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We present the photometric study of an interesting target in the CoRoT exoplanet database: CoRoT 310266512. Its light curve shows primary, secondary and tertiary eclipses that suggests the presence of at least three celestial bodies. The primary and secondary eclipses have the same orbital period, 7.42 days, and the tertiary eclipse has an orbital period of 3.27 days. Two of the tertiary eclipses fall within a primary eclipse and a secondary eclipse. The properties of the light curve indicate the presence of two physically separated systems. The primary and secondary eclipses corresponds to a binary system (System I). The tertiary eclipses correspond to a star-planet system or a star-dwarf system (System II). Some parameters of these two systems are obtained from JKTEBOP [1] program

Corot 310266512: A Light Curve With Primary, Secondary And Tertiary Eclipses