One of the most amazing recent discoveries in our Solar System is how much the landscape of Saturn’s moon Titan resembles Earth: Titan is dotted with lakes and seas; it has river channels, islands, mud, rain clouds and maybe even rainbows. The giant moon is undeniably wet. The “water” on Titan is not, however, H2O. With a surface temperature dipping 290 degrees F below zero, Titan is far too cold for liquid water. Instead, researchers believe the fluid that sculpts Titan is an unknown mixture of methane, ethane, and other hard-to-freeze hydrocarbons.
Yet something has been nagging at Alex Hayes, a planetary scientist on the Cassini radar team at Cornell University. If Titan is really so wet, he wonders, “Where are all the waves?” On Titan, the lakes are eerily smooth, with no discernable wave action down to the millimeter scale, according to radar data from Cassini. “We know there is wind on Titan,” says Hayes. “The moon’s magnificent sand dunes [prove] it.”
Add to that the low gravity of Titan—only 1/7th that of Earth—which offers so little resistance to wave motion, and you have a real puzzle.
Researchers have toyed with several explanations. Perhaps the lakes are frozen. Hayes thinks that is unlikely, however, “because we see evidence of rainfall and surface temperatures well above the melting point of methane.” Or maybe the lakes are covered with a tar-like substance that damps wave motion. “We can’t yet rule that out,” he adds.
The answer might be found in the results of a study Hayes and colleagues published in the July 2013 online edition of the journal Icarus. Taking into account the gravity of Titan, the low viscosity of liquid hydrocarbons, the density of Titan’s atmosphere, and other factors, they calculated how fast wind on Titan would have to blow to stir up waves: A walking-pace breeze of only 1 to 2 mph should do the trick.
This suggests a third possibility: the winds just haven’t been blowing hard enough. Since Cassini reached Saturn in 2004, Titan’s northern hemisphere (where most of the lakes are located) has been locked in the grip of winter. Cold heavy air barely stirs, and seldom reaches the threshold for wave-making.
But now the seasons are changing. In August 2009 the sun crossed Titan’s equator heading north. Summer is coming, bringing light, heat and wind to Titan’s lake country.
“According to [climate models], winds will pick up as we approach the solstice in 2017 and should be strong enough for waves,” he says.
If waves appear, Cassini should be able to detect them. Radar reflections from wavy lake surfaces can tell researchers a great deal. Wave dimensions, for instance, may reveal the viscosity of the underlying fluid and, thus, its chemical composition. Also, wave speeds would track the speed of the overlying winds, providing an independent check of Titan climate models.
Hayes is excited about “bringing oceanography to another world. All we need now,” he says, “are some rough seas.”
Publication: Ralph D. Lorenz, et al., “A global topographic map of Titan,” Icarus, Volume 225, Issue 1, July 2013, Pages 367-377; DOI:10.1016/j.icarus.2013.04.002
The Daily Galaxy via Dr. Tony Phillips, Science@NASA