Why did Mars dry out?
Why did Mars dry out?
Years ago, astronomers detected signs of Mars' watery past. Early evidence came from imaging large numbers of winding channels on the Red Planet. These images suggest
abundant liquids of some type flowed on the planet at some point in its history. In 1972, the Mariner 9 spacecraft orbited Mars and took photos of what appear to be dry riverbeds scattered over the planet's surface.
More recently, Tim Parker of the California Institute ofTechnology suggested many dry lakebeds also exist on Mars — although this interpretation is not as clear as that of the riverbeds. Parker also interpreted some features as ancient shorelines, and even some as basins once filled by lakes. Many of the features Parker interCOLD
AND DRV A mosaic highlighting Mars' Valles Marineris, the solar system's largest canyon, comprises 102 Viking orbiter images. Three Tharsis-area volcanoes are visible in the picture (arrows). In this volcanic region and others, clear evidence of liquid water on the martian surface appears, nasa/jplajsgs
preted and some of the river channels are scarred by craters, suggesting the Red Planet's watery past had concluded by about 3.5 billion years ago.
The clear implication is that Mars had a watery past and, for some reason, dried out, but not completely. Using images from the Mars Global Surveyor satellite, planetary scientists Devon Burr, Alfred McEwen, and colleagues looked carefully at Marte Vallis, a river channel that extends from Elysium Pla- nitia into Amazonis Planitia.
Freshly sculpted features and a lack of craters indicate this river system harbored water in the last 40 million years. Astronomers believe a significant amount of water lies locked inside underground martian aquifers. Future explorers will drill into the planet's mantle to explore the nature of this watery deposit.
In 2000, Mars Global Surveyor scientists Ken Edgett and Michael Maiin explored another feature that suggests a water-laden past for Mars. Edgett and Maiin identified numerous "gullies" extending from rocky outcrop highlands to lower portions of hills. They appear to be analogs to features in Canada, Iceland, and Greenland, where gullies form when
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DRY GULLIES. These gullies in Mars'
Terra Sirenum region suggest liquids once flowed on the Red Planet.
water saturates the ground and then flows downward. If these martian features were formed by water, the implication is rather amazing in that large flows of water must have happened recently — and maybe even still go on today.The mysterious source of such flowing water might be ice that suddenly melts. The flows would have to be significant to leave surface features because the temperatures and pressures on Mars' surface today mean water quickly evaporates once it reaches the surface.
So if Mars was wet and, therefore, also relatively warm in the past, why did it dry out? Planetary scientists don't yet know, but data from the Mars Exploration Rovers and Mars Express suggest a substantial climate change occurred some 600 million years after the planet's formation. One study released in 2006 by French astrophysicist Jean-Pierre Bibring suggests volcanic eruptions drove Mars'changing climate. By studying the mineralogy of gypsum and hematite on the martian surface, Bibring and his colleagues found evidence of a heavy period of volcanism.
If life did gain a toehold on Mars by this point, the climatic change may have shifted the planet to a less hospitable place. Moreover, Mars cooled following this period of volcanism. During the cooling, astronomers believe Mars' magnetic field dissipated because the planet's molten iron core solidified. When the Red Planet's protective shield no longer sheltered living creatures, the solar wind may have stripped away much of the martian atmosphere and sent much of the planet's water into space. After a rather earthlike start, Mars may have — on a planetary timescale — suddenly turned cold, dry, and hostile to living things. S3
Years ago, astronomers detected signs of Mars' watery past. Early evidence came from imaging large numbers of winding channels on the Red Planet. These images suggest
abundant liquids of some type flowed on the planet at some point in its history. In 1972, the Mariner 9 spacecraft orbited Mars and took photos of what appear to be dry riverbeds scattered over the planet's surface.
More recently, Tim Parker of the California Institute ofTechnology suggested many dry lakebeds also exist on Mars — although this interpretation is not as clear as that of the riverbeds. Parker also interpreted some features as ancient shorelines, and even some as basins once filled by lakes. Many of the features Parker interCOLD
AND DRV A mosaic highlighting Mars' Valles Marineris, the solar system's largest canyon, comprises 102 Viking orbiter images. Three Tharsis-area volcanoes are visible in the picture (arrows). In this volcanic region and others, clear evidence of liquid water on the martian surface appears, nasa/jplajsgs
preted and some of the river channels are scarred by craters, suggesting the Red Planet's watery past had concluded by about 3.5 billion years ago.
The clear implication is that Mars had a watery past and, for some reason, dried out, but not completely. Using images from the Mars Global Surveyor satellite, planetary scientists Devon Burr, Alfred McEwen, and colleagues looked carefully at Marte Vallis, a river channel that extends from Elysium Pla- nitia into Amazonis Planitia.
Freshly sculpted features and a lack of craters indicate this river system harbored water in the last 40 million years. Astronomers believe a significant amount of water lies locked inside underground martian aquifers. Future explorers will drill into the planet's mantle to explore the nature of this watery deposit.
In 2000, Mars Global Surveyor scientists Ken Edgett and Michael Maiin explored another feature that suggests a water-laden past for Mars. Edgett and Maiin identified numerous "gullies" extending from rocky outcrop highlands to lower portions of hills. They appear to be analogs to features in Canada, Iceland, and Greenland, where gullies form when
{W'J? jjf '
& f [, WJt'f 'J
DRY GULLIES. These gullies in Mars'
Terra Sirenum region suggest liquids once flowed on the Red Planet.
water saturates the ground and then flows downward. If these martian features were formed by water, the implication is rather amazing in that large flows of water must have happened recently — and maybe even still go on today.The mysterious source of such flowing water might be ice that suddenly melts. The flows would have to be significant to leave surface features because the temperatures and pressures on Mars' surface today mean water quickly evaporates once it reaches the surface.
So if Mars was wet and, therefore, also relatively warm in the past, why did it dry out? Planetary scientists don't yet know, but data from the Mars Exploration Rovers and Mars Express suggest a substantial climate change occurred some 600 million years after the planet's formation. One study released in 2006 by French astrophysicist Jean-Pierre Bibring suggests volcanic eruptions drove Mars'changing climate. By studying the mineralogy of gypsum and hematite on the martian surface, Bibring and his colleagues found evidence of a heavy period of volcanism.
If life did gain a toehold on Mars by this point, the climatic change may have shifted the planet to a less hospitable place. Moreover, Mars cooled following this period of volcanism. During the cooling, astronomers believe Mars' magnetic field dissipated because the planet's molten iron core solidified. When the Red Planet's protective shield no longer sheltered living creatures, the solar wind may have stripped away much of the martian atmosphere and sent much of the planet's water into space. After a rather earthlike start, Mars may have — on a planetary timescale — suddenly turned cold, dry, and hostile to living things. S3
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