47. (a) Estimate the total power radiated into space by the Sun, assuming it to be a perfect emitter at T = 5500 K. The Sun's radius is 7.0 × 10³ m. (b) From this, determine the power per unit area arriving at the Earth, 1.5 × 101 m away (Fig. 14–20). r = 1.5 x 1011 m FIGURE 14-20 Sun Earth Problem 47.
47. (a) Estimate the total power radiated into space by the Sun, assuming it to be a perfect emitter at T = 5500 K. The Sun's radius is 7.0 × 10³ m. (b) From this, determine the power per unit area arriving at the Earth, 1.5 × 101 m away (Fig. 14–20). r = 1.5 x 1011 m FIGURE 14-20 Sun Earth Problem 47.
Physics for Scientists and Engineers: Foundations and Connections
1st Edition
ISBN:9781133939146
Author:Katz, Debora M.
Publisher:Katz, Debora M.
Chapter21: Heat And The First Law Of Thermodynamics
Section: Chapter Questions
Problem 62PQ
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