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Material Type: Exam; Class: Planetary Science; Subject: Earth Sciences; University: University of California-Santa Cruz; Term: Unknown 1989;
Typology: Exams
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Name four Solar system bodies that have dunes (2)
A 50km diameter crater has been extended by 1km due to normal faulting. If the Young’s modulus is 100 GPa, how big were the tectonic stresses? (2)
How long does it take a dike 5 km high and 2m thick to cool? (2)
Give two ways in which some extra-solar planets are very different from the giant planets in our solar system (2)
Give two reasons why big terrestrial planets tend to be hotter inside than small terrestrial planets (2)
Write down the orbital angular momentum of a satellite in terms of its mass m , orbital
a) Using the hydrostatic assumption and the ideal gas law, show that the variation of pressure in an isothermal atmosphere is given by P=P 0 exp (-z/H) , where P 0 is the surface pressure and H is the scale height (4)
c) Use your answer to b) to derive an expression for the total mass contained in a column
d) Now express your answer to c) in terms of P 0 and the gravity g (1) e) Write down an expression for the total mass of atmosphere contained on a planet in terms of P 0 , g and R , the radius of the planet (1) f) If this atmosphere is being heated by solar power S (in Watts), write down an expression for the time t it takes for the entire atmosphere to heat up by 1K in terms of P 0 ,g,R,S and Cp , the specific heat capacity of the gas (2) g) Describe how this time changes as P 0 and Cp change, and explain why these effects make physical sense (2) g) For the Earth, we have P 0 =10^5 Pa, g =10 ms-2, R =6400 km, S =3x10^17 W, Cp =300 Jkg- K-1. What is the time t? (1) (15 total)
Here we’re going to consider a planet with a variable density distribution.
contained inside a radius r (3)
c) Using your answer to a), find the gravity g at a radius r. What is unusual about g? (2) d) Using the hydrostatic assumption, find the general solution for the pressure P(r) inside the planet (4) e) Using the boundary condition that P=0 at r=R , find the particular solution for P(r) , the pressure inside the planet (2) f) What happens at the origin and why? (1)
planet of constant density (2) (15 total)
Here we’ll consider the temperature distribution inside a planet. The general expression for a one-dimensional steady-state conductive temperature distribution T(z) with internal heating is
2 0
2 C p
dz
d T
a) Here we’re going to assume that internal heating is variable, so that H(z)=H 0 exp (-z/d) where H 0 is the heat production rate at the surface and d has the units of distance. Sketch how H varies as a function of z , showing what d represents (1). b) By integrating equation (1) twice, find the general solution for T(z) when the heating rate H(z)=H 0 exp (-z/d) (3) c) One boundary condition is that at the surface T=Ts , where Ts is a constant. Use this fact to determine one of the unknown constants in your answer to b). (1) d) The second boundary condition is that the temperature gradient dT/dz =0 as z gets very large. Use this fact to determine the other unknown constant in your answer to b) (2). e) Hence write down the particular solution to T(z) for these two boundary conditions (1). f) Also write down an expression for the temperature as z gets very large (1) g) Explain why your answer to f) makes physical sense in terms of how it depends on d ,
h) Use your answer to e) to write down an expression for the heat flux at the surface (2) i) Does your answer to h) make sense? (1) (15 total)