NASA orbiter reveals details of a wetter Mars
A new category of minerals suggests liquid water remained on planet's surface longer than once thought.
Provided by NASA Headquarters, Washington, D.C.
October 28, 2008
NASA's Mars Reconnaissance Orbiter observed a new category of minerals spread across large regions of Mars. This discovery suggests liquid water remained on the planet's surface a billion years later than scientists believed. This liquid water may have 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," Scott Murchie said, 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, spacecraft orbiting Mars had observed only two major groups of hydrated minerals, phyllosilicates and hydrated sulfates. 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 is the large martian canyon system 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, California.
Milliken is lead author of an article that describes the identification of opaline silica. The article appears in the November 2008 issue of Geology. The study reveals that the minerals, which NASA's Mars rover Spirit recently found in Gusev Crater, are widespread and occur in relatively young terrains.
In some locations, the orbiter's spectrometer observed opaline silica with iron sulfate minerals, either in or around dry river channels. This pressure indicates the acidic water remained on the martian surface for an extended period of time. Milliken and his colleagues believe that low-temperature acidic water was involved in forming the opal in these areas. In areas where there is no evidence that the water was acidic, deposits may have formed under a wide range of conditions.
"What's important is that the longer liquid water existed on Mars, the longer the window during which Mars may have supported life," Milliken said. "The opaline silica deposits would be good places to explore to assess the potential for habitability on Mars, especially in these younger terrains."
The spectrometer collects 544 colors, or wavelengths, of reflected sunlight to detect minerals on the surface of Mars. Its highest resolution is about 20 times sharper than any previous look at the planet in near-infrared wavelengths.