Most waves on the liquid methane lakes of Saturn’s largest moon, Titan, are only about 1 centimeter high, research shows. This indicates a serene environment that could be good news for future probes sent there.
“There’s a lot of interest in one day sending probes to the lakes, and when that’s done, you want to have a safe landing, and you don’t want a lot of wind,” says Cyril Grima, a research associate at the University of Texas Institute for Geophysics and lead author of the study in Earth and Planetary Science Letters. “Our study shows that because the waves aren’t very high, the winds are likely low.”
Titan is one of the locations in the solar system believed to possess the ingredients for life. In photos taken by the Cassini orbiter, it appears as a smooth brown orb because of its thick atmosphere clouded with gaseous nitrogen and hydrocarbons.
However, radar images from the same probe show that it has a surface crust made of water ice and drenched in liquid hydrocarbons. On Titan, methane and ethane fall from the sky as rain, fill deep lakes that dot the surface, and are possibly spewed into the air by icy volcanoes called cryovolcanoes.
“The atmosphere of Titan is very complex, and it does synthesize complex organic molecules—the bricks of life,” Grima says. “It may act as a laboratory of sorts, where you can see how basic molecules can be transformed into more complex molecules that could eventually lead to life.”
On top of that, it’s also thought to have an ocean of liquid water beneath its icy crust.
Grima developed a technique for measuring surface roughness in minute detail from radar data when he was a graduate student at the Université Grenoble Alpes in France, and then a postdoctoral fellow at UTIG.
Called radar statistical reconnaissance, the technique has been used to measure the snow density and its surface roughness in Antarctica and the Arctic, and to assist the landing site selection of NASA’s Mars lander InSight, which is scheduled to launch next year. Researchers at NASA’s Jet Propulsion Laboratory suggested he apply the technique to measuring Titan’s waves.
The research zeroes in on the three largest lakes in Titan’s northern hemisphere: Kraken Mare, Ligeia Mare, and Punga Mare. Kraken Mare, the largest of the three, is estimated to be larger than the Caspian Sea. By analyzing radar data collected by Cassini during Titan’s early summer season, researchers discovered that the waves across these lakes are diminutive, reaching only about 1 centimeter high and 20 centimeters long.
“Cyril’s work is an independent measure of sea roughness and helps to constrain the size and nature of any wind waves,” says coauthor Alex Hayes, an assistant professor of astronomy at Cornell University. “From the results, it looks like we are right near the threshold for wave generation, where patches of the sea are smooth and patches are rough.”
The results call into question the early summer’s classification as the beginning of the Titan’s windy season, Grima says because high winds probably would have made for larger waves.
Information on Titan’s climate is essential for sending a probe safely to the surface. Although there are no formal plans for a mission, there are plenty of concepts being developed by researchers around the world. The study indicates that if a future mission lands in early summer, there’s a good chance that it is in for a smooth landing.
Other coauthors are from NASA’s Jet Propulsion Laboratory and The Johns Hopkins University Applied Physics Laboratory. NASA and the California Institute of Technology Jet Propulsion Laboratory funded the work.
Source: University of Texas at Austin