C and D Trelequ1- Relating the production of energy in the Sun to its luminosity and determiningthe efficiency of nuclear reactionsa) Considering the fact that the global ppl-chain can be summarized as:4 ¹H+ → He++ + 2e+ + 2v + 2y + kinetic energyfollowed by: 2e+ + 2e → 4y-or, equivalently:4 H+ + 2e¯¯ → He++ + 2v + 6y + kinetic energydetermine the energy (in J) that results from this chain of reactions, including theenergy carried by gamma rays and by neutrinos.(show your steps with the determination of Am in u and then in kg, followed bythe conversion of Am into a AE)b) Consult your class notes to determine the amount of energy carried by the2 neutrinos produced in a ppl chain.c) Determine the number of H nuclei that need to be consumed every second topower the luminosity of the Sun (Lo = 3.828 x 1026 W)d) Convert the result found in c) in kg of hydrogen consumed per second.e) Use the result found in d) to estimate the Main Sequence lifetime of the Sun byassuming that it will consume about 10% of its total mass before running out of Hin its core. Express your result in seconds.f) Does the result found in e) make sense when you convert it into years?g) Determine the "efficiency" of the ppl chain by calculating the ratio(energy produced in J)/ (mass of fuel consumed in kg).h) Compare the efficiency found in g) to the efficiency of a typical chemical reactionsuch as the burning of graphite: C+02 → CO₂ + AE (AE=393.5 kJ/mol).100% efficiency9i) Determine the efficiency of the "annihilation" of a positron with an electron viathe reaction: et + e2y (taking the two gamma rays as the energy produced)metséj) Convert the results found in parts g) and h) into %, considering the % efficiency+of a reaction is 100% when all the matter is destroyed to be converted into energy(as is the case with et + e→ 2y).me

Question

C and D Trelequ1- Relating the production of energy in the Sun to its luminosity and determiningthe efficiency of nuclear reactionsa) Considering the fact that the global ppl-chain can be summarized as:4 ¹H+ → He++ + 2e+ + 2v + 2y + kinetic energyfollowed by: 2e+ + 2e → 4y-or, equivalently:4 H+ + 2e¯¯ → He++ + 2v + 6y + kinetic energydetermine the energy (in J) that results from this chain of reactions, including theenergy carried by gamma rays and by neutrinos.(show your steps with the determination of Am in u and then in kg, followed bythe conversion of Am into a AE)b) Consult your class notes to determine the amount of energy carried by the2 neutrinos produced in a ppl chain.c) Determine the number of H nuclei that need to be consumed every second topower the luminosity of the Sun (Lo = 3.828 x 1026 W)d) Convert the result found in c) in kg of hydrogen consumed per second.e) Use the result found in d) to estimate the Main Sequence lifetime of the Sun byassuming that it will consume about 10% of its total mass before running out of Hin its core. Express your result in seconds.f) Does the result found in e) make sense when you convert it into years?g) Determine the &#34;efficiency&#34; of the ppl chain by calculating the ratio(energy produced in J)/ (mass of fuel consumed in kg).h) Compare the efficiency found in g) to the efficiency of a typical chemical reactionsuch as the burning of graphite: C+02 → CO₂ + AE (AE=393.5 kJ/mol).100% efficiency9i) Determine the efficiency of the &#34;annihilation&#34; of a positron with an electron viathe reaction: et + e2y (taking the two gamma rays as the energy produced)metséj) Convert the results found in parts g) and h) into %, considering the % efficiency+of a reaction is 100% when all the matter is destroyed to be converted into energy(as is the case with et + e→ 2y).me

Accepted Answer

We are given  the luminosity of sun. This is the energy released per second by sun. We know that 4…