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Scientists find 'best evidence' yet for liquid water now on Mars

NASA's ongoing quest to 'follow the water,' in hopes of finding hints of life on Mars, has uncovered seasonally-appearing dark streaks that researchers call 'the best evidence we have to date of liquid water occurring today' – that is, not in the ancient past – 'on Mars.'

Image

This image, which combines orbital imagery with 3-D modeling, shows an oblique view of streaks, or 'flows,' that appear in spring and summer on a steep slope inside Mars' Newton Crater. The seasonal changes at this site and a few others with similar flows might be evidence of salty liquid water active on Mars today. Repeat imaging by HiRISE shows the features appear and incrementally grow during warm seasons and fade in cold seasons.

Univ. of Arizona / JPL-Caltech / NASA

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Liquid water – a necessary ingredient for organic life – may finally have revealed its presence on today's Mars.

Images unveiled today from NASA's Mars Reconnaissance Orbiter have revealed dark, narrow streaks that appear and slowly snake down walls of craters that populate the planet's southern hemisphere. The process occurs from late spring to early fall. The streaks vanish with the return of late fall and winter, only to reappear the following spring.

The streaks originate at rock outcroppings high on steep crater walls, but only on walls facing in the general direction of the equator, which receive more sunlight than poleward-facing slopes.

The features are too narrow to be formed by silt sliding downhill, which has been seen elsewhere on the planet, according to the team of scientists formally reporting the observations in the Aug. 5 issue of the journal Science. Moreover, these streaks are far more rare than the silt slides, suggesting a far less common process at work.

Sudden thaws of carbon-dioxide frost probably triggered those other, silty slides, scientists have theorized. These newly-discovered features, by contrast, appear – and grow – when surface temperatures are too warm for carbon-dioxide frost to exist. Those temperatures range from about 9 degrees below zero Fahrenheit to as high as 80 degrees F during a summer's mid-afternoon. Nine degrees below zero may be too warm for CO2 frost, but not for liquid water heavily laced with salts, says Alfred McEwen, a planetary scientist at the University of Arizona at Tucson and leader of the team reporting the results.

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