmospheric pressure on the Martian surface averages 600 pascals (0.087 psi ; 6.0 mbar ), about 0.6% of Earth's mean sea level pressure of 101.3 kilopascals (14.69 psi; 1.013 bar). It ranges from a low of 30 pascals (0.0044 psi; 0.30 mbar) on Olympus Mons 's peak to over 1,155 pascals (0.1675 psi; 11.55 mbar) in the depths of Hellas Planitia . This pressure is well below the Armstrong limit for the unprotected human body. Mars's atmospheric mass of 25 teratonnes compares to Earth's 5148 teratonnes with a scale height of about 11 kilometres (6.8 mi) versus Earth's 7 kilometres (4.3 mi). |
2016 |
227475 characters 17 sections 34 paragraphs 28 images 345 internal links 143 external links |
2. Observations and measurement from Earth |
methane 0.519 atmosphere 0.295 dioxide 0.208 carbon 0.181 ozone 0.143 ppb 0.135 atmospheric 0.134 argon 0.114 ppbv 0.107 psi 0.106 destruction 0.102 co2 0.096 reported 0.089 sulfur 0.085 pole 0.084 |
The atmosphere of Mars is the layer of gases surrounding Mars . It is composed mostly of carbon dioxide . The atmospheric pressure on the Martian surface averages 600 pascals (0.087 psi ; 6.0 mbar ), about 0.6% of Earth's mean sea level pressure of 101.3 kilopascals (14.69 psi; 1.013 bar). It ranges from a low of 30 pascals (0.0044 psi; 0.30 mbar) on Olympus Mons 's peak to over 1,155 pascals (0.1675 psi; 11.55 mbar) in the depths of Hellas Planitia . This pressure is well below the Armstrong limit for the unprotected human body. Mars's atmospheric mass of 25 teratonnes compares to Earth's 5148 teratonnes with a scale height of about 11 kilometres (6.8 mi) versus Earth's 7 kilometres (4.3 mi). |
2015 |
208292 characters 16 sections 32 paragraphs 26 images 314 internal links 131 external links |
2. Observations and measurement from Earth |
methane 0.521 atmosphere 0.296 dioxide 0.209 carbon 0.181 ozone 0.144 ppb 0.136 atmospheric 0.135 argon 0.114 ppbv 0.108 psi 0.106 destruction 0.102 co2 0.097 reported 0.089 sulfur 0.085 pole 0.084 |
The atmosphere of Mars is the layer of gases surrounding Mars composed mostly of carbon dioxide . The atmospheric pressure on the Martian surface averages 600 pascals (0.087 psi ), about 0.6% of Earth's mean sea level pressure of 101.3 kilopascals (14.69 psi). It ranges from a low of 30 pascals (0.0044 psi) on Olympus Mons 's peak to over 1,155 pascals (0.1675 psi) in the depths of Hellas Planitia . This pressure is well below the Armstrong limit for the unprotected human body. Mars's atmospheric mass of 25 teratonnes compares to Earth's 5148 teratonnes with a scale height of about 11 kilometres (6.8 mi) versus Earth's 7 kilometres (4.3 mi). |
2014 |
179391 characters 16 sections 32 paragraphs 23 images 308 internal links 109 external links |
2. Observations and measurement from Earth |
methane 0.599 atmosphere 0.242 dioxide 0.159 ppbv 0.159 ozone 0.141 ppb 0.134 psi 0.125 atmospheric 0.124 carbon 0.114 argon 0.112 ethane 0.104 destruction 0.101 co2 0.095 sulfur 0.084 curiosity 0.083 |
The atmosphere of Mars is, like that of Venus , composed mostly of carbon dioxide though far thinner. There has been renewed interest in its composition since the detection of traces of methane in 2003 [2] [3] that may indicate life but may also be produced by a geochemical process, volcanic or hydrothermal activity . [4] |
2013 |
156935 characters 16 sections 29 paragraphs 19 images 305 internal links 89 external links |
3. Observations and measurement from Earth |
methane 0.587 atmosphere 0.239 dioxide 0.182 ozone 0.162 psi 0.143 atmospheric 0.133 carbon 0.130 argon 0.128 destruction 0.115 sulfur 0.096 ethane 0.095 co2 0.093 pole 0.083 gases 0.082 teratonnes 0.078 |
The atmosphere of Mars is, like that of Venus , composed mostly of carbon dioxide though far thinner. There has been renewed interest in its composition since the detection of traces of methane [2] [3] that may indicate life but may also be produced by a geochemical process, volcanic or hydrothermal activity . [4] |
2012 |
153240 characters 14 sections 23 paragraphs 18 images 296 internal links 92 external links |
3. Observations and measurement from Earth |
methane 0.657 atmosphere 0.215 psi 0.153 dioxide 0.137 carbon 0.129 destruction 0.123 argon 0.114 ethane 0.102 atmospheric 0.101 co2 0.100 teratonnes 0.084 pascals 0.083 h2 0.079 martian 0.076 source 0.076 |
