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|   › Larger image › Image with scale › Full photomap › View video of Pluto rotating (Credit: NASA, ESA, and M. Buie/Southwest Research Institute)  | 
NASA today released the most detailed set of images ever taken of the distant dwarf planet Pluto. The images taken by NASA's Hubble Space Telescope show an icy and dark molasses-colored, mottled world that is undergoing seasonal changes in its surface color and brightness. Pluto has become significantly redder, while its illuminated northern hemisphere is getting brighter. These changes are most likely consequences of surface ices sublimating on the sunlit pole and then refreezing on the other pole as the dwarf planet heads into the next phase of its 248-year-long seasonal cycle. The dramatic change in color apparently took place in a two-year period, from 2000 to 2002.
The Hubble images will remain our sharpest view of Pluto until NASA's New  Horizons probe is within six months of its Pluto flyby. The Hubble pictures are  proving invaluable for picking out the planet's most interesting-looking  hemisphere for the New Horizons spacecraft to swoop over when it flies by Pluto  in 2015.
Though Pluto is arguably one of the public's favorite planetary objects, it is  also the hardest of which to get a detailed portrait because the world is small  and very far away. Hubble resolves surface variations a few hundred miles  across, which are too coarse for understanding surface geology. But in terms of  surface color and brightness Hubble reveals a complex-looking and variegated  world with white, dark-orange and charcoal-black terrain. The overall color is  believed to be a result of ultraviolet radiation from the distant sun breaking  up methane that is present on Pluto's surface, leaving behind a dark and red  carbon-rich residue.
When Hubble pictures taken in 1994 are compared with a new set of images taken  in 2002 to 2003, astronomers see evidence that the northern polar region has  gotten brighter, while the southern hemisphere has gotten darker. These changes  hint at very complex processes affecting the visible surface, and the new data  will be used in continued research.
 
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The images are allowing planetary astronomers to better interpret more than three decades of Pluto observations from other telescopes, says principal investigator Marc Buie of the Southwest Research Institute in Boulder, Colo. "The Hubble observations are the key to tying together these other diverse constraints on Pluto and showing how it all makes sense by providing a context based on weather and seasonal changes, which opens other new lines of investigation."
The Hubble pictures underscore that Pluto is not simply a ball of ice and rock  but a dynamic world that undergoes dramatic atmospheric changes. These are  driven by seasonal changes that are as much propelled by the planet's 248-year  elliptical orbit as its axial tilt, unlike Earth where the tilt alone drives  seasons. The seasons are very asymmetric because of Pluto's elliptical orbit.  Spring transitions to polar summer quickly in the northern hemisphere because  Pluto is moving faster along its orbit when it is closer to the sun.
Ground-based observations, taken in 1988 and 2002, show that the mass of the  atmosphere doubled over that time. This may be due to warming and sublimating  nitrogen ice. The new Hubble images from 2002 to 2003 are giving astronomers  essential clues about how the seasons on Pluto work and about the fate of its  atmosphere.
The images, taken by the Advanced Camera for Surveys, are invaluable to planning  the details of the New Horizons flyby in 2015. New Horizons will pass by Pluto  so quickly that only one hemisphere will be photographed in the highest possible  detail. Particularly noticeable in the Hubble image is a bright spot that has  been independently noted to be unusually rich in carbon monoxide frost. It is a  prime target for New Horizons. "Everybody is puzzled by this feature," says  Buie. New Horizons will get an excellent look at the boundary between this  bright feature and a nearby region covered in pitch-black surface material.
"The Hubble images will also help New Horizons scientists better calculate the  exposure time for each Pluto snapshot, which is important for taking the most  detailed pictures possible," says Buie. With no chance for re-exposures,  accurate models for the surface of Pluto are essential in preventing pictures  that are either under- or overexposed.
The Hubble images are a few pixels wide. But through a technique called  dithering, multiple, slightly offset pictures can be combined through  computer-image processing to synthesize a higher-resolution view than could be  seen in a single exposure. "This has taken four years and 20 computers operating  continuously and simultaneously to accomplish," says Buie, who developed special  algorithms to sharpen the Hubble data.
The Hubble research results appear in the March 2010 issue of the  Astronomical Journal. Buie's science team members are William Grundy of Lowell  Observatory in Flagstaff, Ariz., and Eliot Young, Leslie Young, and Alan Stern  of Southwest Research Institute in Boulder, Colo.
Buie plans to use Hubble's new Wide Field Camera 3 to make further Pluto  observations prior to the arrival of New Horizons.
The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute conducts Hubble science operations. The institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc. in Washington, D.C.
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