(a) Luminosity of a star depends upon the total radiations emitted by the star.
The star emits 17000 times the radiations emitted by the sun.
$\therefore$ $E = \sigma T^{4}$
Hence, $\frac{E_{1}}{E} = \left( \frac{T_{1}}{T} \right)^{4}$
So, $(17000)^{\frac{1}{4}} = \frac{T_{1}}{T}$ (Given, $E_{1} = 17000E)$
${\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ T}_{1} = 6000 \times 11.4 = 68400\ K$