Science

Dust storms spotted on Saturn's moon Titan for 1st time

Saturn’s largest moon, Titan, is a world most similar to our own, with a considerable atmosphere, lakes and weather patterns. Now astronomers have discovered yet another way in which Titan is like our planet: dust storms.

Moon joins Earth and Mars as objects in the solar system with dust storms

An artist's concept of a dust storm on Titan. Recent data suggests that Titan experienced a dust storm near its equator in 2009. (IPGP/Labex UnivEarthS/University Paris Diderot – C. Epitalon & S. Rodriguez)

Saturn's largest moon, Titan, is a world most similar to our own, with a considerable atmosphere, lakes and weather patterns. Now astronomers have discovered yet another way in which Titan is like our planet: dust storms.

Using data from NASA's Cassini spacecraft — in orbit around Saturn from July 2004 to September 2017 — scientists found what they believe to be giant dust storms around the planet's equatorial regions.

Titan is the second-largest moon in our solar system. Of all the more than 150 known moons in Earth's celestial backyard, it is the only one with a substantial atmosphere, made up of mostly nitrogen, like Earth's. It also has clouds, rivers and lakes. But instead of water, they contain hydrocarbons like methane and ethane, chemicals found in gasoline.

And at first, that's what researchers thought they were looking at when they scanned the data collected in 2009. They thought the brightening region were clouds of methane.

This animation, based on images captured by NASA's Cassini spacecraft during several Titan flybys in 2009 and 2010, shows clear bright spots that researchers suggest are dust storms. (NASA/JPL-Caltech/University of Arizona/University Paris Diderot/IPGP/S. Rodriguez et al. 2018)

"From what we know about cloud formation on Titan, we can say that such methane clouds in this area and in this time of the year are not physically possible," Sebastien Rodriguez, an astronomer at Paris Diderot University in France and lead author of a study on the phenomenon published in Nature Geoscience.

Aside from the unlikelihood that clouds would develop around the equator during this time of year — the moon's northern equinox — another reason for their conclusion was that the formation occurred far lower in the atmosphere than clouds would.

They also ruled out frozen methane rain or icy lavas. That left them with just one explanation: dust.

They'd seen dust on the surface of Titan before. In January 2005, the Huygens probe, which was part of the Cassini mission, landed on the moon's surface, kicking up a small amount of organic dust.

"But what we spotted here with Cassini is at a much larger scale." Rodriguez said.

"The near-surface wind speeds required to raise such an amount of dust as we see in these dust storms would have to be very strong — about five times as strong as the average wind speeds estimated by the Huygens measurements near the surface and with climate models."