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For 759 exoplanets detected by radial velocities method we found that distances of  exoplanets from central star comply in general Schmidt law and these distances depend on  the stellar surface temperature. Every stellar spectral class has a little different  distribution. The Luminosity and the Irradiance has not effect on the distribution of  distances of exoplanets. We have found the new formulas for calculation of effective  temperature of exoplanets for spectral classes F, G, and K. These new formulas we can use  for future calculation of habitable planets

Relationship between Luminosity, Irradiance and Temperature of star on the orbital parameters of exoplanets