A group of stars is observed through several different filters, and some stars are seen to be brightest when observed through either the $V(500-590 \mathrm{nm})$ or $\mathrm{R}(570-710 \mathrm{nm})$ filter.
a. Assuming a star is brightest in the middle of the $\mathrm{R}$ filter, use Wien's law (Unit 23.4 ) to estimate its temperature.
b. If a star is brightest through the $V$ filter, use Wien's law to estimate the range of temperatures it might have.