(Originally published by the Massachussets Institute of Technology)
December 9, 2010
Although most of the 500 exoplanets, or planets outside the solar system, that have been discovered to date are too hot to be habitable, the odds of finding an exoplanet small and cool enough to host life are expected to increase over the next few years as telescope technology improves. Bigger and better telescopes should help astronomers probe the atmospheres of smaller exoplanets to determine if they contain molecules like water and oxygen, which are essential for most life as we know it.
One important clue about the atmosphere and interior of a planet is the ratio of carbon to oxygen in its atmosphere. The rocky, or terrestrial, planets in the solar system — Mercury, Venus, Earth and Mars — all have more oxygen than carbon, just like the sun around which they formed, which has a carbon-to-oxygen ratio of one to two, or 0.5. But that ratio is not known for giant planets like Jupiter (318 times Earth’s mass) because water, which is the main carrier of oxygen, is only present deep in their atmospheres and is therefore difficult to measure. For years, astronomers have developed models about all exoplanetary atmospheres and interiors based on the assumption that their carbon-to-oxygen ratios are also about 0.5.
But a team led by a former postdoctoral researcher in MIT’s Department of Earth, Atmospheric and Planetary Sciences and the MIT Kavli Institute for Astrophysics, recently measured the first-ever planetary atmosphere that is substantially enriched in carbon. The researchers found that the carbon-to-oxygen ratio of WASP-12b, an exoplanet about 1.4 times the mass of Jupiter and located about 1,200 light years away, is greater than one. As they report in a paper published Wednesday in Nature, this carbon-rich atmosphere supports the possibility that rocky exoplanets could be composed of pure carbon rocks like diamond or graphite rather than the silica-based rock found in Earth.
“This is new territory and will motivate researchers to study what the interiors of carbon-rich planets could be made of,” says lead author Nikku Madhusudhan, who is now a postdoctoral researcher at Princeton University. Although WASP-12b is a “hot Jupiter,” or a Jupiter-sized, extremely hot exoplanet that is largely made of gas and has no surface to host life, it could potentially have a form of diamond or graphite in its interior. This first-ever finding of a carbon-rich exoplanet introduces an entirely new class of exotic exoplanets to explore. It’s also possible that rockier, Earth-sized exoplanets may have formed around the same star as WASP-12b billions of years ago. If detected, these smaller planets could also have carbon-rich atmospheres and interiors, meaning that for life to exist on these planets, it might have to survive with very little water and oxygen and plenty of methane, says Madhusudhan. That might not be so far-fetched given last week’s announcement by NASA of the discovery on Earth of bacteria that can survive in arsenic, a poison to humans.
Astronomers can figure out a planet’s atmospheric composition by observing its flux, or the light emitted by the planet at different wavelengths. The team, coordinated by Joe Harrington, a planetary scientist at the University of Central Florida, used NASA's Spitzer Space Telescope to observe the flux from WASP-12b right before it passed behind the star, an event known as secondary eclipse. Those observations were then combined with previously published observations obtained from Earth using the Canada-France-Hawaii Telescope in Hawaii. The planet was discovered in 2009 by researchers at the United Kingdom-based consortium for Wide Angle Search for Planets (WASP), who are also co-authors of the study.
Madhusudhan used the observations to conduct a detailed atmospheric analysis using a modeling technique he pioneered for exoplanetary atmospheres. The computer program he developed combines certain variables, such as a planet's temperature distribution, with different amounts of the most prominent molecules that exist in such atmospheres, which are methane, carbon dioxide, carbon monoxide, water vapor and ammonia, into one formula that produces theoretical flux values. The program analyzes millions of combinations of these variables, tracking those that most closely match the flux values measured by the telescopes. Through statistical analysis of these values, Madhusudhan can determine the most likely composition of the atmosphere.
Based on theories about what extremely hot Jupiters such as WASP-12b should look like, assuming carbon-to-oxygen ratios of 0.5, previous models suggested that their atmospheres should have plenty of water vapor, very little methane and an atmospheric layer known as a stratosphere. Instead, Madhusudhan’s team detected an atmosphere with more than 100 times excess methane and less water than had been expected. The observed composition is consistent with a carbon-to-oxygen ratio that is greater than one. The team also discovered the lack of a strong stratosphere, which contradicts existing theories of hot Jupiter atmospheres.
The discovery suggests that chunks of rock called planetesimals that slammed together to form WASP-12b billions of years ago may have been made of carbon-rich compounds like tar — a far cry from the watery, icy planetesimals that are thought to have formed the solar-system planets. This means that if smaller exoplanets are found to have carbon-rich atmospheres, their surfaces could be covered in a tar-like substance. Future research will investigate whether life — perhaps drastically different from life as we know it — could survive in such a carbon-rich environment.
“It’s exciting to even think about the possibility” of what carbon-rich planets could look like, says Adam Showman, a planetary scientist at the University of Arizona, who explains that although researchers knew that other solar systems should have a range of carbon-to-oxygen values, “this paper finally moves the discussion from pure speculation to plausible reality.” He notes that exoplanets with carbon-based interiors could exhibit a range of surface features, atmospheric compositions and potential for oceans or life.
In future work, Madhusudhan plans to study exoplanets of different sizes and temperatures to determine how common carbon-rich atmospheres are. He will also develop new models of carbon-rich exoplanets to investigate how such planets may have formed, what material might exist in their interiors and what kind of life could survive with very little water and oxygen and lots of methane.