From Earth, both Mercury and Venus occasionally pass across the front of the Sun. When they do, they look like tiny black dots passing across the bright surface.
Such transits block a tiny fraction of the light that COROT is able to detect.
The convection rotation and planetary transits space telescope (COROT) has found the smallest terrestrial planet ever detected outside the solar system. The amazing planet is less than twice the size of Earth and orbits a Sun-like star. Its temperature is so high that it might be covered in lava or water vapor.
About 330 exoplanets have been discovered so far, most of which are gas giants with characteristics similar to Jupiter and Neptune.
The new find, COROT-Exo-7b, is different. Its diameter is less than twice that of Earth, and it orbits its star once every 20 hours. It is located very close to its parent star, and has a high temperature, between 1,800° and 2,700° Fahrenheit (1,000° and 1,500° Celsius). Astronomers detected the new planet as it transited its parent star, dimming the light from the star as it passed in front of it.
The density of the planet is still under investigation. It may be rocky like Earth and covered in liquid lava. It may also belong to a class of planets that are thought to be made up of water and rock in almost equal amounts. Given the high temperatures measured, the planet would be a very hot and humid place.
“Finding such a small planet was not a complete surprise”, said Daniel Rouan, researcher at the Observatoire de Paris Lesia, who coordinates the project with Alain Leger, from Institut d’Astrophysique Spatiale (Paris). “COROT-Exo-7b belongs to a class of objects whose existence had been predicted for some time. COROT was designed precisely in the hope of discovering some of these objects,” he said.
Few exoplanets found have a mass comparable to Earth’s and the other terrestrial planets — Venus, Mars, and Mercury. Terrestrial planets are difficult to detect. Most of the methods used so far are indirect and sensitive to the mass of the planet, while COROT can directly measure the size of its surface. In addition, its location in space allows for longer periods of uninterrupted observation than would be possible from the ground.
Recent measurements have indicated planets of small masses exist but their size remained undetermined until now.
The internal structure of COROT-exo-7b puzzles scientists. They are unsure if it is an ‘ocean planet’ — a kind of planet whose existence has never been proved so far. In theory, such planets would initially be covered partially in ice, and they would later drift towards their star, with the ice melting to cover it in liquid.
“This discovery is a very important step on the road to understanding the formation and evolution of our planet,” said Malcolm Fridlund, European Space Agency’s COROT project scientist. “For the first time, we have unambiguously detected a planet that is ‘rocky’ in the same sense as Earth. We now have to understand this object further to put it into context, and continue our search for smaller, more earthlike objects with COROT,” he said.
