Weather forecasters on a pair of exoplanets would have an easy job. Today's forecast: cloudy. Tomorrow: overcast. Extended outlook: more clouds. Scientists using the Hubble Space Telescope have characterized the atmospheres of two of the most common type of planets in the Milky Way galaxy and found both may be blanketed with clouds. The best guess is that the clouds are not like anything found on Earth. Their scorching atmospheres are predicted to be hundreds of degrees Fahrenheit – too hot for a rainy day.
Weather forecasters on exoplanet GJ 1214b would have an easy job. Today's forecast: cloudy. Tomorrow: overcast. Extended outlook: more clouds.
Two teams of scientists using NASA's Hubble Space Telescope report they have characterized the atmospheres of a pair of planets with masses intermediate between gas giants, like Jupiter, and smaller, rockier planets, like Earth. A survey by NASA's Kepler space telescope mission showed that objects in this size range are among the most common type of planets in our Milky Way galaxy. The researchers described their work as an important milestone on the road to characterizing potentially habitable, Earth-like worlds beyond the solar system.
The findings appear in separate papers in the January 2 issue of the journal Nature.
The two planets studied are known as GJ 436b and GJ 1214b. GJ 436b is categorized as a "warm Neptune" because it is much closer to its star than frigid Neptune is to our Sun. The planet is located 36 light-years away in the constellation Leo.
GJ 1214b is known as a "super-Earth" type planet. Super-Earths are planets with masses between that of Earth and Neptune. Because no such planet exists in our solar system, the physical nature of super-Earths is largely unknown. GJ1214b is located just 40 light-years from Earth, in the constellation Ophiuchus.
Both GJ 436b and GJ 1214b can be observed passing in front of, or transiting, their parent stars. This provides an opportunity to study these planets in more detail as starlight filters through their atmospheres.
An atmospheric study of GJ 436b based on such transit observations with Hubble over the last year is presented in one of the papers, led by Heather Knutson of the California Institute of Technology in Pasadena, Calif. The news is about what they didn't find. The Hubble spectra were featureless and revealed no chemical fingerprints whatsoever in the planet's atmosphere. "Either this planet has a high cloud layer obscuring the view, or it has a cloud-free atmosphere that is deficient in hydrogen, which would make it very unlike Neptune," said Knutson. "Instead of hydrogen, it could have relatively large amounts of heavier molecules such as water vapor, carbon monoxide, and carbon dioxide, which would compress the atmosphere and make it hard for us to detect any chemical signatures."
Observations similar to those obtained for GJ 436b had been previously obtained for GJ 1214b. The first spectra of this planet were also featureless and presented a similar puzzle: The planet's atmosphere either was predominantly water vapor or hydrogen-dominated with high-altitude clouds.
A team of astronomers led by Laura Kreidberg and Jacob Bean of the University of Chicago used Hubble to obtain a deeper view of GJ 1214b that revealed what they consider definitive evidence of high clouds blanketing the planet. These clouds hide any information about the composition and behavior of the lower atmosphere and surface. The new Hubble spectra also revealed no chemical fingerprints whatsoever in the planet's atmosphere, but the high precision of the new data enabled them to rule out cloud-free compositions of water vapor, methane, nitrogen, carbon monoxide, or carbon dioxide for the first time.
"Both planets are telling us something about the diversity of planet types that occur outside of our own solar system; in this case we are discovering that we may not know them as well as we thought," said Knutson. "We'd really like to determine the size at which these planets transition from looking like mini-gas giants to something more like a water world or a rocky, scaled-up version of the Earth. Both of these observations are fundamentally trying to answer that question."
Models of GJ 436b and GJ 1214b predict clouds that could be made out of potassium chloride or zinc sulfide at the scorching temperatures of several hundred degrees Fahrenheit predicted to be found in these atmospheres. "You would expect very different kinds of clouds to form on these planets than you would find, say, on Earth," said Kreidberg.
The Chicago team had to make a big effort to conclusively determine the nature of GJ 1214b's cloudy atmosphere. Kreidberg explained, "We really pushed the limits of what is possible with Hubble to make this measurement – our work devoted more Hubble time to a single exoplanet than ever before. This advance lays the foundation for characterizing other Earths with similar techniques." Added Bean, "I think it's very exciting that we can use a telescope like Hubble that was never designed with this in mind, do these kinds of observations with such exquisite precision, and really nail down some aspect of a super-Earth atmosphere."
Knutson continued, "For exoplanets, clouds are incredibly frustrating because they can hide the bulk composition of the atmosphere that we want to measure." However, more will be learned with the launch of the James Webb Space Telescope later this decade. Said Kreidberg, "Looking forward, the James Webb Space Telescope will be transformative. The new capabilities of this telescope will allow us to peer through the clouds on GJ 1214b and similar exoplanets."
About GJ 1214b:
Object Description: Extrasolar Planet
R.A.: 17h 15m 18s.94
Dec.: +04° 57' 49".72
Distance: 40 light-years (12.3 parsecs)
Exposure Dates: September 27, 2012 - August 4, 2013
The Hubble data are from proposal 13021: J. Bean (University of Chicago), J.-M. Desert (California Institute of Technology), S. Seager (Massachusetts Institute of Technology), D. Deming (University of Maryland), B. Benneke (Massachusetts Institute of Technology), Z. Berta-Thompson (Harvard University), K. Stevenson (University of Chicago), and D. Homeier (Lyon Centre for Astrophysics Research).
The science team includes: L. Kreidberg and J. Bean (University of Chicago), J.-M. Desert (California Institute of Technology), B. Benneke (Massachusetts Institute of Technology), D. Deming (University of Maryland), K. Stevenson (University of Chicago), S. Seager (Massachusetts Institute of Technology), Z. Berta-Thompson (Harvard University), A. Seifahrt (University of Chicago), and D. Homeier (Lyon Centre for Astrophysics Research).
About GJ 436b:
Object Description: Extrasolar Planet
R.A.: 11h 42m 11s.09
Dec.: +26° 42' 23".65
Distance: 36 light-years (9.2 parsecs)
Exposure Dates: October 26, November 29, and December 10, 2012, and January 2, 2013
The Hubble data are from proposal 11622: H. Knutson (California Institute of Technology), D. Charbonneau (Harvard University), and S. Seager (Massachusetts Institute of Technology).
The science team includes: H. Knutson (California Institute of Technology), B. Benneke (Massachusetts Institute of Technology), D. Deming (University of Maryland), and D. Homeier (Lyon Centre for Astrophysics Research).