Calculating Energy Released Per Proton & Mass Converted to Energy/sec

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SUMMARY

The discussion focuses on calculating the energy released per proton during nuclear fusion in the Sun, specifically through the proton-proton chain reaction. The energy released per proton is established as 6.55 MeV, leading to the conclusion that approximately 4.3 x 10^9 kg of mass is converted to energy every second, based on the Sun's luminosity of 3.826 x 10^26 W. The calculations involve using the famous equation E = mc² to relate energy output to mass conversion.

PREREQUISITES
  • Understanding of nuclear fusion processes, specifically the proton-proton chain reaction.
  • Familiarity with energy units, particularly MeV and Joules.
  • Knowledge of Einstein's mass-energy equivalence principle (E = mc²).
  • Basic grasp of astrophysical concepts, particularly solar luminosity and its implications.
NEXT STEPS
  • Research the detailed mechanics of the proton-proton chain reaction in stellar environments.
  • Learn about the conversion of MeV to Joules and how to apply it in energy calculations.
  • Explore the implications of mass-energy conversion in astrophysics, particularly in stellar evolution.
  • Investigate the role of neutrinos in nuclear reactions and their impact on energy calculations.
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Astrophysicists, students studying nuclear physics, and anyone interested in understanding the energy production mechanisms of stars, particularly the Sun.

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H1 means hydrogen with mass 1, H2 means hydrogen with mass 2 (has a neutron), etc


1) H1 + H1 -> H2 + positron + neutrino + 1.18 Mev (+0.26MeV)
2) H1 + H2 -> He3 + photon + 5.49MeV
3) He3 + He3 -> He4 + 2*H1 + 12.86 MeV

(The neutrino produced in 1 for all practical purposes do not interact with matter, so their energy can be ignored (neutrino energy 0.26MeV)

Using the above 3 equations, calculate the energy released per proton. Note that the equations must be properly combined in order to find the overall reaction! Given the sun's luminosity calculate the amount of hydrogen converted to helium every second. How much mass per second is converted directly to energy?


Homework Equations


sun's luminosity: 3.826*10^26 W

answers: 6.55 MeV, 6.2*10^11 kg, 4.3x10^9 kg.

The Attempt at a Solution



I have shown each proton has released 6.55 MeV. but how do i calculate the amount of hydrogen converted to helium every second?
 
Last edited:
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(I removed part of my reply, since I missed at first where you said you'd gotten the 6.55 MeV per proton.)

Having gotten that answer, you have the energy release (in MeV) from one pp-reaction. Given what the luminosity (power output) of the Sun is, how many of these reactions would be needed per second? How many protons cease to exist as individuals and become groups of four in nuclei every second? How much mass is that?

Last question -- Since you have the Sun's luminosity, what mass is that energy equivalent to (that will take you from, say, Joules per second to kg/sec)? What famous equation might you use?
 
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part c I've got, directly using E = mc² gives 4.3*10^9 kg

but i still have trouble with part b :(

Luminosity of sun is 3.826*10^26 W which is 3.826*10^26 J/s
6.55 MeV = 1.049 * 10^-12 protons/J .
 
Last edited:
Qyzren said:
i still have trouble with part b :(

Luminosity of sun is 3.826*10^26 W which is 3.826*10^26 J/s
6.55 MeV = 1.049 * 10^-12 J/proton .
so if you divide it you can get 3.64*10^38 J/proton...
Watch your units: that division gives you 3.64·10^38 protons/sec. What mass does that many protons have?

just using E = mc2 to convert J to kg won't get me the answer of 6.2*10^11 kg :(

That equation is for finding the mass-equivalent of the 3.826·10^26 J/sec, which is the answer for the third question.
 

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