NASA Maps Geology of Pluto's 'Heart'

This map covers a portion of Pluto's surface that measures 1,290 miles (2,070km) from top to bottom, and includes the vast nitrogen-ice plain informally named Sputnik Planum and surrounding terrain. The map is overlaid with colors that represent different geological terrains. Each terrain, or unit, is defined by its texture and morphology – smooth, pitted, craggy, hummocky or ridged, for example

A newly created geological map of Pluto's famous heart-shaped region shows just how varied and complex the distant dwarf planet is.

Scientists on NASA's New Horizons mission, which performed the first-ever flyby of Pluto on July 14, have put together a color-coded geological map of Sputnik Planum, the huge nitrogen-ice plain that occupies the left side of Pluto's heart-shaped Tombaugh Regio.

The map covers an area that stretches 1,290 miles (2,070 kilometers) from top to bottom and features a resolution of at least 1,050 feet (320 meters) per pixel, NASA said. (Some parts of the map are even sharper than that.)

The blue and greenish units represent different textures seen across Sputnik Planum, from the cellular terrain in the center and north, to the smooth and pitted plains in the south. The black lines represent troughs that mark the boundaries of cellular regions in the nitrogen ice. Purple represents the chaotic mountain ranges that line Sputnik's western border, and the pink, floating hills at its eastern edge

The newly released map allows researchers to see variations in Pluto's terrain, which, in turn, can provide insight into the geological history of the dwarf planet.

For example, the bright yellow regions on the map are impact craters, which are notably absent from Sputnik Planum proper. This suggests that this portion of Pluto has been resurfaced recently; there hasn't been time for craters to pepper the surface there, scientists have said.

Other colors show different kinds of terrain, which are defined by their texture and form. One area coded with a greenish hue is defined as "featureless plains," while very light blue denotes "bright, cellular plains."

Hills of water ice on Pluto 'float' in a sea of frozen nitrogen and move over time like icebergs in Earth's Arctic Ocean. This shows the inset in context next to a larger view. The resolution is about 1050ft (320 meters) per pixel and 300 miles (almost 500km) long and 210 miles (340km) wide. It was taken 9,950 miles (16,000km) from Pluto, 12 minutes before New Horizons' closest approach to Pluto on July 14

The black lines are troughs, which delineate "cells" of nitrogen ice on Sputnik Planum that are thought to form as a result of convective processes.

The red area at the southern tip of the map shows the 2.5-mile-high (4.0 km) Wright Mons, which might be a volcano that spews ice rather than lava. Scientists aren't sure why the material around it, which looks reddish-brown in New Horizons' "true color" photos, isn't more widespread on the surface, NASA officials said.

To make this map, New Horizons team members used the spacecraft's Long Range Reconnaissance Imager (LORRI), taking pictures at a distance of 48,000 miles (77,300 km) from Pluto on July 14. At the time, New Horizons was less than 2 hours away from its closest approach, which brought the probe within just 7,800 miles (12,550 km) of Pluto's surface.

NASA