
"Measuring water isotopes (water variants with different molecular masses) is a crucial element of understanding how Mars as a planet has lost its water over time, and therefore how the habitability of Mars has changed throughout its history," said Manish Patel, a planetary scientist at the Open University in the U.K. and the co-principal investigator of NOMAD.
The presence of dried ancient valleys on the planet suggests that water once flowed on the surface of Mars. But much of Martian water is now locked up on the polar caps and underground. (Related: Geological curiosity: Mars "blueberries" reveal what ancient Mars may have looked like.)
The finding could also provide clues to some of the greatest mysteries of the Red Planet, including whether it is still geologically active. As the researchers wrote in a paper, which was published on Feb. 10 in the journal Science Advances, hydrogen chloride has been suggested as an indicator of active magmatic processes.
'This research is a key component in our quest to unearth the mysteries of the Red Planet," said Sue Horne, head of space exploration at the U.K. Space Agency.
Ultimately, the study might help answer the question of habitability. "Understanding water vapor on Mars would help answer the all-important question, was there life on Mars?" Horne said.
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