Glimpses of the events that nurtured life on Earth more than 3.5 billion years ago are coming from an unlikely venue almost 1 billion miles away, according to the leader of an effort to understand Titan, one of the most unusual moons in the solar system.
In a talk here today at the 246th
"Data sent back to Earth from space missions allow us to test an idea that underpins modern science's portrait of the origin of life on Earth," Lunine said. "We think that simple organic chemicals present on the primordial Earth, influenced by sunlight and other sources of energy, underwent reactions that produced more and more complex chemicals. At some point, they crossed a threshold -- developing the ability to reproduce themselves. Could we test this theory in the lab? These processes have been underway on Titan for billions of years. We don't have a billion years in the lab. We don't even have a thousand years."
Lunine, who is with
Titan is the only moon in the solar system known to have an atmosphere. Like Earth, most of it consists of nitrogen, with methane the second-most abundant. Sunlight strikes Titan's upper atmosphere, breaking that compound into pieces that react with each other and nitrogen to form organic compounds. Those include ethane, acetylene, hydrogen cyanide, cyanoacetylene and others -- all familiar terrestrial chemicals.
"We've got a very good inventory of what's there in the atmosphere," Lunine said. "What we've only recently begun to understand is the fate of these organics at the surface of Titan."
Lunine explained that for a long time, Mars had captured the public's and scientists' imagination as a possible location to find interesting organic chemistry and hints at life outside the Earth -- and for good reason: It is an Earth-like planet relatively close to the Sun. But scientists have only found simple organic materials on the red planet.
Recent research has provided fascinating hints that liquid water may exist deep under Titan's surface. Other data suggest that areas of Titan's seafloor may be similar to areas of Earth's seafloors where hydrothermal vents exist. These passways into Earth's interior spout hot, mineral-rich water that fosters an array of once-unknown forms of life. Lunine also cited research that has identified prime potential landing spots on Titan should the
Scientists now know, thanks to the joint NASA-ESA spacecraft that arrived at Saturn in 2004 after a seven-year journey through the solar system, that Titan shares a surprising number of features with Earth. The enormous volumes of data that Cassini's 12 scientific instruments and the Huygens surface probe streamed back to Earth paint a complex picture of Titan's surface and the dense atmosphere that enshrouds it. Rivers flow into lakes. Wind sweeps across dunes. Giant storms brew, and clouds float across the hazy sky.
The catch is that Titan, nearly a billion miles from the Sun and a little larger than the Earth's own moon, is mostly frozen. It only receives about 1 percent of the sunlight that Earth gets. As a result, it is unimaginably frigid. At minus 290 degrees Fahrenheit -- that's 160 degrees colder than the coldest recorded temperature in
Lunine acknowledged funding from the
The research was part of a symposium on "Chemical Frontiers in Solar System Exploration," which covers the gamut of the latest discoveries in space science, and experimental design and devices that are pushing the field to new levels. The following topics were among more than 30 presentations in the symposium:
Molecules and molecular evolution in cold extraterrestrial environments: The chemist's approach
Ice-gas interactions during planet formation
Composition and chemical history of early solar system ices
OSIRIS-REx will return a sample of asteroid 1999 RQ36 for astrochemistry
Other symposium topics include the chemistry of star and planet formation, low-temperature chemical reactions and new analytical techniques to study molecular interactions in space.
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