NASA’s Mars Reconnaissance Orbiter has revealed Martian rocks containing a hydrated mineral similar to opal described as a new category of minerals spread across large regions of Mars. This discovery suggests that liquid water remained on the planet’s surface a billion years later than scientists believed, and it played an important role in shaping the planet’s surface and possibly hosting life. The rocks are light-toned and appear cream-colored in this false-color image taken by the High Resolution Imaging Science Experiment camera on the right.
Image Credit: NASA/JPL-Caltech/Univ. of Arizona
Images acquired by the orbiter reveal that different layers of rock have different properties and chemistry. The opal minerals are located in distinct beds of rock outside of the large Valles Marineris canyon system and are also found in rocks within the canyon. The presence of opal in these relatively young rocks tells scientists that water, possibly as rivers and small ponds, interacted with the surface as recently as two billion years ago, one billion years later than scientists had expected. The discovery of this new category of minerals spread across large regions of Mars suggests that liquid water played an important role in shaping the planet’s surface and possibly hosting life.
Researchers examining data from the orbiter’s Compact Reconnaissance Imaging Spectrometer for Mars have found evidence of hydrated silica, commonly known as opal. The hydrated, or water-containing, mineral deposits are telltale signs of where and when water was present on ancient Mars. “This is an exciting discovery because it extends the time range for liquid water on Mars, and the places where it might have supported life,” said Scott Murchie, the spectrometer’s principal investigator at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. “The identification of opaline silica tells us that water may have existed as recently as 2 billion years ago.”
Until now, only two major groups of hydrated minerals, phyllosilicates and hydrated sulfates, had been observed by spacecraft orbiting Mars. Clay-like phyllosilicates formed more than 3.5 billion years ago where igneous rock came into long-term contact with water. During the next several hundred million years, until approximately 3 billion years ago, hydrated sulfates formed from the evaporation of salty and sometimes acidic water.
The newly discovered opaline silicates are the youngest of the three types of hydrated minerals. They formed where liquid water altered materials created by volcanic activity or meteorite impact on the Martian surface. One such location noted by scientists is the large Martian canyon system called Valles Marineris. “We see numerous outcrops of opal-like minerals, commonly in thin layers extending for very long distances around the rim of Valles Marineris and sometimes within the canyon system itself,” said Ralph Milliken of NASA’s Jet Propulsion Laboratory in Pasadena, Calif.
