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Universe
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Author: Robert Geller, Roger Freedman, William J. Kaufmann
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Chapter 13, Problem 66Q
To determine

Escape speed on Titan and the value for limiting molecular mass of a gas, which can be retained under the effect of gravitational pull of Titan. Assume that the average atmospheric temperature on Titan is 95 K.

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Answer to Problem 66Q

Solution:

2.6 km/s, 2.05×1026 kg

Explanation of Solution

Given data:

The average atmospheric temperature is 95 K.

Formula used:

The formula of the escape velocity is as:

vescape=(2GMR)12

Here, vescape is the escape velocity on Titan, M is the mass of Titan, R is the radius of Titan, and G is the universal gravitational constant having value 6.67×1011 Nm2/kg2.

The requirement for the retention of gas is,

vescape>6(3kTm)12

Here, m is the atomic mass of the gas, T is the temperature of the Titan’s surface, μ is the molecular weight of the gas, and k is Boltzmann constant having value 1.38×1023 m2kg/s2K.

Explanation:

The diameter of Titan is 5150 km and the mass of Titan is 1.34×1023 kg.

Since, radius is half of the diameter, the radius of Titan is,

R=D2

Here, D is the diameter of Titan.

Substitute 5150 km for d.

r=5150 km2(1000 m1 km)=2575 km 

Recall the formula of the escape velocity.

vescape=(2GMR)12

Substitute 2575.5 km for R, 1.34×1023 kg for M and 6.67×1011 Nm2/kg2 for G.

vescape=(2(6.67×1011 Nm2/kg2)(1.34×1023 kg)2575 km)12=(1.79×10132575.5 km(1000 m1 km))12=(6966530.771)12=2.6×103 m/s

Further solve as,

vescape=2.6×103 m/s(1 km1000 m)=2.6 km/s

Recall the requirement for the retention of gas.

vescape>6(3kTm)12

Substitute 1.38×1023 m2kg/s2K for k, 95 K for and 2.6×103 m/s for vescape.

2.6×103 m/s>6(3(1.38×1023 m2kg/s2K)(95 K)m)122.6×103>6(3.933×1021m)12

Squaring both sides.

(2.63×103)2>36(3.933×1021m)m>1.416×10196.91×106m>2.05×1026 kg

Conclusion:

Therefore, the gas with molecular mass greater than 2.05×1026 kg is retained.

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Students have asked these similar questions
Assuming all other variables were earth based besides atmospheric pressure, calculate the temperature at which water would boil at sea level on Titan versus Earth? And explain why using molecular concepts. Consider the pressure of Earth’s atmosphere at sea level to be 1 atm and the pressure of Titan’s atmosphere at sea level to be 1.45 atm.    ps plz stop refusing my questions or im going to cancel this membership
Compare Titan to Rhea. Estimate the strength of surface gravity on Titan compared to the gravity on Titan. How does this affect the possibility of an atmosphere on each?  Use g=GM/R2  Titan Radius: 2,575 km, Mass: 2.31 x 1021 kg Rhea Radius: 764 km, Mass: 1.35 x 1023 kg
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