Thursday, July 14, 2016

NEW HORIZONS’ TOP 10 PLUTO PICS


One year ago, NASA’s New Horizons mission made history by exploring Pluto and its moons – giving humankind our first real look at this fascinating world on the frontier of our solar system.

Since those amazing days in July 2015 the New Horizons spacecraft has transmitted numerous images and many other kinds of data home for scientists and the public alike to study, analyze, and just plain love. From Pluto’s iconic “heart” and sweeping ice‐ mountain vistas to its flowing glaciers and dramatic blue skies, it’s hard to pick just one favorite picture. So the mission team has picked 10 – and in no special order, placed them here.

Click the titles for more information about each image. You’ve seen nine of them before, and the team added a 10th favorite, also sure to become one of New Horizons’ “greatest hits.”

What’s your favorite image? Tag @NASANewHorizons and #plutoflyby on Twitter, and let us know!


Vast Glacial Flows



New Horizons discovers flowing ices in Pluto’s heart-shaped feature.
Jagged Ice Shorelines and Snowy Pits



NASA’s New Horizons spacecraft zooms in on the southeastern portion of Pluto’s great ice plains, where at lower right the plains
Blue Skies



Blue haze around Pluto.
Charon Becomes a Real World



Pluto
The Vistas of Pluto



Pluto's mountains, frozen plains and foggy hazes
A Dynamic Duo: Pluto and Charon in Enhanced Color




Pluto and it's moon Charon
Strange Snakeskin Terrain



Terrain of Pluto in closeup
Pluto’s Heart




Pluto
Far Away Snow‐Capped Mountains



Pluto’s Snowcapped Methane Peaks
Colorful Composition Maps of Pluto



These compositional maps indicate the regions rich in ices of methane, nitrogen and carbon monoxide, and water ice.


The powerful instruments on New Horizons not only gave scientists insight on what Pluto looked like, their data also confirmed (or, in many cases, dispelled) their ideas of what Pluto was made of. These compositional maps – assembled using data from the Linear Etalon Imaging Spectral Array (LEISA) component of the Ralph instrument – indicate the regions rich in ices of methane (CH4), nitrogen (N2) and carbon monoxide (CO), and, of course, water ice (H2O).

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