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We measured the photometric flux of the cataclysmic variable TT Arietis(BD+14 341) using the MOST space telescope. Periodic oscillations of the fluxreveal the orbital period as well as other features of this binary system. Weapplied a Discrete Fourier Transform (DFT) on a reduced dataset to retrieve thefrequencies of TT Arietis. The analysis of the system revealed a photometricperiod of 3.19 hours. Though the MOST data has a high cadence of 52.8 seconds,a fine structure of the accretion disk is not obvious.

TT Arietis - Observations of a Cataclysmic Variable Star with the MOST Space Telescope