Categories: Science

Wet-and-wild water worlds could kind beneath stress

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From:
Springer Nature

Planetary science: Water worlds would possibly kind beneath stress (N&V)

Some exoplanets could produce water throughout their formation through reactions between rocks and hydrogen, in response to new analysis in Nature. The findings supply perception into why some exoplanets have water on their floor.

The presence of water is a key ingredient in figuring out a planet’s habitability, and water has been thought to kind by way of condensation from area as ice or snow at low temperatures. This course of has usually been noticed in exoplanets between the dimensions of Earth and Neptune which might be situated far-off from their host star. However, NASA’s Kepler mission has discovered exoplanets between the sizes of Earth and Neptune with liquid water that orbit near their solar, calling this course of into query.

Harrison Horn and colleagues simulated reactions that would happen throughout planetary formation by heating rock samples with pulsed lasers in a high-pressure laboratory atmosphere. They noticed that hydrogen reacted with melted silicates from the rocks to launch oxygen, which then bonded with leftover hydrogen to kind water molecules. The authors recommend that this response may most certainly happen within the high-pressure and high-temperature core–envelope boundary of exoplanets, the place the denser, rocky core meets an outer envelope of gaseous parts. They recommend that this water-generating response may happen over billions of years on some exoplanets extra huge than Earth. However, the velocity of those reactions is decided by how a lot hydrogen is accessible and the way scorching the core–envelope boundary is.

The authors observe that these findings problem the pre-existing information on how water types on exoplanets of sure sizes and at sure distances from their host star.


Journal/
convention:

Nature


Organisation/s:
Arizona State University, USA


Funder:
S.-H.S. and H.W.H. had been supported by the National Science
Foundation (NSF) grants AST-2108129, AST-2406790 and EAR-1921298. Portions of this work
had been carried out at GeoSoilEnviroCARS (The University of Chicago, Sector 13), Advanced
Photon Source, Argonne National Laboratory. GeoSoilEnviroCARS is supported by the NSF,
Earth Sciences (EAR-1634415). This analysis used assets of the Advanced Photon Source,
a US DOE Office of Science User Facility operated for the DOE Office of Science by the
Argonne National Laboratory beneath contract no. DE-AC02-06CH11357. We acknowledge the
use of amenities within the Eyring Materials Center at ASU. Part of this work was carried out beneath
the auspices of the US DOE by Lawrence Livermore National Laboratory beneath contract
DE-AC52-07NA27344. The opinions are these of the authors and don’t essentially characterize
the opinions of LLNL, LLNS, DOE, NNSA or the US authorities. The US authorities, and the
writer, by accepting the article for publication, acknowledge that the US authorities
retains a non-exclusive, paid-up, irrevocable, worldwide licence to publish or reproduce
the printed type of this manuscript, or enable others to take action, for US authorities functions
(launch authorization no. LLNL-JRNL-872168). A.V. acknowledges help by ISF grants
770/21 and 773/21.


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