We have
"M_1=3^m"
"R_1=72"
"M_2=8^m"
"R_2=6"
Record the luminosities of each star
"L_1=4\\pi R_1^{2}\\sigma T_1^{4}"
"L_2=4\\pi R_2^{2}\\sigma T_2^{4}"
We apply the Pogson formula
"\\frac{L_2}{L_1}=2.512^{M_1-M_2}"
Substitute luminosities
"\\frac{4\\pi R_2^{2}\\sigma T_2^{4}}{4\\pi R_1^{2}\\sigma T_1^{4}}=2.512^{M_1-M_2}"
Simplify the expression
"\\frac{ R_2^{2} T_2^{4}}{R_1^{2}T_1^{4}}=2.512^{3-8}"
"\\frac{ R_2^{2} T_2^{4}}{R_1^{2}T_1^{4}}=2.512^{-5}=0.01"
Where will we write
"\\frac{ T_2}{T_1}=\\sqrt[4]{0.01 \\cdot \\frac{R_1^{2}}{R_2^{2}}}"
"\\frac{ T_2}{T_1}=\\sqrt[4]{0.01 \\cdot \\frac{72^{2}}{6^{2}}}=\\sqrt[4]{0.01 \\cdot 144}=1.095"
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