Question 1 Sun’s central temperature: Use the equation of state to find the central temperature of the Sun. The mean molecular mass for the Sun is 0.6.
We have equation of state
where PC central pressure of earth so we can write
where TC = central temperature of earth.
now we have PC=
m=mproton/2=0.84*10-27 kg
constant density
WHERE R =696,340 km PUTTING VALUE WE GET
density of su as 1.41 g/cm³ now by putting all value in above equation we get
TC 1.2*107 k
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