Kepler-93: A testbed for detailed seismic modelling and orbital evolution of super-Earths around solar-like stars

The advent of space-based photometry missions such as CoRoT, Kepler and TESS has sparkled the development asteroseismology exoplanetology. PLATO will further strengthen multi-disciplinary studies. Testing asteroseismic modelling its importance for our understanding planetary systems is crucial. We carried out a detailed Kepler-93, an exoplanet host star observed by Kepler. This particularly interesting it very similar to benchmark target (G spectral type, ~ 6000K, 1 Msun Rsun) provides real-life testbed potential procedures be used PLATO. use global local minimization techniques seismic varying ingredients stellar models. compute inversions mean density. these revised parameters provide new simulate orbital evolution system under effects tides atmospheric evaporation. Our fundamental Kepler-93: density = 1.654 +/- 0.004 g/cm3, M 0.907 0.023 , R 0.918 0.008 Rsun Age 6.78 0.32 Gyr. uncertainties we report this are within requirements For Kepler-93b, find Mp 4.01 0.67 Mearth, Rp 1.478 0.014 Rearth semi-major axis 0.0533 0.0005 AU. According simulations, seems unlikely that Kepler-93b formed with mass large enough impacted tides. PLATO, able requirements. illustrate what synergies can achieved regarding evaporation exoplanets. note high-quality radial velocity follow-up constrain formation scenarii