Now astronomers are trying to work out whether its atmosphere is thick, or whether it's thin and wispy. Starting with the assumption that GJ 1132b formed with a water-rich atmosphere, astronomer Laura Schaefer, of the Harvard-Smithsonian Center for Astrophysics (CfA), and her team believe the latter is most likely.
In that scenario, the water molecules (H2O) on the exoplanet would have been broken down by the powerful ultraviolet light, releasing the hydrogen atoms to space, leaving the heavier oxygen behind as a thin atmosphere.
To test this idea, we need more powerful observatories to analyze the world's spectroscopic signature to see if its atmosphere does indeed contain oxygen. NASA's James Webb Space Telescope, which is scheduled for launch in 2018, could be used to detect this atmospheric oxygen.
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"On cooler planets, oxygen could be a sign of alien life and habitability. But on a hot planet like GJ 1132b, it's a sign of the exact opposite -- a planet that's being baked and sterilized," said Schaefer in a CfA statement.
Early in GJ 1132b's atmospheric evolution, its water vapor content would have acted as a powerful greenhouse gas, amplifying the star's already powerful heating. This would have ensured that the surface of the planet remained in a molten state for millions of years. Although the magma would have absorbed a little of the oxygen, and more would have been vented into space, enough would linger that could be detected with advanced astronomical studies.
"This planet might be the first time we detect oxygen on a rocky planet outside the solar system," said Robin Wordsworth, of the Harvard Paulson School of Engineering and Applied Sciences.
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Through studies of GJ 1132b, astronomers hope to understand how Venus' atmosphere evolved. Venus, too, is thought to have evolved with a water-rich atmosphere, but over time, the sun's ultraviolet light broke down the water molecules -- a process known as "photodissociation" -- causing the lighter hydrogen to be lost to space. However, very little oxygen has been detected in the Venusian atmosphere, creating a puzzle for planetary scientists.
Refinements to Schaefer's magma ocean-atmosphere model could, in this case, also be used to better understand Venus' mysterious atmosphere, as well as revealing how an exoplanet's atmosphere evolves when more advanced observatories go online.