HUBBLE ATLAS
The Changing Faces of Pluto — image from the Hubble Space Telescope

Solar System

The Changing Faces of Pluto

February 4, 2010 · NASA

Zoom to full resolution Original on NASA ↗

This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003.

Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but 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, molasses-colored, carbon-rich residue.

The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the highest possible detail when NASA's New Horizons probe flies by Pluto in 2015.

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 series of pictures took four years and 20 computers operating continuously and simultaneously to accomplish.

About the colours

The image is a composite of separate exposures made by the ACS/HRC instrument on the Hubble Space Telescope. Two filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F435W (B) Green: F555W (V)

About the data

The image was created from Hubble data from proposals 5330 : A. Stern (Southwest Research Institute), L. Trafton (University of Texas, Austin), and M. Buie (Southwest Research Institute); and 9391 : M. Buie (Southwest Research Institute), W. Grundy (Lowell Observatory), and E. Young, L. Young, and A. Stern (Southwest Research Institute). The science team comprises: M. Buie (Southwest Research Institute), W. Grundy (Lowell Observatory), and E. Young, L. Young, and A. Stern (Southwest Research Institute).