Pressure Gradient in Hydrostatic Equilibrium

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SUMMARY

The discussion focuses on deriving the relationship between gas pressure and height in an isothermal atmosphere under hydrostatic equilibrium. The key equation used is the pressure gradient equation, dP/dr = -gρ, where g is the constant gravitational acceleration. The solution reveals that gas pressure decreases exponentially with height, confirmed by manipulating the ideal gas law to relate number density and pressure. The final expression for pressure as a function of height is derived from the number density relationship.

PREREQUISITES
  • Understanding of hydrostatic equilibrium principles
  • Familiarity with the ideal gas law
  • Basic knowledge of differential equations
  • Concept of isothermal processes in thermodynamics
NEXT STEPS
  • Study the derivation of the ideal gas law and its applications
  • Learn about differential equations in physical contexts
  • Explore the concept of isothermal processes in greater detail
  • Investigate the implications of hydrostatic equilibrium in astrophysics
USEFUL FOR

Students studying atmospheric physics, meteorologists, and anyone interested in the principles of hydrostatic equilibrium and gas behavior in an isothermal atmosphere.

SHISHKABOB
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Homework Statement


Consider an isothermal atmosphere (T = const.) over a sufficiently small range of radii, so that you can assume that the gravitation acceleration g is constant. Use the equation for the gas pressure gradient in hydrostatic equilibrium to show that the gas pressure decreases exponentially with height.


Homework Equations



\frac{dP}{dr} = -g\rho


The Attempt at a Solution



so I solve the differential equation for P and I get

P = -\rho gr = \frac{-GM\rho}{r}

I think I'm doing something really dumb here...
 
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Hi Shishkabob! :biggrin:

You need to re-check solving your differential equation. Is the density independent of pressure? Can you simply use it as a constant??

(Hint : Think about manipulating the ideal gas equation to form a relation)
 
oh okay, thanks for the tip. I found a relationship between the number density of the gas and the pressure, and so I had a differential equation that was dn/dr. Which I solved for the number density as a function of r and then just resubstituted stuff in for pressure.
 

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