While there is one large lake and a few smaller ones near Titan’s south pole, almost all of Titan’s lakes appear near the moon’s north pole. Cassini scientists have been able to study much of the terrain with radar, which can penetrate beneath Titan’s clouds and thick haze. And until now, Cassini’s visual and infrared mapping spectrometer and imaging science subsystem had only been able to capture distant oblique or partial views of this area.
Several factors combined recently to give these instruments great observing opportunities. Two recent flybys provided better viewing geometry. Sunlight has begun to pierce the winter darkness that shrouded Titan’s north pole at Cassini’s arrival in the Saturn system nine years ago. A thick cap of haze that once hung over the north pole also has dissipated as northern summer approaches. And Titan’s beautiful, nearly cloudless, rain-free weather continued during Cassini’s flybys this past summer.
The images are mosaics in infrared light based on data obtained during flybys of Titan on July 10, July 26, and September 12, 2013. The colorized mosaic from the visual and infrared mapping spectrometer, which maps infrared colors onto the visible-color spectrum, reveals differences in the composition of material around the lakes. The data suggest parts of Titan’s lakes and seas may have evaporated and left behind the Titan equivalent of Earth’s salt flats. Only at Titan, the evaporated material is thought to be organic chemicals originally from Titan’s haze particles that once dissolved in liquid methane. They appear orange in this image against the greenish backdrop of Titan’s typical bedrock of water ice.
The near-infrared images from Cassini’s imaging cameras show a bright unit of terrain in the northern land of lakes that had not previously been visible in the data. The bright area suggests that the surface here is unique from the rest of Titan, which might explain why almost all of the lakes are found in this region. Titan’s lakes have very distinctive shapes — rounded cookie-cutter silhouettes and steep sides — and a variety of formation mechanisms have been proposed. The explanations range from the collapse of land after a volcanic eruption to karst terrain, where liquids dissolve soluble bedrock. Karst terrains on Earth can create spectacular topography such as the Carlsbad Caverns in New Mexico.
“Ever since the lakes and seas were discovered, we’ve been wondering why they’re concentrated at high northern latitudes,” said Elizabeth Turtle from the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. “So, seeing that there’s something special about the surface in this region is a big clue to help narrow down the possible explanations.”
Launched in 1997, Cassini has been exploring the Saturn system since 2004. A full Saturn year is 30 years, and Cassini has been able to observe nearly a third of a Saturn year. In that time, Saturn and its moons have seen the seasons change from northern winter to northern summer.
“Titan’s northern lakes region is one of the most Earth-like and intriguing in the solar system,” said Linda Spilker from NASA’s Jet Propulsion Laboratory in Pasadena, California. “We know lakes here change with the seasons, and Cassini’s long mission at Saturn gives us the opportunity to watch the seasons change at Titan, too. Now that the Sun is shining in the north and we have these wonderful views, we can begin to compare the different data sets and tease out what Titan’s lakes are doing near the north pole.”
