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We present new findings about KIC 8043961. We find the effective temperatures of the components as 6900± 200 K for the primary, and 6598± 200 K for the secondary, while the logarithm of the surface gravities are found to be 4.06 cm s−2 and 3.77 cm s−2, respectively. Combination of the light curve with the spectroscopic orbit model results leads to a mass ratio of 1.09 ± 0.07 with an orbital inclination of 73.71± 0.14 and a semi-major axis of 8.05± 0.22R . Masses of the primary and secondary components are calculated as 1.379 ± 0.109M and 1.513 ± 0.181M , while the radii are found to be 1.806± 0.084R and 2.611± 0.059R . In addition, we obtain a considerable light contribution (≈0.54%) of a third body. We compute a possible mass for the third body as 0.778± 0.002M . We find that the primary component exhibits γ Dor type pulsations with 137 frequencies.

γ DOR: A PULSATING COMPONENT OF KIC 8043961 IN A STELLAR TRIPLE SYSTEM