The seven rocky planets circling the nearby star TRAPPIST-1 have lots of water, a new study suggests — perhaps too much to make them good bets for life.

All of the TRAPPIST-1 worlds likely harbor hundreds of Earth oceans’ worth of water on their surfaces, and the wettest ones may have over 1,000 times more of the stuff than our planet does, according to the study.

Surprisingly, this probably isn’t great news for the TRAPPIST-1 system’s life-hosting potential, study team members said. [Meet the 7 Earth-Size Exoplanets of TRAPPIST-1]

“Too much water can be a bad thing,” lead author Cayman Unterborn, a postdoctoral fellow in the School of Earth and Space Exploration at Arizona State University, told “The TRAPPIST-1s are interesting, but maybe not for life.”

TRAPPIST-1 is a dim red dwarf star that lies about 39 light-years from Earth. Astronomers discovered three planets circling the star in 2016, and four more were announced a year later. Each of the seven worlds — which are known as TRAPPIST-1b, c, d, e, f, g and h — is about the same size as Earth. And three of the alien worlds (e, f and g) are thought to lie in TRAPPIST-1’s “habitable zone” — that just-right range of distances where liquid water could likely exist on a planet’s surface.

TRAPPIST-1 is about 2,000 times dimmer than the sun, so the red dwarf’s habitable zone is very close-in. Indeed, all seven TRAPPIST-1 planets lie closer to their star than Mercury does to the sun.

This diagram shows illustrations of the seven TRAPPIST-1 planets and compares some of their key characteristics with those of the rocky planets in our own solar system.

Credit: NASA/JPL-Caltech

All of the TRAPPIST-1 planets were discovered via the “transit method“; several different instruments noticed the tiny brightness dips that resulted when the worlds crossed their host star’s face. The magnitude of these dips revealed the sizes of the worlds. And astronomers have been able to estimate the planets’ masses, though not nearly as precisely, by studying how their transits have varied over time. (These variations occur as neighboring planets tug on one another gravitationally.)

With this mass and volume information in hand, Unterborn and his team used computer models to get a better idea of the composition of six of the TRAPPIST-1 worlds. (They didn’t deal with TRAPPIST-1h, the outermost planet, because not enough is known about it.)

This modeling work suggested that there’s a wetness gradient in the TRAPPIST-1 system. The innermost planets, b and c, are probably about 10 percent water by mass, whereas the wet stuff makes up at least 50 percent of the more distant f and g. The middle planets d and e fall somewhere in between.

All of these worlds are sopping wet, even at the low end of the gradient. For comparison, Earth is just 0.2 percent water by mass. Indeed, the TRAPPIST-1 planets are probably “water worlds,” with no land to break the monotony of wind and wave, Unterborn said.

If that is indeed the case, the odds of finding life in the system may not be great.

“With no exposed land, key geochemical cycles including the drawdown of carbon and phosphorus into oceanic reservoirs from continental weathering will be muted, thus limiting the size of the biosphere,” the researchers wrote in the new study, which was published online today (March 19) in the journal Nature Astronomy. “As such, although these planets may be habitable in the classical definition of the presence of surface water, any biosignature observed from this system may not be fully distinguishable from abiotic, purely geochemical sources.”

And all that water might shut down some key geological processes that could help life get a foothold, Unterborn said. For example, rocks in Earth’s mantle often become liquid after moving upward to a zone of lower pressure, where their melting point is lower. But such “decompression melting” may occur rarely, if at all, on the TRAPPIST-1 worlds, because the huge weight of the overlying global oceans jacks up mantle pressures so much.

Without molten rock near the surface, there can be no volcanoes (at least not the kind we’re used to here on Earth). And without volcanoes, heat-trapping gases, such as carbon dioxide, may have a hard time reaching the atmosphere — which means the TRAPPIST-1 planets may have been subjected to a “runaway snowball” effect, Unterborn said. [Gallery: The Strangest Alien Planets]

Planets orbiting red dwarfs face other habitability challenges, many researchers have stressed. For example, if these worlds orbit tightly enough to be in the habitable zone, they’re almost certainly “tidally locked,” meaning they always show the same face to their parent star. So, one side of such planets may be boiling hot while the other is frigid. This problem could be mitigated by the presence of a thick atmosphere, which would circulate heat. But red dwarfs fire off lots of powerful flares, which may quickly strip away the atmospheres of habitable-zone worlds.

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