Scientists Reconsider Habitability of Saturn's Moon

Scientists Reconsider Habitability of Saturn's Moon
False color image of Saturn's moon Titan. (Image credit: NASA/JPL/Space Science Institute)

Recent findings from NASA's Cassini spacecraft and new discoveries about organisms here on Earth that thrive in extreme conditions are causing scientists to rethink the possibility that there may be life on Saturn's cloudy moon Titan.

Analyzing data from Cassini's recent Titan flybys, scientists at the Southwestern Research Institute (SwRI) in Texas and Washington State University announced last week that several of the key elements crucial for life on Earth are also present on Titan, including liquid reservoirs, organic molecules and ample energy sources.

Discovered in 1655 by a Dutch astronomer, Titan is the second largest moon in the solar system apart from Jupiter's Ganymede. Looking around, a person standing on Titan's surface would see rocky fields strewn with small ice pebbles. Gazing up, one would see clouds racing across the orange Titan sky as if on fast forward, because like Venus, Titan's atmosphere rotates much faster than its surface. Saturn and its magnificent rings would not be visible most of the time, due to the dense haze of orange smog that blankets the entire moon.

The Sun's ultraviolet light reacts with nitrogen and methane high in the upper reaches of Titan's atmosphere, producing the orange smog and a steady stream of organic materials that fall steadily onto the moon's surface. 

Many of the natural forces that shape the Earth's landscape are also active on Titan, including shifting continental plates, wind erosion, possibly oceans-albeit of ethane and methane and not water-and volcanoes. On Earth, these forces raise mountains and carve canyons, yet much of Titan's surface looks smooth, leading many scientists to suspect that the moon is relatively young.

If life does exist on Titan, a good place to look for it may be in hot springs connected to hydrocarbon reservoirs, said David Grinspoon, a researcher at SwRI's Space Science and Engineering Division.

Grinspoon speculated that life on Titan, if there is any, might be able to produce energy by mixing acetylene, a hydrocarbon abundant in Titan's atmosphere, with hydrogen. The energy could then be harnessed to power metabolism or to heat their surroundings.

"In environments that are energy-rich but liquid-poor, like near the surface of Titan, natural selection may favor organisms that use their metabolic heat to melt their own watering holes," Grinspoon said.

The researchers presented their ideas Sept. 8 at the 2005 Meeting for the American Astronomical Society's Division for Planetary Sciences.

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Staff Writer

Ker Than is a science writer and children's book author who joined Space.com as a Staff Writer from 2005 to 2007. Ker covered astronomy and human spaceflight while at Space.com, including space shuttle launches, and has authored three science books for kids about earthquakes, stars and black holes. Ker's work has also appeared in National Geographic, Nature News, New Scientist and Sky & Telescope, among others. He earned a bachelor's degree in biology from UC Irvine and a master's degree in science journalism from New York University. Ker is currently the Director of Science Communications at Stanford University.