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New Horizons’ Flyby of Pluto Concludes into Five Papers

March 18, 2016 By Karen Jackson Leave a Comment

Ever since New Horizons fulfilled the mission it set out for more than ten years ago – to do a flyby of the dwarf planet Pluto – scientists have been thoroughly caught with studying every single piece of data and image that the probe beamed back to Earth. It is not very clear why humanity feels a strong attraction to the small, frozen and distant planet of our solar system. However, ever since its discovery in 1930, scientists have put in superhuman efforts to understand the peculiar nature of one of the last known objects of the solar system we live in.

This week, New Horizons scientists have finally published no less than five papers regarding Pluto in the journal Science, detailing all findings that they have achieved following the probe’s flyby of Pluto’s system during last summer. What was previously believed to be a dark, cold piece of rock slowly drifting onto the very edges of the solar system is now depicted of having a complex world with active and varied geology, what appears to be an atmosphere that can generate clouds of unknown chemistry.

And as small as this dwarf planet is, it still manages to maintain an entire system of even smaller moons and shows what appears to be a very animated world, despite its location at an average 39.5 astronomical units (AU; 1 astronomical unit equals roughly 143 million kilometers or 93 million miles) from the sun.

The first set of papers that are being published following the staggering exploration of New Horizons, the space craft that literally has gone where no man had gone before, even if remotely, treat the various aspects of the numerous discoveries made by scientists from nearly 50 gigabits of data that was collected by the craft. Out of everything that New Horizons has seen and learned, researchers have compiled a list of several central points of their findings, as they are treated and explained in the papers.

The geologic analysis of Pluto’s surface revealed a planet that has been active in the past 4 billion years, while some of its geographical areas are smooth and lacking in craters, which suggests young and newly formed (in astronomical terms, 10 million years old does qualify as new) planes. Studying Pluto’s atmosphere revealed possible reasons behind the formation of what is now known as the planet’s haze players, as well as temperature levels and the composition that seems to different depending on altitude.

The summary of all the findings that the New Horizons made during its five months spent nearby Pluto’s system can be found in PDF form on the Science Magazine official website.

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New Horizons Data Still Keeps Shedding Light on Pluto

February 26, 2016 By Nancy Young Leave a Comment

Even if it has been more than half a year since the probe’s fly-by of Pluto, the New Horizons data still keeps shedding light on Pluto. Images of the planet and data reads have been incoming from the distant probe ever since it has gone out of hibernation and gone back in action. This data has gone through multiple testing phases and research with the scientists from NASA since; after that, the data has slowly been made available to the public in order to share with the rest of humanity just how far our species has gone.

The most recent discovery that has been thrown our way by the NASA newsfeed is a beautiful picture of Pluto’s North Pole. The image was taken by New Horizons using the Ralph/Multispectral Visible Imaging Camera (MVIC), at an altitude of 21,100 miles from the surface of Pluto and about 45 minutes after the probe’s closest approach to the dwarf planet on July 14^th 2015.

The image depicts heavily battered terrain and incredibly long canyons scarring the entirety of that area. The canyons run through Pluto’s Lowell Region – also known as the Percival Lowell area – some of them as wide as 45 miles across. A closer study made on the nature of the canyons that seem to run close to the north pole of the planet has revealed that the ravines walls appear to look old; at least older than other, sharper canyon regions that were found on the planet.

Scientists have theorized two possible reasons for that: one would be that the canyons in this region are made of weaker materials that degrade faster. The other explanation would suggest that Pluto had tectonic activity in the past. The deepest of canyons measure about 2.5 miles depth in this particular region. Researchers also theorized that their creation may very well have been a result of subsurface ice melting below the ground, eventually causing a cave-in.

Scientists have also made a point of observing the yellow terrains that are particularly visible closer to the North Pole than they are in the other regions of the planet. While it’s not with a hundred percent certainty, scientists suspect that the hue is a result of methane deposits that ended up being processed more by the solar radiation than bluer terrain in other zones on the planet.

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More Astonishing News From New Horizons Spacecraft

February 5, 2016 By Michael Turner Leave a Comment

Mere days ago, we were graced with a real life image of Charon as it was taken last summer from the edges of the solar system and now we have even more astonishing news form New Horizons spacecraft. This time it’s about Pluto itself, and the amazing images that were rendered by NASA after the space probe that was launched back in 2006 did a fly by the dwarf planet last year during the summer.

The data that the probe has been feeding and beaming back to Earth along its 10-year trip has provided an immense amount of insight about the workings of our own solar system and truly went where nobody had been before. The newest news feeds from NASA display even more information that New Horizons has gathered from the farthest edges of our solar system; and more explicitly images and recordings of the dwarf planet Pluto.

Scientists have been studying all of the data gathered from Pluto ever since it first started getting fed to them back on Earth. A new analysis suggests that Pluto’s glaciers and made of water ice and that they float similarly to how icebergs do on the surface of the earth.

The reason this is possible is because of a difference in density. Because the water ice that the glaciers are made of has a lower density of the frozen nitrogen that the surface below them has (also common to objects in the Kuiper belt), they tend to ‘float’ or travel slowly. Although the glaciers there remain hard and frozen solid due to the -380 degrees Fahrenheit temperature on Pluto, they seem to break apart and move in a series.

These were conclusions drawn after closely studying the images depicting one particular zone of the planet Pluto – namely the Sputnik Planum. It was detected that the glaciers would slowly move across the flat plane, sometimes as much as 12 miles across it. In earth terms, this would translate in gigantic icebergs that move across the frozen oceans. Except in Pluto’s case, it’s a gigantic frozen surface of nitrogen.

A particular portion of the Sputnik Planum, namely the Challenger Colles, appears to be a large accumulation of these glaciers. Scientists speculate that this is a place where the nitrogen ice below is shallower than in other parts, making the water ice glaciers ‘station’ and gather here. The Challenger Colles zone is 37 by 22 miles, while the entire Sputnik Planum zone is believed to span for about 300 by 210 miles.

The image taken by New Horizons was captured about 12 minutes before the probe’s closest approach to Pluto, from a range of approximately 9,950 miles from the surface on July 14^th, 2015.

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