The time "t" may be obtained as
"t = \\dfrac{S}{v}" , where "S" is the distance between the Sun and Earth and "v" is the velocity of light. Therefore,
"t = \\dfrac{1.5\\cdot10^8\\cdot10^3\\,\\mathrm{m}}{3\\cdot10^8\\,\\mathrm{m\/s}} = 500\\,\\mathrm{s} = 8.3\\,\\mathrm{min}."
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