Astronomers have discovered three super-Earth planets orbiting a star about 100 light-years away from our solar system. The three exoplanets discovered by researchers at Harvard-Smithsonian Center for Astrophysics (CfA) in the US have radii of about 1.6, 1.3, and 2.1 Earth-radii respectively.
CfA astronomers Joseph Rodriguez, Andrew Vanderburg, Jason Eastman, David Latham, and Samuel Quinn and their team of scientists discovered three small transiting planets orbiting the star GJ9827 which lies at the relatively close distance of 100 light-years. The three exoplanets are categorised as super-Earths, that is, with masses that are larger than Earth’s but less than Neptune’s. GJ9827 is one of the few known stars to have multiple transiting terrestrial-sized exoplanets that are suited for atmospheric characterisation.
“Its three exoplanets are particularly interesting because two of them have radii between 1.5 and 2.0 Earth-radii,” said Joseph Rodriguez from CfA. “Across this range in radii, the composition of planets is expected to change from rocky to gaseous; moreover, there are relatively few such candidates for study.”
The study indicated that these planets orbit very close to the star, with periods of 1.2, 3.6 and 6.2 days respectively, and at these close distances they have fairly hot temperatures, estimated at 1,172, 811 and 680 degrees kelvin. Future observations will probe their atmospheres and provide a much more detailed picture of this unusual family of super-Earths, researchers said.
Over 3,500 extra-solar planets have been confirmed to date, according to the study published in The Astronomical Journal. Most of them were discovered using the transit method, and astronomers can combine the transit light curves with velocity wobble observations to determine the planet’s mass and radius, and thereby constrain its interior structure.
Further, it was pointed out that the planet’s atmosphere can be studied owing to the fact that the chemical composition of the atmosphere means its opacity varies with wavelength. By measuring the depth of the transit at different wavelengths, it is possible to infer the composition and temperature of the planet’s atmosphere.