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A powerful new model to detect life on planets outside of our solar system, more accurately than ever before, has been developed by researchers from °×С½ãÂÛ̳ Physics & Astronomy and the University of New South Wales.

Methane (CH4) is the simplest organic molecule.

Hot methane is important in cool stars, brown dwarfs, exoplanets, gas turbine engines, and elsewhere. There is a pressing need for an accurate and complete spectroscopic database for methane at elevated temperatures.ÌýThisÌýpaper presents a comprehensive spectroscopic line list for methane containing almost 10 billion transitions, 2,000 times more than any previous compilation, covering a broad spectroscopic range and applicable for temperatures up to 1,500 K.ÌýIt demonstrate that such a line list is essential for correctly modeling the brown dwarf 2MASS 0559- 14 (see figure) and leads to large changes in exoplanet models. We believe that this line list will have a large effect on the field of exoplanets and cool stars.

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