It was a daunting task that took five years and the accumulation of many data sets from NASA’s powerful Hubble and Spitzer space telescopes.
But in the end, a team led by UdeM astronomy professor Björn Benneke has assembled for the first time a “fingerprint” of the chemical composition of a new class of planet unlike anything found in our solar system.
The one that Benneke’s team studied in particular – described in a paper published in Nature Astronomy – is called GJ 3470 b.
It may be a cross between Earth and Neptune, with a large rocky core buried beneath a deep hydrogen and helium atmosphere so heavy it crushes everything beneath it. GJ 3470 b weighs 12.6 times the mass of Earth, and less than Neptune, which is more than 17 Earth masses.
Many similarly sized worlds have been discovered by NASA’s Kepler space observatory. In fact, 80 per cent of the planets in our galaxy fall into this mass and size range. However, astronomers have never been able to understand the chemical nature of such a planet until now.
Only by making an inventory of the what’s in GJ 3470 b’s atmosphere was the team able to uncover clues to the planet’s nature and origin.
“This is a big discovery in how planets are formed,” said Benneke, whose team included 16 researchers in the U.S. and one in the Netherlands. “GJ 3470 b orbits very close to its star and is 30 times less massive than Jupiter but has managed to accrete the same kind of primordial hydrogen/helium atmosphere, largely unpolluted by heavier elements. We don’t have anything like this in the solar system, and that’s what makes it striking.”
Changes in starlight
Key to studying the atmosphere of a world like GJ 3470 b are spectroscopic observations. To probe the planet, the astronomers enlisted the combined multi-wavelength capabilities of the Hubble and Spitzer telescopes. They measured changes in starlight as the planet passed in front of its star (transit) and passed behind it (eclipse). In total, the two space telescopes observed 12 transits and 20 eclipses.
“For the first time we have a spectroscopic signature of such a world,” said Benneke, the study’s lead author, adding that so far his team has been unable to come up with a name to classify the type of planet GJ 3470 b is: “super-Earth,” “sub-Neptune” or something else.
One thing they can accurately describe is GJ 3470b’s atmosphere: it’s mostly clear, covered only in thin hazes that are transparent under infrared light, so the scientists were able probe deep into it.
“We expected to find an atmosphere strongly enriched in heavier elements like oxygen and carbon that create abundant water vapor and methane gas,” said Benneke. “Instead, we found an atmosphere that is so poor in heavy elements that its composition resembles the hydrogen/helium rich composition of the sun.”
The new evidence suggests that, unlike other exoplanets that are thought to have migrated toward their star from a distance much farther out in the galaxy, GJ 3470 b formed just where it is today, Benneke believes.
So close to a red dwarf
Why? Probably because the planet was born precariously close to its red dwarf star. Benneke hypothesizes that it essentially started out as a dry rock 1.5 to two times the diameter of Earth; it then rapidly accreted hydrogen from a primordial disk of gas around its star.
“If the planet had formed further from the star, where water and other astronomical ices can condense, we would have expected to see more water and methane in the atmosphere,” the scientist explained.
“We’re seeing an object that was able to accrete hydrogen from the protoplanetary disk, but didn’t run away to become what we call a ‘hot Jupiter’ – this is intriguing. One explanation is that the circumstellar disk dissipated before the planet could bulk up further. So it got stuck being a sub-Neptune.”
Soon, thanks to its unprecedented sensitivity in the infrared spectrum, NASA’s James Webb Space Telescope will be able to probe even deeper into GJ 3470 b’s atmosphere. That will allow closer observation of the transits and eclipses of GJ3470b to a precision of between 3 and 5 micrometres, where atmospheric hazes become increasingly transparent.
Source: University of Montreal