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This paper summarizes the project work on asteroseismology at the ERASMUS+GATE 2020 Summer school on space satellite data. The aim was to do a globalasteroseismic analysis of KIC 5006817 and quantify its stellar properties usingthe high-quality, state of the art space missions data. We employed theaperture photometry to analyze the data from the Kepler space telescope and theTransiting Exoplanet Survey Satellite (TESS). Using the lightkurve Pythonpackage, we have derived the asteroseismic parameters and calculated thestellar parameters using the scaling relations. Our analysis of KIC 5006817confirmed its classification as a heartbeat binary. The rich oscillationspectrum facilitate estimating power excess ($\nu_{\rm max}$) at145.50$\pm$0.50 $\mu$Hz and large frequency separation ($\Delta\nu$) to be11.63$\pm$0.10 $\mu$Hz. Our results showed that the primary component is alow-luminosity, red-giant branch star with a mass, radius, surface gravity, andluminosity of 1.53$\pm$0.07 M$_\odot$, 5.91$\pm$0.12 R$_\odot$, 3.08$\pm$0.01dex, and 19.66$\pm$0.73 L$_\odot$, respectively. The orbital period of thesystem is 94.83$\pm$0.05 d.

Asteroseismology of the heartbeat star KIC 5006817