Data from the New Horizons mission revealed many previously unknown things about Pluto, and hinted at others. One tantalising tidbit was the prospect of an ammonia-rich ocean of water under the surface, a liquid sea beneath the frozen plains.
"Thanks to the incredible data retued by New Horizons, we were able to observe tectonic features on Pluto's surface, update our thermal evolution model with new data and infer that Pluto most likely has a subsurface ocean today," said lead author Noah Hammond, a graduate student in Brown University's Department of Earth, Environmental and Planetary Sciences. The paper has been published in the joual Geophysical Research Letters.
The team updated a thermal model of Pluto based on detailed data from the New Horizons probe, with tectonic features such as fault lines hundreds of kilometres long and up to 4 km (2.5 miles) deep, and mountains of water ice that indicated Pluto is slowly expanding over time. If Pluto had had oceans that completely froze long ago, then the dwarf planet would have been shrinking over time.
"What New Horizons showed was that there are extensional tectonic features, which indicate that Pluto underwent a period of global expansion," Hammond said. "A subsurface ocean that was slowly freezing over would cause this kind of expansion."
How could the water remain liquid so far from the sun? The slow natural decay of radioactive elements in Pluto's core may have been sufficient to keep the water unfrozen beneath the icy surface. Over time, however, that water could have started to refreeze. Since water expands as it tus into ice, this would have produced the features seen on Pluto's surface.
"We now have half a dozen worlds, like [Satu's moon] Enceladus, [Jupiter's moons] Europa and Ganymede, and now Pluto, that seem to have oceans in their interiors," said New Horizons lead scientist Alan Ste earlier this year. "It's interesting that only Earth wears its ocean on the outside. From the surface, we don't see them. Who knew that oceans would tu out to be fairly common?"
To determine whether the ocean is still liquid or whether it has already frozen entirely, Hammond and his team ran a thermal evolution model using New Horizons data on Pluto's diameter and density. They found that, if the ocean under Pluto's surface had frozen completely already, it would have changed to a phase called ice II, which has a much more compressed structure than ordinary water ice, aka ice I. Basically, if there was no liquid water under Pluto's surface, it would show signs of contraction, rather than expansion.
This stage would only occur if Pluto's icy shell was more than 260 km (155 miles) thick, but evidence suggests that Pluto's shell is at least 300 km (186 miles) thick. So the case for liquid water on Pluto is strong.
"That's amazing to me," Hammond said. "The possibility that you could have vast liquid water ocean habitats so far from the sun on Pluto -- and that the same could also be possible on other Kuiper belt objects as well -- is absolutely incredible."
en apple news...
ما را در سایت en apple news دنبال می کنید
برچسب : نویسنده : استخدام کار applen بازدید : 382 تاريخ : پنجشنبه 3 تير 1395 ساعت: 22:02