Young, Jupiter-like planet discovered
- Los Alamos National Laboratory
- Nancy Ambrosiano
- Communications Office
- (505) 667-0471
Insights into planet formation could come from this observation
LOS ALAMOS, N.M., Aug. 13, 2015—A team of researchers has discovered a Jupiter-like planet within a young system that could provide a new understanding of how planets formed around our sun.
The new planet, called 51 Eridani b, is the first exoplanet discovered by the Gemini Planet Imager (GPI), a new instrument operated by an international collaboration headed by Bruce Macintosh, a professor of physics in the Kavli Institute at Stanford University. It is a million times fainter than its star and shows the strongest methane signature ever detected on an alien planet, which should yield additional clues as to how the planet formed.
“The exploration of very young planetary systems that will evolve to look like our own has just begun,” said Didier Saumon of Los Alamos National Laboratory, whose role was theoretical modeling and data analysis for the project.
“The Gemini Planet Imager is amazing new technology that has quickly discovered the first extrasolar analog of Jupiter, but much younger,” Saumon said.
The Gemini Planet Imager was designed specifically for discovering and analyzing faint, young planets orbiting bright stars. The GPI is located on the 8-meter Gemini South Telescope in Chile, although the coordinating science teams are spread globally.
After GPI was installed on the telescope in Chile, the team set out to look for planets orbiting young stars. They’ve looked at almost a hundred stars so far. “This is exactly the kind of planet we envisioned discovering when we designed GPI,” says James Graham, professor at UC Berkeley and Project Scientist for GPI.
The results are published in the current issue of Science.
As Saumon describes it, “this first analysis shows first, unequivocally, the presence of methane gas as the major carbon-bearing gas and water vapor in the atmosphere of the planet (which is otherwise dominated by hydrogen and helium, very much like our own Jupiter). The presence of methane, at the exclusion of other carbon-bearing gasses (such as carbon monoxide) is a first,” he said.
Also Saumon notes that “the planet is cooler and less luminous than any other planet found by direct imaging (i.e. photographed) so far, but still hotter than Jupiter (800F versus -200F).”
“Many of the exoplanets astronomers have imaged before have atmospheres that look like very cool stars,” said Macintosh, who led the construction of GPI and now leads the planet-hunting survey. “This one looks like a planet.”
Using GPI to study more young solar systems such as 51 Eridani b, he said, will help astronomers understand the formation of our neighbor planets, and how common that planet-forming mechanism is throughout the universe.
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