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Silica on Mars volcano tells of wet and cozy past

Such environments may have provided habitats for microbes analogous to some of Earth's earliest life-forms.

martian-volcano
This volcanic cone in the Nili Patera caldera on Mars has hydrothermal mineral deposits on the southern flanks and nearby terrains. Light-toned patches on the closest flank of the cone, and the entire field of light-toned material on the left of the cone are hydrothermal deposits. The cone is about 5 kilometers (3 miles) in diameter at the base.
NASA/JPL-Caltech/MSSS/JHU-APL/Brown Univ.
Light-colored mounds of a mineral deposited on a volcanic cone more than 3 billion years ago may preserve evidence of one of the most recent habitable microenvironments on Mars.

Observations by NASA's Mars Reconnaissance Orbiter enabled researchers to identify the mineral as hydrated silica and to see its volcanic context. The mounds' compositions and their location on the flanks of a volcanic cone provide the best evidence yet found on Mars for an intact deposit from a hydrothermal environment — a steam fumarole, or hot spring. Such environments may have provided habitats for some of Earth's earliest life- forms.

"The heat and water required to create this deposit probably made this a habitable zone," said J.R. Skok from Brown University in Providence, Rhode Island. "If life did exist there, this would be a promising type of deposit to entomb evidence of it — a microbial mortuary."

No studies have yet determined whether Mars has ever supported life. The new results add to accumulating evidence that, at some times and in some places, Mars has had favorable environments for microbial life. This specific place would have been habitable when most of Mars was already dry and cold. Concentrations of hydrated silica have been identified on Mars previously, including a nearly pure patch found by NASA's Mars Exploration Rover Spirit in 2007. However, none of those earlier findings was in such an intact setting as this one, and the setting adds evidence about the origin.

"You have spectacular context for this deposit,” Skok said. “It's right on the flank of a volcano. The setting remains essentially the same as it was when the silica was deposited."

The small cone rises about 100 yards (100 meters) from the floor of a shallow bowl named Nili Patera. The patera, which is the floor of a volcanic caldera, spans about 30 miles (50 kilometers) in the Syrtis Major volcanic region of equatorial Mars. Before the cone formed, free-flowing lava blanketed nearby plains. The collapse of an underground magma chamber from which lava had emanated created the bowl. Subsequent lava flows, still with a runny texture, coated the floor of Nili Patera. The cone grew from even later flows, apparently after evolution of the underground magma had thickened its texture so that the erupted lava would mound up.

"We can read a series of chapters in this history book and know that the cone grew from the last gasp of a giant volcanic system," said John Mustard from Brown University. "The cooling and solidification of most of the magma concentrated its silica and water content."

Observations by cameras on the Mars Reconnaissance Orbiter revealed patches of bright deposits near the summit of the cone, fanning down its flank, and on flatter ground in the vicinity. The Brown researchers partnered with Scott Murchie of Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, to analyze the bright exposures with the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument on the orbiter.

Silica can be dissolved, transported, and concentrated by hot water or steam. Hydrated silica identified by the spectrometer in uphill locations, confirmed by stereo imaging, indicates that hot springs fed by underground heating created these deposits. Silica deposits around hydrothermal vents in Iceland are among the best parallels on Earth.

“The habitable zone would have been within and alongside the conduits carrying the heated water,” Murchie said. The volcanic activity that built the cone in Nili Patera appears to have happened more recently than the 3.7-billion-year or greater age of Mars' potentially habitable early wet environments recorded in clay minerals identified from orbit.

Light-colored mounds of a mineral deposited on a volcanic cone more than 3 billion years ago may preserve evidence of one of the most recent habitable microenvironments on Mars.

Observations by NASA's Mars Reconnaissance Orbiter enabled researchers to identify the mineral as hydrated silica and to see its volcanic context. The mounds' compositions and their location on the flanks of a volcanic cone provide the best evidence yet found on Mars for an intact deposit from a hydrothermal environment — a steam fumarole, or hot spring. Such environments may have provided habitats for some of Earth's earliest life- forms.

"The heat and water required to create this deposit probably made this a habitable zone," said J.R. Skok from Brown University in Providence, Rhode Island. "If life did exist there, this would be a promising type of deposit to entomb evidence of it — a microbial mortuary."

No studies have yet determined whether Mars has ever supported life. The new results add to accumulating evidence that, at some times and in some places, Mars has had favorable environments for microbial life. This specific place would have been habitable when most of Mars was already dry and cold. Concentrations of hydrated silica have been identified on Mars previously, including a nearly pure patch found by NASA's Mars Exploration Rover Spirit in 2007. However, none of those earlier findings was in such an intact setting as this one, and the setting adds evidence about the origin.

"You have spectacular context for this deposit,” Skok said. “It's right on the flank of a volcano. The setting remains essentially the same as it was when the silica was deposited."

The small cone rises about 100 yards (100 meters) from the floor of a shallow bowl named Nili Patera. The patera, which is the floor of a volcanic caldera, spans about 30 miles (50 kilometers) in the Syrtis Major volcanic region of equatorial Mars. Before the cone formed, free-flowing lava blanketed nearby plains. The collapse of an underground magma chamber from which lava had emanated created the bowl. Subsequent lava flows, still with a runny texture, coated the floor of Nili Patera. The cone grew from even later flows, apparently after evolution of the underground magma had thickened its texture so that the erupted lava would mound up.

"We can read a series of chapters in this history book and know that the cone grew from the last gasp of a giant volcanic system," said John Mustard from Brown University. "The cooling and solidification of most of the magma concentrated its silica and water content."

Observations by cameras on the Mars Reconnaissance Orbiter revealed patches of bright deposits near the summit of the cone, fanning down its flank, and on flatter ground in the vicinity. The Brown researchers partnered with Scott Murchie of Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, to analyze the bright exposures with the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument on the orbiter.

Silica can be dissolved, transported, and concentrated by hot water or steam. Hydrated silica identified by the spectrometer in uphill locations, confirmed by stereo imaging, indicates that hot springs fed by underground heating created these deposits. Silica deposits around hydrothermal vents in Iceland are among the best parallels on Earth.

“The habitable zone would have been within and alongside the conduits carrying the heated water,” Murchie said. The volcanic activity that built the cone in Nili Patera appears to have happened more recently than the 3.7-billion-year or greater age of Mars' potentially habitable early wet environments recorded in clay minerals identified from orbit.

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