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The astrophysical S-factor for the process p7Be --> 8Bgamma of radiativecapture by the 8B ground state is described up to 5 MeV, within the modifiedpotential cluster model. The signatures of the S-factor resonances at 0.632,2.18 and 3.36 MeV due to M1 and E2 transitions from the scattering of resonance3P1, 3F3 and 3D2 waves to the ground 3P2 state are illuminated using totalcross sections, astrophysical S-factors and reaction rates at temperatures from0.01 to 10.0 T9. Experimental data on the S-factor are reproduced well in therange 100 keV to 3 MeV. The importance of the input of the 0.632 MeV resonanceto the reaction rate is proved. Our calculations (performed in advance) confirmthe latest data for the S-factor at 19 keV.

New Results for the p7Be-->8Bgamma Astrophysical S-factor from 10 keV to 5 MeV and Reactions Rate from 0.01 to 10 T9