I have a question in an assignment that says "Estimate the central pressure of 0.5, 1.0, and50 solar mass stars. Compare these pressures to the central pressure of the sun"
I can estimate for the sun using the Hydrostatic equilibrium equation:
dP/dr = -GM(r)p(r)/R^2...
Hello,
I was given a question in school that says use the hydrostatic equilibrium equation and mass conservation equation to come up with a lower limit of the central pressure of a star at it's centre. Here is how I think:
1) Refer to the density in both equations as the same and sub...