Radiation pressure is given by $\text{P}_\text{R}=\frac{(1+\alpha)\text{I}}{\text{C}}$
where α is the coefficient of reflection of the surface.
For completely reflecting surface $\alpha=1$
For completely absorbing surface $\alpha=0$
So, radiation pressure depends on the nature of surface on which the light is falling but independent of wavelength of light falling.
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$(A)$ Fusion of two nuclei with mass numbers lying in the range of $1 < \mathrm{A} < 50$ will release energy
$(B)$ Fusion of two nuclei with mass numbers lying in the range of $51 < \mathrm{A} < 100$ will release energy
$(C)$ Fission of a nucleus lying in the mass range of $100 < \mathrm{A} < 200$ will release energy when broken into two equal fragments
$(D)$ Fission of a nucleus lying in the mass range of $200 < \mathrm{A} < 260$ will release energy when broken into two equal fragments
