Gravitational redshift is given by the following approximate equation
where λ is the is the shifted wavelength, λ0 is the rest wavelength, G is the gravitational constant, and r is the distance from the gravitating body with mass M, c is the speed of light
Using (1) we got:
In our case, 2MΘ=2×1.98892×1030 kg, r=2 m
We got: λ=881.4×10-6 m
Answer:
881.4×10-6 m
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