A warm Jupiter-sized planet transiting the pre-main sequence star V1298 Tau
arXiv:1902.09670 · doi:10.3847/1538-3881/ab290f
Abstract
We report the detection of V1298 Tau b, a warm Jupiter-sized planet ( = 0.91 0.05~ , days) transiting a young solar analog with an estimated age of 23 million years. The star and its planet belong to Group 29, a young association in the foreground of the Taurus-Auriga star-forming region. While hot Jupiters have been previously reported around young stars, those planets are non-transiting and near-term atmospheric characterization is not feasible. The V1298 Tau system is a compelling target for follow-up study through transmission spectroscopy and Doppler tomography owing to the transit depth (0.5\%), host star brightness ( = 8.1 mag), and rapid stellar rotation ( = 23 \kms). Although the planet is Jupiter-sized, its mass is presently unknown due to high-amplitude radial velocity jitter. Nevertheless, V1298 Tau b may help constrain formation scenarios for at least one class of close-in exoplanets, providing a window into the nascent evolution of planetary interiors and atmospheres.
arXiv commentAccepted to AJ
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