Answer:
[tex]L_A = 9 L_B[/tex]
Explanation:
The formula that relates the luminosity of a star (L) to its radius (R) and the temperature (T) is
[tex]L=\frac{R^2}{T^4}[/tex]
For star B, we can write:
[tex]L_B=\frac{R_B^2}{T_B^4}[/tex]
For star A, we have
[tex]T_A = 2 T_B\\R_A = 12 R_B[/tex]
So the luminosity of star A is
[tex]L_A=\frac{R_A^2}{T_A^4}=\frac{(12 R_B)^2}{(2 T_B)^4}=\frac{144 R_B^2}{16 T_B^4}=9\frac{R_B^2}{T_B^4}=9 L_B[/tex]