Cicek, C.Bulut, A.Bulut, I2025-01-272025-01-272019978-0-7354-1925-40094-243Xhttps://doi.org/10.1063/1.5135471https://hdl.handle.net/20.500.12428/2795035th International Physics Congress of the Turkish-Physical-Society (TPS) -- SEP 04-08, 2019 -- Bodrum, TURKEYIn this study, the analysis of the Kepler light curve of the eclipsing binary KIC 10296163 (Gaia DR2 2085670964017513856, R.A.(2000) = 19(h)564(m)40(s).07, DEC2000 = +47(0) 21'21 ''.97, m(R) = 13.43 mag) is presented. The light curve of the system shows a secondary minimum from a shifted phase 0.5 which indicates the ellipticity of the orbit. By using the PHOEBE program we analysed the light curve to achieve the orbital parameters of the system. The results of our analysis indicates a detached system where the orbit is highly eccentric (e = 0.357 +/- 0.003). Therefore, KIC 11858541 is a suitable candidate for apsidal motion studies.eninfo:eu-repo/semantics/closedAccessConference Object217810.1063/1.5135471N/AWOS:0006188797000742-s2.0-85076469295Q4