Methane gas rises from rotting garbage on Earth and droplets of liquid methane rain down on Saturn’s moon Titan. Even the planets Neptune and Uranus have an abundance of methane in their atmospheres. That’s why they appear blue-green.
Methane is a common chemical in our solar system, generated by living organisms and natural, non-living things.
So why are astronomers delighted to find methane in the atmosphere of a faraway planet orbiting another star? The detection was made with the Near-Infrared Camera and Multi-Object Spectrometer aboard NASA’s Hubble Space Telescope. The Jupiter-sized planet, called HD 189733b, is too hot to sustain life because it is too close to its parent star. The gas-giant planet completes an orbit in just over two days. Life as we know it could not exist on a planet whose atmosphere is a scorching 1,700 degrees Fahrenheit, about the temperature it takes to melt silver.
But astronomers say this detection offers hope that they will one day be able to probe the atmospheres of cooler, more hospitable worlds. Finding methane in the atmosphere of HD 189733b demonstrates that astronomers can successfully use spectroscopy to detect organic molecules on planets around other stars. Spectroscopy splits light into its component colors to reveal the “fingerprints” of various chemicals.
“This observation is one of the first steps in the search for life on another planet,” says astrophysicist Marc Kuchner of NASA Goddard Space Flight Center’s Exoplanets and Stellar Astrophysics Laboratory. “We need to study the chemistry in a planet’s atmosphere in order to determine whether the planet could harbor life.”
As the HD 189733b observation shows, organic chemicals like methane can be produced by chemical processes that do not require life. On Titan, Saturn’s largest moon, the abundance of methane may have been generated by a geological process between water and rock deep inside the moon. Even on Earth, not all the methane is the byproduct of life processes. A small amount of the gas is produced by volcanism.
Discovering methane on an Earth-like world in a habitable zone around a star — a location where liquid water could exist on the planet’s surface — would be promising, Kuchner says.
In their search for habitable planets, scientists have only one blueprint of life: Earth. Shaped, in part, by biological evolution, our planet has just the right balance of methane, oxygen, nitrogen, and water in its atmosphere. In addition, Earth orbits at just the right distance from its star, at a point where temperatures are ideal for liquid oceans to form and life therefore to thrive. But that does not rule out the possibility of other blueprints of life.
“There could be other ingredients and conditions for life that we don’t know about,” Kuchner says. “But how do we know if we have found a life-bearing planet if it is different from Earth?”
In fact, scientists may have missed signs of life on Mars when the Viking spacecraft visited the Red Planet more than 30 years ago. In 2007, a scientist at the University of Giessen in Germany announced that a reevaluation of Martian data suggests it may contain microbial life. The researcher said soil collected by Viking may have shown signs of a weird life form based on hydrogen peroxide on the subfreezing, dry Martian surface.
The tests conducted by instruments onboard the spacecraft, however, may have killed any Mars organisms, the German researcher and other scientists claim. The Viking spacecraft was equipped to analyze soil samples for indications of Earth-like living matter that thrived in water and warm temperatures. The Mars organisms had evolved to adapt to a frigid, dry environment.
One way to study alien worlds for life is to develop models of planetary atmospheres in a lab. The Virtual Planetary Laboratory at the California Institute of Technology’s Spitzer Science Center is one such “planetary model factory.” The research is driven by the idea that not all life is going to metabolize food and energy exactly as life on Earth does. So they are cooking up alternative environments on distant worlds where life could form.
Planets also can change over time. Earth is one example. Over the last 4.6 billion years, the amount of oxygen in Earth’s atmosphere has changed drastically over billions of years. Today’s oxygen levels are relatively high, but billions of years ago, oxygen did not exist on the planet.
Back then, the first homesteaders, members of a family of single-cell microorganisms called archaea, thrived in Earth’s hostile environment. One type of archaeon was a methanogen, which emitted methane as a byproduct of its life process. Multi-cellular life began forming about 500 million years ago, when the oxygen level in Earth’s atmosphere rose rapidly. The increase was probably due to blue-green algae that produced oxygen as a waste byproduct.
Even if scientists discover the right mix of chemicals for a habitable planet, they may not be able to rule out whether non-biological processes created them.
In 1990 noted astronomer Carl Sagan conducted a test on whether scientists could prove if life exists on Earth. He and several colleagues used the Galileo spacecraft, which was en route to Jupiter, to take snapshots of Earth to look for evidence of life.
The spacecraft’s instruments detected far more oxygen, methane, and nitrous oxide in Earth’s atmosphere than a lifeless planet would normally have. Other important ingredients of life discovered by Galileo were water in its solid, liquid, and gaseous forms and chlorophyll, which plants use for photosynthesis, covering some land surfaces.
“Our results are consistent with the hypothesis that widespread biological activity now exists, of all the worlds in this solar system, only on Earth,” Sagan and his colleagues wrote in their paper, published in the journal Nature.
He wondered, however, whether people from alien worlds would come to the same conclusion.
“But how plausible a world covered with carbon-fixing photosynthetic organisms, using water as the electron donor and generating a massive (and poisonous) oxygen atmosphere, might be to observers from a very different world is an open question.”
The most convincing clue for Earthly life was the modulated radio waves emanating from our planet’s surface.
“On the basis of these observations, a strong case can be made that the signals are generated by an intelligent form of life on Earth,” Sagan wrote. The researchers also noted that as recently as a century ago, these signals, and hence intelligent life, would not have been detected by a passing spaceship.
If the Galileo analysis of Earth is any measure, then proving the existence of life on a distant world will be a challenging task for future telescopes. “How can you take a spectrum of an extrasolar planet’s atmosphere and know for certain whether there is life or not?” Kuchner asks. “There is probably a huge range of atmospheres on extrasolar planets. Some probably have biomarkers of life, but those biosignatures are not a ‘slam-dunk’ for life on those planets. I think life on another planet may not be confirmed unless we go there.”
One way to bolster evidence for habitable planets is to build up an inventory of the atmospheres of many distant worlds so that astronomers can make comparisons to better determine the ones where life could exist.
"Tales of ... The hunt for life on other worlds" explains how scientists used spectroscopy to detect methane on a Jupiter-sized planet that orbits close to its parent star. The planet is unlikely to harbor life as we know it because the temperature is hot enough to melt silver. The discovery is significant because scientists may be able to use this method to study planets that are more likely to harbor life.
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HubbleSite press release: "Hubble Finds First Organic Molecule on an Exoplanet"
HubbleSite: Press releases on Extrasolar Planets