154 Problems €4 Sdutio~ on Thermodynom'ca €4 Statiaticd Mechanics
dz dz dz
dt dt dt
is pL-. Hence we obtain the equation pL- = -j, giving q = - =
-j/pL = n(T - To)/pLz.
(b) The above expression can be written as
dt = pL zdz.
n(T - To)
t = pL(~i - zf)/2n(T - To).
If we take z1 = 1 cm and 22 = 2 cm, then At = 1.2 x lo3 s = 20 min.
1156
Consider a spherical black asteroid (made of rock) which has been
ejected from the solar system, so that the radiation from the sun no longer
has a significant effect on the temperature of the asteroid. Radioactive ele-
ments produce heat uniformly inside the asteroid at a rate of q = 3 x
cal/g.sec. The density of the rock is p = 3.5 g/cm3, and the thermal con-
ductivity is k = 5 x The radius of the asteroid is
R = 100 km. Determine the central temperature T, and the surface tem-
perature T,, of the asteroid assuming that a steady state has been achieved.
(UC, Berkeley)
cal/deg.cmsec.
Solution:
The surface temperature satisfies
4rR3
4rR20T,4 = Q = - 3 PQ 1
80
T, = (z)' = 22.5 K.
The equation of heat conduction inside the asteroid is
V. (-kVT) = Qp.
Using spherical coordinates, we have