This radar image of the surface of Saturn's moon Titan was acquired on October 26, 2004, when the Cassini spacecraft flew approximately 994 miles (1,600 kms) above the surface. Brighter areas may correspond to rougher terrains and darker areas are thought to be smoother. This image highlights some of the darker terrain, which the Cassini team dubbed "Si-Si the Cat." This nickname was chosen after a team member's daughter, Si-Si, pointed out that the dark terrain has a cat-like appearance. Image
As we search for extraterrestrial life, Earth in some sense always provides our framework. The data indicate that life does in fact exist on this planet, and it existed here sometime before about 3.5 billion years ago (give or take a couple hundred million years). However, thanks to plate tectonics and other pesky processes, we're missing some critical information about this early time. This includes information about how life got started on Earth.
Titan may come to our rescue. As the largest of Saturn's moons--much larger than our own moon, larger even than the planet Mercury--Titan has several striking similarities with Earth. For one, it has a substantial, largely nitrogen atmosphere. For another, it supports an active volatile cycle. And the effects of this volatile cycle make Titan appear 'surprisingly Earth-like' (as scientists with the Cassini-Huygens mission have been saying). For example, images show what are interpreted to be convective clouds forming and then dissipating, apparently raining out onto the surface and producing what looked for all the world (pun intended) like terrestrial rivers and lakes.
But Titan also has significant dis-similarities from Earth, at least as we know it today. Instead of a water-based volatile cycle as on Earth, Titan cycles hydrocarbons. At Titan's temperature, water is about as solid as rock on Earth, but hydrocarbons--which are gaseous under terrestrial conditions--can evaporate into the atmosphere, re-condense into rain, and fall veeeery slowly (Titan's gravity is about 1/7th of Earth's) to the surface, either to pond or flow over the surface as a liquid. A summer cloudburst on Titan would be something like standing in a cloud of droplets of liquid natural gas at -300 degrees Fahrenheit. In addition to N2, Titan's atmosphere contains significant amounts of methane, and ethane and other hydrocarbon compounds have been detected.
One thing Titan's atmosphere does not contain is oxygen (which is probably just as well--oxygen + hydrocarbons is highly flammable). The story of the rise of oxygen on Earth is not well understood. Oxygen-rich habitats must have developed around the time of those cyanobacteria that produce oxygen (>2.7 Ga), but before that time, that is, during the Archean (3.8-2.5 Ga), life must have developed under oxygen-poor conditions. So how does that relate to Titan? Well, it means that Titan is like early Earth in not having oxygen. It's also good for astrobiologists interested in exploring the chemical, possibly pre-biotic, pathways that may have lead to the development of biota on early Earth.
This exploration takes a variety of forms. Some of it is theoretical modeling, trying to understand the large-scale movement and resultant combinations of materials that occur on Titan's surface. For example, in some equatorial regions, Cassini imagery shows what look like giant wind-blown dunes. These dunes seem to be composed preferentially of fine-grained organic sediments, which may facilitate interesting (i.e., biologically relevant) chemical interactions. These organic sediments form by UV photolysis and recombination of hydrocarbons in Titan's atmosphere, a process that gives Titan its orange haze (kind of like an L.A. smog on steroids). After these complex organic molecules are formed, they settle out of the sky onto Titan's surface to form dunes, fill up depressions, line river channels, and generally add to Titan's air of being a giant 'Rorschach inkblot test.' (In support of this statement, I respectfully cite the fact that an area of dark terrain in an early Radar image was referred to by the Cassini Team itself as 'Si-si the cat.' [See Image.]
Another approach to discovering pre-biotic chemistry of Titan and early Earth is experimental. This approach has a long history, dating back to the Miller-Urey experiment, in which gases believed to represent the atmosphere of early Earth were cruelly subjected to shock treatment (ie., simulated lightening) as a test to see how life might have arisen on Earth. Two decades, later in the late 1970's, Carl Sagan and Bishun Khare (who is now, appropriately, a scientist at the Carl Sagan Center), did a similar style of experiment using gases found in Titan's atmosphere. They created dark, reddish gunk, which they termed 'tholin' (from the Greek word for 'muddy'). These types of experiments require continual 'updating' as we learn more about the true conditions--and the actual gas species--that existed on early Earth and exist on Titan. A recent study, the most faithful yet to Titan's conditions, used a deuterium lamp to simulate atmospheric UV radiation of methane and measured the properties of the resultant aerosols.
This work is all focused on understanding Titan as an analogue for pre-biotic Earth. A small and courageous group of scientists have suggested that life may exist on Titan even today. This runs contrary to the maxim that life as we know it requires liquid water, of which Titan has none, but is based on the idea that non-aqueous life might arise through analogue chemistry. For example, ammonia--like water--is a polar molecule and dissolves other molecules--including hydrocarbons--with electrical charge.
Continued research here on Earth may inform us about this possibility for life on Titan today. Likewise, continued spacecraft investigation of Titan may tell use about life on Earth in the ancient past. In the exploration for life, Titan and Earth symbolize spatial and temporal symbiosis.
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