Evidence of a liquid ocean beneath the icy surface of Pluto
has been growing since New Horizons, a NASA spacecraft, flew past the dwarf
planet last year.
Researchers have now made a new estimation of how
thick the liquid layer covering Pluto’s surface could be by studying thermal
models of the impact dynamics formed by an enormous crater on the dwarf planet’s
surface.
“Thermal models of Pluto’s interior and tectonic evidence
found on the surface suggest that an ocean may exist, but it’s not easy to
infer its size or anything else about it,”
Brown University assistant professor David Johnson, who is leading the study, said.
“We’ve been able to put some constraints on its thickness and get some clues
about composition.”
The study was recently published by Geophysical Research Letters and has discovered that there is a
possibility that the ocean of water beneath the surface of Pluto is 62 miles deep. The study also maintains that the ocean is composed of the
salt content similar to the Dead Sea.
The research was conducted on the famous heart-shaped Sputnik
Planum, located on the western lobe of the planet.
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