Clues to where water on Mars must have vanished emerge

Where did the rest of the water go? Some of it disappeared into space. Water molecules, pummelled by particles of solar wind, broke apart into hydrogen and oxygen atoms, and those, especially the lighter hydrogen atoms, sped out of the atmosphere, lost to outer space.

But most of the water, a new study concludes, went down, sucked into the red planet’s rocks. And there it remains, trapped within minerals and salts. Indeed, as much as 99 percent of the water that once flowed on Mars could still be there, the researchers estimated in a paper published this week in the journal Science. Data from the past two decades of robotic missions to Mars, including NASA’s Curiosity rover and the Mars Reconnaissance Orbiter, showed a wide distribution of what geologists call hydrated minerals.

“It became very, very clear that it was common and not rare to find evidence of water alteration,” said Bethany L. Ehlmann, a professor of planetary science at the California Institute of Technology and one of the authors of the paper. Dr. Ehlmann, speaking at a news briefing Tuesday at the Lunar and Planetary Science conference, said that as the rocks are altered by liquid water, water molecules become incorporated into minerals like clays. “Water is effectively trapped into the crust,” she said. To get a sense of the amount of water, planetary scientists talk about a “global equivalent layer” — that is, if Mars were smoothed out into a uniform, featureless ball, how deep would the water have been? The scientists estimated that the depth would have been 100 to 1,500 meters, or 330 to 5,000 feet.

The most likely depth was about 2,000 feet, they said, or roughly one-fourth as much water as is in the Atlantic Ocean.

The data and simulations also indicated that the water was almost all gone by three billion years ago, around the time on Earth when life consisted of single-cell microbes in the oceans. “This means that Mars has been dry for quite a long time,” said Eva Scheller, a Caltech graduate student who was the lead author of the Science paper. Today, there is still water equivalent to a global ocean 65 to 130 feet deep, but that is mostly frozen in the polar ice caps.

Planetary scientists have long marvelled at ancient evidence of flowing water carved in the Martian surface — gigantic canyons, tendrils of winding river channels and deltas where the rivers disgorged sediments into lakes. NASA’s latest robotic Mars explorer, Perseverance, which landed last month in the Jezero crater, will be headed to a river delta at its edge in hopes of finding signs of past life.

Without a time machine, there is no way to observe directly how much water was on a younger Mars more than three billion years ago. But the hydrogen atoms floating today in the atmosphere of Mars preserve a ghostly hint of the ancient ocean. On Earth, about one in 5,000 hydrogen atoms is a version known as deuterium that is twice as heavy because its nucleus contains both a neutron and a proton. (The nucleus of a common-variety hydrogen atom has only a proton, no neutrons.) On Earth, water is also absorbed in rocks, but it does not stay there indefinitely. The movement of Earth’s crust pushes rocks down into the mantle, where they melt, and the molten rock — and water — comes back up through volcanoes. On Mars, volcanism, like liquid water, appears to have gone away long ago.

Chang is a science reporter for NYT©2020

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