We propose a new method to use the kinematic Sunyaev-Zeldovich for measuring the baryon fraction in cluster of galaxies .
In this proposal we need a configuration in which a supernova Type Ia resides in a brightest cluster galaxy of intermediate redshift clusters .
We show this supernova Type Ia can be used to measure the bulk velocity of a galaxy cluster .
We assert that the redshift range of 0.4 < z < 0.6 is suitable for this proposal .
The main contribution to the deviation of standard candles distance modulus from cosmological background prediction in this redshift range comes from peculiar velocity of the host galaxy and gravitational lensing .
In this work we argue that by the knowledge of the bulk flow of the galaxy cluster and the cosmic microwave background photons temperature change due to kinematic Sunyaev-Zeldovich , we can constrain the baryon fraction of galaxy cluster .
The probability of this configuration for clusters is obtained .
We estimate in a conservative parameter estimation the large synoptic survey telescope can find spectroscopically followed \sim 4500 galaxy clusters with a bright cluster galaxy which hosts a type Ia Supernova each year .
Finally , we show the improving of the distance modulus measurement is the key improvement in future surveys which will be crucial to detect the baryon fraction of cluster with the proposed method .