A star converts all its hydrogen to helium, achieving a 100% helium composition. Next, it converts the helium to carbon via the triple-alpha process,

H4e+H4e+H4e12C+7.27MeV

The mass of the star is role="math" localid="1661754478822" 4.6×1032kg, and it generates energy at the rate of 5.3x103W. How long will it take to convert all the helium to carbon at this rate?

Short Answer

Expert verified

The required time is 1.6×108yr.

Step by step solution

01

Describe the expression for the time

Let m be the mass of helium, the number of three-helium atoms in this mass equals the number of moles multiplied by the number of atoms in one mole, where the number of moles equals the mass divided by three the molar mass of the helium.

N3He=mHeNA3MHe

Let be the energy release per fusion, then the total energy released by fusion equals the number of fusions multiplied by N3He.

Efusion=N3HeQ=mHeNAQ3MHe

The energy also can be written as follows:

Efusion=PtmHeNAQ3MHe=Ptt=mHeNAQ3MHeP

02

Find the time required to convert all the helium to carbon

Substitute all the known values in equation (1).

t=4.6×1035g6.022×1023mol-17.27MeV1.602×10-13J/MeV34.0g/mol5.3×1030W=5.07×1015s=5.07×1015s3.154×107s/yr=1.6×108yr

Therefore, the required time is 1.6×108yr.

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The effective Q for the proton–proton cycle of Fig. 43-11 is 26.2 MeV. (a) Express this as energy per kilogram of hydrogen consumed. (b) The power of the Sun is 3.9x1026W. If its energy derives from the proton–proton cycle, at what rate is it losing hydrogen? (c) At what rate is it losing mass? (d) Account for the difference in the results for (b) and (c). (e) The mass of the Sun is 2.0x1030kg. If it loses mass at the constant rate calculated in (c), how long will it take to lose 0.10% of its mass?

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