eso0950 — Science Release

Astronomers Find World with Thick, Inhospitable Atmosphere and an Icy Heart

16 December 2009

Astronomers have discovered the second super-Earth exoplanet [1] for which they have determined the mass and radius, giving vital clues about its structure. It is also the first super-Earth where an atmosphere has been found. The exoplanet, orbiting a small star only 40 light-years away from us, opens up dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interior is likely to be mostly made of water ice. Its surface appears to be fairly hot and the planet is surrounded by a thick atmosphere, which makes it inhospitable for life as we know it on Earth.

In this week��s issue of Nature, astronomers announce the discovery of a planet around the nearby, low-mass star GJ1214 [2]. It is the second time a transiting super-Earth has been detected, after the recent discovery of the planet Corot-7b [3]. A transit occurs when the planet's orbit is aligned so that we see it crossing the face of its parent star. The newly discovered planet has a mass about six times that of our terrestrial home and 2.7 times its radius, falling in size between the Earth and the ice giants of the Solar System, Uranus and Neptune.

Although the mass of GJ1214b is similar to that of Corot-7b, its radius is much larger, suggesting that the composition of the two planets must be quite different. While Corot-7b probably has a rocky core and may be covered with lava, astronomers believe that three quarters of GJ1214b is composed of water ice, the rest being made of silicon and iron.

GJ1214b orbits its star once every 38 hours at a distance of only two million kilometres ��Ԉ�70 times closer to its star than the Earth is to the Sun. ��Being so close to its host star, the planet must have a surface temperature of about 200 degrees Celsius, too hot for water to be liquid,�� says David Charbonneau, lead author of the paper reporting the discovery.

When the astronomers compared the measured radius of GJ1214b with theoretical models of planets, they found that the observed radius exceeds the models�� predictions: there is something more than the planet��s solid surface blocking the star��s light �� a surrounding atmosphere, 200 km thick. ��This atmosphere is much thicker than that of the Earth, so the high pressure and absence of light would rule out life as we know it,�� says Charbonneau, ��but these conditions are still very interesting, as they could allow for some complex chemistry to take place.��

��Because the planet is too hot to have kept an atmosphere for long, GJ1214b represents the first opportunity to study a newly formed atmosphere enshrouding a world orbiting another star,�� adds team member Xavier Bonfils. ��Because the planet is so close to us, it will be possible to study its atmosphere even with current facilities.��

The planet was first discovered as a transiting object within the MEarth project, which follows about 2000 low-mass stars to look for transits by exoplanets [4]. To confirm the planetary nature of GJ1214b and to obtain its mass (using the so-called Doppler method), the astronomers needed the full precision of the HARPS spectrograph, attached to ESO��s 3.6-metre telescope at La Silla. An instrument with unrivalled stability and great precision, HARPS is the world��s most successful hunter for small exoplanets.

��This is the second super-Earth exoplanet for which the mass and radius could be obtained, allowing us to determine the density and to infer the inner structure,�� adds co-author Stephane Udry. ��In both cases, data from HARPS was essential to characterise the planet.��

��The differences in composition between these two planets are relevant to the quest for habitable worlds,�� concludes Charbonneau. If super-Earth planets in general are surrounded by an atmosphere similar to that of GJ1214b, they may well be inhospitable to the development of life as we know it on our own planet.

Notes

[1] A super-Earth is defined as a planet between one and ten times the mass of the Earth. An exoplanet is a planet orbiting a star other than the Sun.

[2] The star GJ1214 is five times smaller than our Sun and intrinsically three hundred times less bright.

[3] Corot-7b is the smallest and fastest-orbiting exoplanet known and has a density quite similar to the Earth's, suggesting a solid, rocky world. Discovered by the CoRoT satellite as a transiting object, its true nature was revealed by HARPS (eso0933).

[4] The MEarth project uses an armada of eight small telescopes each with a diameter of 40 cm, located on top of Mount Hopkins, Arizona, USA. MEarth looks for stars that change brightness. The goal is to find a planet that crosses in front of, or transits, its star. During such a mini-eclipse, the planet blocks a small portion of the star��s light, making it dimmer. NASA��s Kepler mission also uses transits to look for Earth-sized planets orbiting Sun-like stars. However, such systems dim by only one part in ten thousand. The higher precision required to detect the drop means that such worlds can only be found from space. In contrast, a super-Earth transiting a small, red dwarf star yields a greater proportional decrease in brightness and a stronger signal that is detectable from the ground.

More information

This research was presented in a paper appearing this week in Nature (��A Super-Earth Transiting a Nearby Low-Mass Star��, by David Charbonneau et al.).

The team is composed of David Charbonneau, Zachory K. Berta, Jonathan Irwin, Christopher J. Burke, Philip Nutzman, Lars Buchhave, David W. Latham, Ruth A. Murray-Clay, Matthew J. Holman, and Emilio E. Falco (Harvard-Smithsonian Center for Astrophysics, Cambridge, USA), Christophe Lovis, Stephane Udry, Didier Queloz, Francesco Pepe, and Michel Mayor (Observatoire de l��Universit�� de Gen��ve, Switzerland), Xavier Bonfils, Xavier Delfosse, and Thierry Forveille (University Joseph Fourier �� Grenoble 1/CNRS, LOAG, Grenoble, France), and Joshua N. Winn (Kavli Institute for Astrophysics and Space Research, MIT, Cambridge, USA).

ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world��s most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world��s most advanced visible-light astronomical observatory, and VISTA, the world��s largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become ��the world��s biggest eye on the sky��.

Contacts

St��phane Udry
Geneva University, Switzerland
Geneva, Switzerland
Tel: +41 22 379 2467
Email: stephane.udry@unige.ch

Xavier Bonfils
Universit�� Joseph Fourier - Grenoble 1 / CNRS, Laboratoire d'Astrophysique de Grenoble (LAOG), France
France
Tel: +33 47 65 14 215
Email: xavier.bonfils@obs.ujf-grenoble.fr

David Charbonneau
Harvard-Smithsonian Center for Astrophysics
Cambridge, USA
Tel: +1 617 496 6515
Email: dcharbon@cfa.harvard.edu

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