The planet GJ 1214b was discovered in 2009 using the HARPS¹ instrument on ESO's 3.6-metre telescope in Chile (eso0950 - http://www.eso.org/public/news/eso0950/). Initial findings suggested that this planet had an atmosphere, which has now been confirmed and studied in detail by an international team of astronomers², led by Jacob Bean (Harvard–Smithsonian Center for Astrophysics), using the FORS instrument on ESO's Very Large Telescope. "This is the first super-Earth to have its atmosphere analysed. We've reached a real milestone³ on the road toward characterising these worlds," said Bean.

GJ 1214b has a radius⁴（半径） of about 2.6 times that of the Earth and is about 6.5 times as massive, putting it squarely into the class of exoplanets（外部行星） known as super-Earths. Its host star lies about 40 light-years from Earth in the constellation⁵（星座，星群） of Ophiuchus (the Serpent Bearer). It is a faint star, but it is also small, which means that the size of the planet is large compared to the stellar disc, making it relatively⁶ easy to study. The planet travels across the disc of its parent star once every 38 hours as it orbits at a distance of only two million kilometres: about seventy times closer than the Earth orbits the Sun.

To study the atmosphere, the team observed the light coming from the star as the planet passed in front of it. During these transits⁷, some of the starlight passes through the planet's atmosphere and, depending on the chemical composition and weather on the planet, specific wavelengths⁸ of light are absorbed. The team then compared these precise new measurements with what they would expect to see for several possible atmospheric¹⁰ compositions.

Before the new observations, astronomers had suggested three possible atmospheres for GJ 1214b. The first was the intriguing¹¹（有趣的，迷人的） possibility that the planet was shrouded¹² by water, which, given the close proximity¹³ to the star, would be in the form of steam. The second possibility was that this is a rocky world with an atmosphere consisting mostly of hydrogen, but with high clouds or hazes¹⁴ obscuring the view. The third option was that this exoplanet was like a mini-Neptune, with a small rocky core and a deep hydrogen-rich atmosphere.

The new measurements do not show the telltale（报警的，泄密的） signs of hydrogen and hence rule out the third option. Therefore, the atmosphere is either rich in steam, or it is blanketed by clouds or hazes, similar to those seen in the atmospheres of Venus and Titan in our Solar System, which hide the signature of hydrogen..

"Although we can't yet say exactly what that atmosphere is made of, it is an exciting step forward to be able to narrow down the options for such a distant world to either steamy or hazy（朦胧的，模糊的） ," says Bean. "Follow-up observations in longer wavelength⁹ infrared¹⁵ light are now needed to determine which of these atmospheres exists on GJ 1214b."