Q 1628045801.     Two spherical stars `A` and `B` emit blackbody radiation. The radius of `A` is `400` times that of `B` and `A` emits `10^4` times the power emitted from `B`. The ratio ` ( \frac{\lambda_A}{\lambda_B} )` of their wavelengths `\lambda_A` and `\lambda_B` at which the peaks occur in their respective radiation curves is

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