21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 5, Problem 44QP
To determine

The average temperature of Eris when it is farthest from the Sun.

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Saturn is even further at 1434X109m from the sun.  Calculate the approximate strength of the greenhouse effect on Jupiter.  The observed surface temperature is 133K, the albedo is 0.47, the solar constant is 15W/m2.
Which of these things did the Voyager spacecraft discover about Enceladus in the early 1980s, indicating that it is somewhat unusual among planetary bodies in our solar system? Check the TWO items that apply.   a It has a thick atmosphere, made mostly of nitrogen. b It has the darkest, least reflective surface of all the known planetary bodies. c It is the brightest (i.e. most reflective) object in the solar system. d The entire surface is more heavily-cratered than any other body in our solar system. e Its surface is very smooth in some places.
The fraction of the energy flux received which is reflected into space is the albedo of Venus, av, which is about 0.76.  The fraction of the energy flux which is absorbed is then (1-av) = 1. - 0.76 = 0.24.  So the amount of energy actually absorbed by Venus in each second is Lv = (1-av)Ev. Lv = (1-av)Ev = ___________________ ergs/s And next calculate the effective temperature of Venus: Tv4 = (Lv/(4pdv2))/s   =    Lv/(4spdv2)  = __________________ K4 and taking the square root of Tv4 twice in succession we get the effective Temperature Tv: Tv  = [Lv/(4spdv2)]0.25  =  _________________ K Calculate Venus' emittance assuming that the Venus' actual temperature, Tvr, is 472o C  =  745 K:  ev = Lv/(4pdv2s Tvr4)   =  __________________ .
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