Using data from Nasa’s Kepler and Spitzer space telescopes, astronomers have created the first cloud map of a Jupiter-like exoplanet known as Kepler-7b.

The planet is marked by high clouds in the west and clear skies in the east. This is the first look at cloud structures on a distant world.

“By observing this planet with Spitzer and Kepler for more than three years, we were able to produce a very low-resolution ‘map’ of this giant, gaseous planet,” said Brice-Olivier Demory of Massachusetts Institute of Technology in Cambridge. “We wouldn’t expect to see oceans or continents on this type of world, but we detected a clear, reflective signature that we interpreted as clouds.”

Kepler’s visible-light observations of Kepler-7b’s moon-like phases led to a rough map of the planet that showed a bright spot on its western hemisphere. But these data were not enough on their own to decipher whether the bright spot was coming from clouds or heat. The Spitzer Space Telescope played a crucial role in answering this question.

Like Kepler, Spitzer can fix its gaze at a star system as a planet orbits around the star, gathering clues about the planet’s atmosphere. Spitzer’s ability to detect infrared light means it was able to measure Kepler-7b’s temperature, estimating it to be between 816 and 982 degrees Celsius. This is relatively cool for a planet that orbits so close to its star – within 0,06 astronomical units (one astronomical unit is the distance from Earth and the Sun) – and, according to astronomers, too cool to be the source of light Kepler observed. Instead, they determined, light from the planet’s star is bouncing off cloud tops located on the west side of the planet.

“Kepler-7b reflects much more light than most giant planets we’ve found, which we attribute to clouds in the upper atmosphere,” said Thomas Barclay, Kepler scientist at Nasa’s Ames Research Centre. “Unlike those on Earth, the cloud patterns on this planet do not seem to change much over time – it has a remarkably stable climate.”

The findings are an early step toward using similar techniques to study the atmospheres of planets more like Earth in composition and size.

Source: Jet Propulsion Laboratory