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New Horizons Pluto Mission update thread

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Pluto's present, hazy atmosphere is almost entirely free of clouds, though scientists from NASA's New Horizons mission have identified some cloud candidates after examining images taken by the New Horizons Long Range Reconnaissance Imager.



Serenity Chasma, Charon.

New Horizons scientists have spotted signs of long run-out landslides.
 

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NASA's New Horizons spacecraft has sent back the last bit of data from its 2015 flyby of Pluto.

The picture — one of a sequence of shots of Pluto and its big moon, Charon — arrived earlier this week at Mission Control in Maryland.

It took more than five hours for the image to reach Earth from New Horizons, some 3 billion miles away.


In all, more than 50 gigabits of data were relayed over the past 15 months to Johns Hopkins University's Applied Physics Laboratory in Laurel, Maryland.

The final data arrived Tuesday, and NASA announced the safe arrival Thursday.

The team will make absolutely certain nothing got left behind, before erasing the recorders to make room for future observations.

Now the spacecraft is 350 million miles from the dwarf planet and aiming for 2014 MU69, another remote object in the Kuiper Belt.
 

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Can't remember if I posted these before




It's kinda mindblowing that Pluto and Charon are locked in eternal dance and Pluto with its cold but pulsing heart, which may have an ocean beneath, just faces away from Charon. And all that stuff is rich in CO, methane, water and nitrogen ices. And even there, so many AUs away, Solar wind still hits them and produces some cool X-rays. Come on, it's fantastic. It's .. I dunno it's just awesome. Few years ago I wouldn't have given a flying fuck about stuff like this, was busy with computers and other hardware. Really happy that I don't care about that stuff anymore. Science and truth forever, everything else is transitory. But I digress :D




 
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A new study led by Douglas Hamilton, professor of astronomy at the University of Maryland, suggests that Sputnik Planitia formed early in Pluto's history.

“The main difference between my model and others is that I suggest that the ice cap formed early, when Pluto was still spinning quickly, and that the basin formed later and not from an impact,” said Hamilton, who is lead author of the paper. “The ice cap provides a slight asymmetry that either locks toward or away from Charon when Pluto's spin slows to match the orbital motion of the moon.”
 
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Could there be life in Pluto's ocean?


Pluto is thought to possess a subsurface ocean, which is not so much a sign of water as it is a tremendous clue that other dwarf planets in deep space also may contain similarly exotic oceans, naturally leading to the question of life, said one co-investigator with NASA's New Horizon mission to Pluto and the Kuiper Belt.

William McKinnon, professor of Earth and planetary sciences in Arts & Sciences at Washington University in St. Louis and a co-author on two of four new Pluto studies published Dec. 1 in Nature, argues that beneath the heart-shaped region on Pluto known as Sputnik Planitia there lies an ocean laden with ammonia.

The presence of the pungent, colorless liquid helps to explain not only Pluto's orientation in space but also the persistence of the massive, ice-capped ocean that other researchers call “slushy” — but McKinnon prefers to depict as syrupy.

“In fact, New Horizons has detected ammonia as a compound on Pluto's big moon, Charon, and on one of Pluto's small moons. So it's almost certainly inside Pluto,” McKinnon said. “What I think is down there in the ocean is rather noxious, very cold, salty and very ammonia-rich — almost a syrup.

“It's no place for germs, much less fish or squid, or any life as we know it,” he added. “But as with the methane seas on Titan — Saturn's main moon — it raises the question of whether some truly novel life forms could exist in these exotic, cold liquids.”

“The idea that bodies of Pluto's scale, of which there are more than one out there in the Kuiper Belt, they could all have these kinds of oceans. But they'd be very exotic compared to what we think of as an ocean”.

“Life can tolerate a lot of stuff: It can tolerate a lot of salt, extreme cold, extreme heat, etc. But I don't think it can tolerate the amount of ammonia Pluto needs to prevent its ocean from freezing — ammonia is a superb antifreeze. Not that ammonia is all bad. On Earth, microorganisms in the soil fix nitrogen to ammonia, which is important for making DNA and proteins and such.

“If you’re going to talk about life in an ocean that’s completely covered with an ice shell, it seems most likely that the best you could hope for is some extremely primitive kind of organism. It might even be pre-cellular, like we think the earliest life on Earth was.”

The newly published research delves into the creation — likely by a 125-mile-wide Kuiper Belt object striking Pluto more than 4 billion years ago — of the basin that includes Sputnik Planitia.

The collapse of the huge crater lifts Pluto's subsurface ocean, and the dense water — combined with dense surface nitrogen ice that fills in the hole — forms a huge mass excess that causes Pluto to tip over, reorienting itself with respect to Charon.

But the ocean uplift won't last if warm water ice at the base of the covering ice shell can flow and adjust in the manner of glaciers on Earth. Add enough ammonia to the water, and it can chill to incredibly cold temperatures (down to minus 145 Fahrenheit) and still be liquid, even if quite viscous, like chilled pancake syrup. At these temperatures, water ice is rigid, and the uplifted surface ocean becomes permanent.

“All of these ideas about an ocean inside Pluto are credible, but they are inferences, not direct detections,” McKinnon said, sounding the call. “If we want to confirm that such an ocean exists, we will need gravity measurements or subsurface radar sounding, all of which could be accomplished by a future orbiter mission to Pluto. It's up to the next generation to pick up where New Horizons left off!”


View of Pluto with color-coded topography as measured by NASA's New Horizons spacecraft. Purple and blue are low and yellow and red are high, and the informally named Sputnik Planitia stands out at top as a broad, 1300 km wide, 2.5 km deep elliptical basin, most likely the site of an ancient impact on Pluto. New Horizons data imply that deep beneath this nitrogen-ice filled basin is an ocean of dense, salty, ammonia-rich water.
 
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Researchers found evidence that snow and ice features previously only seen on Earth, have been spotted on Pluto.

“Penitentes” which are formed by erosion, are bowl-shaped depressions with spires around the edge, and are several metres high.

The groundbreaking research, done in collaboration with researchers at NASA and Johns Hopkins University, indicates that these icy features may exist on other planets where environmental conditions are similar.

 
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A new study from the Georgia Institute of Technology provides additional insight into how Charon affects the continuous stripping of Pluto's atmosphere by solar wind.

When Charon is positioned between Sun and Pluto it can significantly reduce atmospheric loss.

Charon doesn't always have its own atmosphere. But when it does, it creates a shield for Pluto and redirects much of the solar wind around and away.

This barrier creates a more acute angle of Pluto's bow shock, slowing down the deterioration of the atmosphere. When Charon doesn't have an atmosphere, or when it's behind or next to Pluto (a term scientists call “downstream”), then Charon has only a minor effect on the interaction of the solar wind with Pluto.

As a result, Pluto still has more of its volatile elements, which have long since been blown off the inner planets by solar wind. Even at its great distance from the Sun, Pluto is slowly losing its atmosphere. Knowing the rate at which Pluto's atmosphere is being lost can tell us how much atmosphere it had to begin with, and therefore what it looked like originally. From there, we can get an idea of what the Solar System was made of during its formation.



 
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