New Issue: Orbital Catastrophe Ahead? Read Now

Scientists Explain Pluto’s Red-Headed Moon

Data from the New Horizons probe suggests Pluto's atmosphere paints the north pole of Charon, its largest moon

Pluto's largest moon Charon has a red spot at its north pole that may be caused by the atmosphere of Pluto, scientists announced on Sept. 14, 2016.

Pluto may be sharing its atmosphere with its largest moon, Charon, creating the visually striking red spot at the satellite's north pole.

New research suggests that conditions on the two worlds over the past few billion years would allow Pluto's traveling atmosphere to freeze out on the frigid moon Charon, while radiation would quickly transform the methane and nitrogen ices to a sticky residue known as tholins.

"Methane is volatile enough that it can only stick to the surface during the long, cold polar winters," Will Grundy, lead author of the new study, told Space.com by email. Grundy, a planetary scientist at the Lowell Observatory in Arizona, is part of NASA's New Horizons mission that made a historic flyby of Pluto in July 2015. After modeling conditions on Charon over the past few billion years, he and his colleagues found that, after methane from Pluto froze, radiation stripped away the hydrogen. (Methane is made up of hydrogen and carbon.) The carbon left behind joined with other molecules to make heavier fragments of materials able to stick around even after temperatures warmed [Amazing Pluto Flyby Photos by NASA's New Horizons]


On supporting science journalism

If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today.


"As more and more fragments join up, they build progressively bigger and more carbon-rich, complicated molecules until they are so complex that we don't even try to give them chemical names, just describe them with generic terms like 'organic molecules' or 'tholins,'" Grundy said. "These are what produce the reddish color."

The research was published online Sept. 14 in the journal Nature.

A captured atmosphere

When New Horizons made its historic flyby of Pluto, it also studied the moons around the dwarf planet. The largest of these moons, Charon, is nearly the size of Pluto itself, leading many scientists to classify the pair as a double-planet system. New Horizons revealed that the massive moon sports a red spot at its northern pole. 

Based on early measurements taken by the New Horizons spacecraft, Grundy and many othersimmediately speculated that the red spot was made of tholins created by the transfer of Pluto's atmosphere to Charon. They theorized that some of the material could freeze and that, later, radiation could convert it to tholins.

Pluto's small size means that it has trouble holding on to much of an atmosphere; many scientists questioned whether much of an atmosphere would remain by the time New Horizons made its visit. Observations revealed that Pluto manages to hold on to much of the gas around it, but some still escapes the dwarf planet's grasp.

"Pluto's atmosphere escapes radially outward in all directions, but Charon's gravity is strong enough to intercept a few percent of that flow," Grundy said. [Fly Through Giant Canyon on Pluto's Moon Charon | Video]

To measure the probability that Pluto's captured atmosphere became Charon's red spot, Grundy and colleagues modeled how temperatures changed over the moon's history. Charon's winters are cold, with polar temperatures only a few degrees higher than absolute zero (minus 459.67 degrees Fahrenheit, or minus 273.15 degrees Celsius) at coldest. Because the winters last so long—well over 100 Earth-years—the imported atmosphere has enough time to freeze.

The warmer temperatures near Charon’s equator allows less of the material to fall to the surface, which is why the red spot doesn't extend across the face of the moon. Charon itself is too small to hold on to its own gaseous atmosphere very long, so as the 100-year winters end, the atmosphere evaporates, leaving behind the larger hydrocarbons.

"For the most part, Charon's surface is too warm for methane to stick, so the methane molecules that make it to Charon's surface just bounce around there until they either escape back to space again or find a place cold enough to stick," Grundy said. "The winter pole does get cold enough for methane to stick; so methane will accumulate there, but only until the sun rises again in the spring and warms it back up."

Winter on Charon

During Charon's long winters, radiation from the sun and galactic cosmic rays convertedthe atmosphere to heavier material that does not evaporate rapidly when temperatures rise. When the winter pole tilted back toward the sun, ushering in spring, the remaining methane and nitrogen evaporated, leaving behind material that gradually changed to the reddish organics spotted at the surface. Grundy and his team estimate that about 30 centimeters (12 inches) of tholins would be produced at the poles over Charon's billion-year lifetime. The process should continue in the winter poles today, with material slowly building up its red spot.

Although Charon's southern pole was shrouded in darkness during the flyby, the researchers analyzed the light reflecting off of the dayside of Pluto to identify a slow dimming unrelated to the illumination, suggesting that the south pole may also boast its own spot.

"We don't have any color data to say that it's red, but in the black-and-white images lit by Pluto shine, it does show a darkening that is similar in darkness and size to what's seen around the northern pole," Grundy said. "The two poles take turns being the winter pole, just like on Earth."

Copyright 2016 SPACE.com, a Purch company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

Subscribe to Support Independent Journalism

Great science journalism requires human expertise, time, effort and creativity. And it costs money. That’s why I and the journalists here at Scientific American hope you’ll join our community.

When you subscribe, you are supporting staff and freelance journalists who are passionate about telling science stories that are true, important and compelling. Our editors and reporters are often experts in their fields, which means they understand the nuances of big discoveries and can untangle the breakthroughs from the hype. With a subscription, you are also supporting rigorous fact-checking to ensure the words we publish are precise and accurate. And you’re supporting original illustrations, graphics and photos that bring you closer to an advanced laboratory, an ice sheet in Antarctica or a space mission in orbit. You’re helping us craft other types of high-quality journalism as well: Our newsletters are carefully written, edited and curated by staffers you have or will come to know and love. Our Science Quickly podcast is based on original reporting, collaboration with editors and scientists and exacting production.

Subscriptions keep this engine running so we can continue to deliver thoughtful, rigorous and independent science journalism to you. In an era of viral misinformation, this work is crucial. If you value what we do, I hope you’ll consider joining us as a subscriber

Thank you,

Jeanna Bryner, Editor in Chief, Scientific American

Subscribe