Ever since NASA’s New Horizons spacecraft flew by Pluto last year, evidence has been mounting that the dwarf planet may have a liquid ocean beneath its icy shell. Now, by modeling the impact dynamics that created a massive crater on Pluto’s surface, a team of researchers has made a new estimate of how thick that liquid layer might be. The study, led by Brown University geologist Brandon Johnson and published in Geophysical Research Letters, finds a high likelihood that there’s more than 100 km of water beneath Pluto’s surface...
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A large section of Pluto’s icy surface is renewed by convection that replace older ices with fresher material. Combining computer models with topographic and compositional data gathered by NASA’s New Horizons spacecraft last summer, New Horizons team members have been able to determine the depth of this layer of solid nitrogen ice within Pluto’s distinctive “heart” feature, Sputnik Planum – and how fast that ice is flowing.
Mission scientists used state-of-the-art computer simula...
Read MoreThese Pluto images are the best close-ups  that humans may see for decades...
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