Pluto’s bizarre polygons now have a science explanation

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Pluto composite

A composite image of Pluto created using data from NASA’s New Horizons mission. (Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute)

Pluto is geologically alive.

Bizarre geometric shapes first spotted on the dwarf planet’s surface in 2015 are indications that a process called sublimation is ongoing, a new study suggests.

A fresh model indicates that the polygonal nitrogen ice on Pluto — spotted by NASA’s New Horizons spacecraft during a flyby — froze directly from vapor, rather than passing through a liquid state in between.

Lead author Adrien Morison, a research fellow at the University of Exeter in England, said his team’s work is the first explanation, based on modeling, that shows why the polygons are there. 

“Pluto is still geologically active despite being far away from the sun and having limited internal energy sources,” Morison said in a university statement. “This included at Sputnik Planitia, where the surface conditions allow the gaseous nitrogen in its atmosphere to coexist with solid nitrogen.”

Related: Destination Pluto: NASA’s New Horizons mission in pictures

The surface of Pluto’s icy Sputnik Planum — seen here in a photo captured by NASA’s New Horizons spacecraft during its close flyby of the dwarf planet on July 14, 2015 — is covered with churning ice “cells” that are geologically young and turning over due to convection.

The surface of Pluto’s icy Sputnik Planum — seen here in a photo captured by NASA’s New Horizons spacecraft during its close flyby of the dwarf planet on July 14, 2015 — is covered with churning ice “cells” that are geologically young and turning over due to convection. (Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute)

Sputnik Planitia is the most prominent geological feature on Pluto, as it is a huge oval-shaped zone straddling the equator of Pluto. Estimates from 2016, when it used to be called Sputnik Planum, peg the zone at 347,500 square miles (900,000 square kilometers) and at least 1.2 to 1.8 miles (2 to 3 km) deep. 

The new study consisted of numerical simulations, showing that as the nitrogen at Pluto cools during sublimation in Sputnik Planitia, it will produce polygons consistent with the size and topographical amplitude seen in New Horizons’ images. The new model also is consistent with larger worldwide climate models showing that the sublimation of Sputnik Planitia started one million or two million years ago.

This sublimation process may occur at other icy worlds around the solar system, the team noted, including Triton (a large moon at Neptune), or the Kuiper Belt objects Eris and Makemake far out in the solar system. But more observations of their surfaces would likely be required, which would in turn likely need spacecraft. Thus far there are no missions slotted to visit these various worlds.

A study based on the research was published Wednesday (Dec. 15) in Nature.

Follow Elizabeth Howell on Twitter @howellspace. Follow us on Twitter @Spacedotcom or Facebook. 

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