© 2019 - All Rights Reserved
“This is important for deducing how much water could have been on Mars, and whether the water was from Mars itself rather than comets or meteorites,” said Martin Kunz, a staff scientist at Berkeley Lab’s ALS who participated in X-ray studies of the shocked whitlockite samples.
“If even a part of merrillite had been whitlockite before, it changes the water budget of Mars dramatically,” said Oliver Tschauner, a professor of research in the Department of Geoscience at UNLV who co-led the study with Christopher Adcock, an assistant research professor at UNLV.
“The overarching question here is about water on Mars and its early history on Mars: Had there ever been an environment that enabled a generation of life on Mars?” Tschauner said.
“The only missing link now is to prove that (merrillite) had, in fact, really been Martian whitlockite before,” Tschauner said. “We have to go back to the real meteorites and see if there had been traces of water.”
“Most of them are very similar in the rock composition as well as the minerals that are occurring, and have a similar impact age,” he said. Mars is likely to have formed about 4.6 billion years ago, about the same time as Earth and the rest of our solar system.
“It’s really important to get a rock that hasn’t been ‘kicked'” like the Martian meteorites have, said Kunz, in order to learn more about the planet’s water history.