4. Given a value for Mars’ radius of 3400 km, an albedo of Mars of 0.15, and Mars’ distance from the Sun of 1.52 AU, then:
a. determine the power, Psq.m, of the radiation from the Sun flowing through and area of 1 m2 facing the Sun with the area located at a distance of Mars from the Sun of 0.72 AU.
b. What power, Pabs, is absorbed by Mars?
c. What would mars’ surface temperature, T, be, assuming that Mars radiated into space an amount, Pem , that is equal to the power it absorbed?
d. What is the mean temperature on Mars, how much is it different from the temperature you computed in c) and what is the reason for the difference (if the difference is large)?
4. Given a value for Mars’ radius of 3400 km, an albedo of Mars of 0.15,...
I can see here that for question B Stefan–Boltzmann law was used. However, the energy per unit area is being divided per 4. why? The ratio distance of Mars from the Sun 1.5 6. distance of Earth from the Sun (a) Show that the intensity of solar radiation at the orbit of Mars is about 600 W m2 (b) Determine, in K, the mean surface temperature of Mars. Assume that Mars acts as a black body. 121 (c) The atmosphere...
Atpherical object with a radius r = 1.1x107m and mass mis in equilibrium at a distance d = 1.1x10m from a star due to the cancellation of gravitational and radiation forces. Let M..4.810 kg be the mass of the star, and P. -3.410 W be the total average power radiated by it uniformly in all directions. You will also need the gravitational constant G.6.7x10-"Nm /kg) and the speed of light - 3x10 m/s in the following questions Part A What...