The atmosphere of Mars is, like that of Venus , composed mostly of carbon dioxide though far thinner. There has been renewed interest in its composition since the detection of traces of methane [2] [3] that may indicate life but may also be produced by a geochemical process, volcanic or hydrothermal activity . [4] |
2011 |
120531 characters 12 sections 21 paragraphs 15 images 274 internal links 60 external links |
methane 0.655 atmosphere 0.206 dioxide 0.150 psi 0.140 destruction 0.135 carbon 0.130 argon 0.125 ethane 0.112 co2 0.109 atmospheric 0.100 mol 0.100 teratonnes 0.092 pascals 0.091 martian 0.083 source 0.083 |
The atmosphere of Mars is relatively thin and is composed mostly of carbon dioxide (95.32%). There has been interest in studying its composition since the detection of trace amounts of methane , [1] [2] which may indicate the presence of life on Mars , but may also be produced by a geochemical process, volcanic or hydrothermal activity . [3] |
|
2010 |
102419 characters 10 sections 19 paragraphs 7 images 263 internal links 46 external links |
methane 0.640 atmosphere 0.210 carbon 0.149 psi 0.148 dioxide 0.146 destruction 0.143 argon 0.132 biogenic 0.126 ethane 0.118 atmospheric 0.106 teratonnes 0.097 co2 0.096 pascals 0.096 sources 0.093 water 0.092 |
Mars , the 4th planet from the Sun , has a very different atmosphere from that of the Earth . There has been much interest [1] in studying its composition since the recent detection of trace amounts of methane , [2] which may indicate the presence of life on Mars ; its presence could also be caused by a geochemical process, or it could be the result of volcanic or hydrothermal activity . [3] |
|
2009 |
99452 characters 11 sections 20 paragraphs 7 images 264 internal links 44 external links |
methane 0.617 atmosphere 0.220 carbon 0.157 dioxide 0.153 destruction 0.150 argon 0.139 biogenic 0.132 kpa 0.126 ethane 0.124 atmospheric 0.111 teratonnes 0.102 sources 0.097 martian 0.092 pa 0.090 lifetime 0.087 |
Mars , the 4th planet from the Sun , has a very different atmosphere from that of the Earth . There has been much interest [1] in studying its composition since the recent detection of a small amount of methane , [2] which may signal life on Mars ; it could also be a geochemical process or the result of volcanic or hydrothermal activity . [3] |
|
2008 |
68566 characters 10 sections 13 paragraphs 6 images 260 internal links 22 external links |
methane 0.483 atmosphere 0.286 dioxide 0.214 argon 0.195 carbon 0.186 kpa 0.176 teratonnes 0.142 co2 0.142 pa 0.127 atmospheric 0.103 poles 0.097 martian 0.089 uniformly 0.086 prove 0.081 biological 0.081 |
Mars , the fourth planet from the Sun , has a very different atmosphere from that of Earth . There has been much interest [1] [2] in studying its composition since the recent detection of a small amount of methane , [3] which may signal life on Mars ; it could also be a geochemical process or the result of volcanic or hydrothermal activity . [4] |
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2007 |
41462 characters 9 sections 16 paragraphs 3 images 107 internal links 17 external links |
methane 0.426 atmosphere 0.347 argon 0.245 dioxide 0.224 carbon 0.194 kpa 0.185 pa 0.133 template 0.126 condense 0.122 gasses 0.115 atmospheric 0.108 uniformly 0.090 vapour 0.086 prove 0.085 biological 0.085 |
Mars , the fourth planet from the Sun , has a very different atmosphere from that of Earth . There has been much interest [1] [2] in studying its composition since the recent detection of a small amount of methane , [3] which may signal life on Mars . |
|
2006 |
15372 characters 6 sections 6 paragraphs 1 images 54 internal links 7 external links |
methane 0.333 kpa 0.330 pa 0.237 atmosphere 0.235 accompanied 0.141 poles 0.137 tawny 0.133 1155 0.113 dioxide 0.109 co2 0.106 pressure 0.104 unproven 0.103 clouds 0.103 thin 0.102 temperature 0.101 |
Mars , the fourth planet from the Sun , has a very different atmosphere from that of Earth . There has been a lot of interest in studying its composition since the recent detection of a small amount of methane , which may signal life on Mars . |