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- The next four questions use this description. Our Sun has a peak emission wavelength of about 500 nm and a radius of about 700,000 km. Your dark-adapted eye has a pupil diameter of about 7 mm and can detect light intensity down to about 1.5 x 10-11 W/m2. Assume the emissivity of the Sun is equal to 1. First, given these numbers, what is the surface temperature of the Sun in Kelvin to 3 significant digits? What is the power output of the Sun in moles of watts? (in other words, take the number of watts and divide it by Avogadro's number) Assuming that all of the Sun's power is given off as 500 nm photons*, how many photons are given off by the Sun every second? Report your answer to the nearest power of 10 (e.g. if you got 7 x 1024, give your answer as 25).(12.1) In an adiabatic expansion of an ideal gas, pV is constant. Show also that TV7-1 = constant, (12.22) T = constant x p¹-1/. (12.23)In a Gas Law Experiment, when the volume is doubled and absolute temperature of a fixed amount of gas is halved, the pressure of the gas is … (choose a, b, c or d as answer) (a) one-fourth of the original pressure (b) half of the original pressure (c) the same as the original pressure (d) double the original pressure. Explain your choice.