Final answer:
Using Wien's Law and the given peak wavelength of 300 nm, we can calculate the surface temperature of a white dwarf to be approximately 9700 K, which matches closest with option B) 9700 K.
Step-by-step explanation:
To determine the surface temperature of a white dwarf based on its peak wavelength, we can use Wien's Law. Wien's Law gives a relationship between the temperature of a star and the wavelength at which it emits the most energy. The formula for Wien's Law can be expressed as λ_max * T = b, where λ_max is the peak wavelength, T is the temperature in Kelvin, and b is Wien's displacement constant, approximately equal to 2.897 x 10^(-3) meter*Kelvin.
Given the peak wavelength λ_max of 300 nm (or 300 x 10^(-9) meters) for the white dwarf, we can rearrange Wien's Law to solve for the temperature (T):
T = b / λ_max
Substituting the known values,
T = (2.897 x 10^(-3) m*K) / (300 x 10^(-9) m)
T = 9,656.67 K
Looking at the choices provided, the surface temperature of the white dwarf that most closely matches our calculation is option B) 9700 K.