On earth, the solar constant is approximately I = 1367 W/m2 . This corresponds to the power per unit area that a detector at the edge of the earth atmosphere would sense if perpendicular to the solar rays. This value can be obtained from the sun/earth geometry and by considering the sun as a blackbody at Tsun = 6000 K emitting radiation according to EEbb = σσTT 4 where σσ = 5.67 × 10−8 W m−2K−4. Earth distance to sun = 150 000 000 km Mars to sun distance = 230 000 000 km With the information above, compute the solar constant in Mars. No need to do the actual calculation; instead, simply describe the step(s) you would take to solve the problem and list the relevant equation(s)