Our Sun emits most of its radiation at a wavelength of 550nm. If a star were 5.00 times hotter than our Sun, it would emit most of its radiation at a wavelength of nm 1st attempt Feedback Q See Hint Our Sun emits most of its radiation at a wavelength of 550 nm. If a star were 5.00 times hotter than our Sun, it would emit most of its radiation at a wavelength of 275 nm

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Answer:

[tex]\lambda_{star} = 1.100\times 10^{-7} meter[/tex]

Explanation:

By wein's law

[tex]\lambda\times T= 2.898\times 10^{-3} kelvin meter[/tex]

where;

λ = wavelenght

T= Temperature (in kelvin)

[tex]2.898\times 10^{-3} mk[/tex] = Wein's constant

so

[tex]\lambda\times  T(sun) = 2.898\times 10^{-3}[/tex]

[tex]550\times 10^{-9}\times T (sun) = 2.898\times 10^{-3}[/tex]

[tex]T (sun) = \frac{2.898\times 10^{-3}}{ 550\times 10 ^{-9}}[/tex]

T (sun) = 5269.09 kelvin

from data given we have

[tex] T( star ) = 5\times T (sun)[/tex]

so,

[tex]\lambda_{star}\times  T(star) = 2.898\times 10^{-3}[/tex]

[tex]\lambda_{star}\times 5\times T(sun) = 2.898\times 10^{-3}kelvin meter[/tex]

[tex]\lambda_{star}\times 5\times 5269.09 = 2.898\times 10^{-3}kelvin meter[/tex]

[tex]\lambda_{star} = \frac{(2.898\times 10^{-3}kelvin meter)}{(5 \times 5.269 \times 10^{3}kelvin)}[/tex]

[tex]\lambda_{star} = 1.100\times 10^{-7} meter[/tex]