Pluto’s famous heart powers icy winds on the dwarf planet

The left lobe of Pluto's heart-shaped feature is a 600-mile-wide (1,000 kilometers) ice plain known as Sputnik Planitia.

The left lobe of Pluto’s heart-shaped feature is a 600-mile-wide (1,000 kilometers) ice plain known as Sputnik Planitia. (Image: © NASA/JHUAPL/SwRI)

Pluto’s icy heart is beating. The dwarf planet’s famous heart-shaped feature, which NASA’s New Horizons spacecraft discovered during its epic July 2015 flyby, drives atmospheric circulation patterns on Pluto, a new study suggests.

Most of the action comes courtesy of the heart’s left lobe, a 600-mile-wide (1,000 kilometers) nitrogen-ice plain called Sputnik Planitia. This exotic ice vaporizes during the day and condenses into ice again at night, causing nitrogen winds to blow, the researchers determined. (Pluto’s atmosphere is dominated by nitrogen, like Earth’s, though the dwarf planet’s air is about 100,000 times thinner than the stuff we breathe.)

These winds carry heat, particles of haze and grains of ice westward, staining the ices there with dark streaks.

“This highlights the fact that Pluto’s atmosphere and winds — even if the density of the atmosphere is very low — can impact the surface,” study lead author Tanguy Bertrand, an astrophysicist and planetary scientist at NASA’s Ames Research Center in California, said in a statement.

And that westward direction is interesting in itself, considering that Pluto spins eastward on its axis. The dwarf planet’s atmosphere therefore exhibits an odd “retrorotation,” study team members said.

Bertrand and his colleagues studied data gathered by New Horizons during the probe’s 2015 close encounter. The researchers also performed computer simulations to model Pluto’s nitrogen cycle and weather, especially the dwarf planet’s winds.

This work revealed the likely presence of westerly winds — a high-altitude variety that races along at least 2.5 miles (4 kilometers) above the surface and a fast-moving type closer to the ground that follows Sputnik Planitia’s western edge.

That edge is bounded by high cliffs, which appear to trap the near-surface winds inside the Sputnik Planitia basin for a spell before they can escape to the west, the new study suggested.

“It’s very much the kind of thing that’s due to the topography or specifics of the setting,” planetary scientist Candice Hansen-Koharcheck, of the Planetary Science Institute in Tucson, Arizona, said in the same statement.

“I’m impressed that Pluto’s models have advanced to the point that you can talk about regional weather,” added Hansen-Koharcheck, who was not involved in the new study.

New Horizons’ Pluto flyby revealed that the dwarf planet is far more complex and diverse than anyone had thought, featuring towering water-ice mountains and weird “bladed” terrain in addition to the photogenic heart (whose official name, Tombaugh Regio, honors the discoverer of Pluto, Clyde Tombaugh).

The new study, which was published online Tuesday (Feb. 4) in the Journal of Geophysical Research: Planets, reinforces and extends that basic message.

“Sputnik Planitia may be as important for Pluto’s climate as the ocean is for Earth’s climate,” Bertrand said. “If you remove Sputnik Planitia — if you remove the heart of Pluto — you won’t have the same circulation.”

Read more at www.space.com


PRINCIPIA SCIENTIFIC INTERNATIONAL, legally registered in the UK as a company incorporated for charitable purposes. Head Office: 27 Old Gloucester Street, London WC1N 3AX. 

Please DONATE TODAY To Help Our Non-Profit Mission To Defend The Scientific Method.

Trackback from your site.

Comments (2)

  • Avatar

    Joseph Olson

    |

    GREAT NEWS….there is a place in our solar system to relocate our useless wind mills.

    Reply

  • Avatar

    Andy Rowlands

    |

    Very interesting article.

    Reply

Leave a comment

Save my name, email, and website in this browser for the next time I comment.
Share via