A portion of the Sun’s energy comes from the reaction4 11H----->42He + 2 01ewhich requires a temperature of 106 to 107 K. Use the massof the helium-4 nucleus given in Table to determinehow much energy is released per mol of hydrogen atoms. Mass of Nucleus(amu)4.00150Mass of IndividualNucleons (amu)4.03188Mass Defect(amu)BindingEnergy (J)4.53 x 10-12Binding Energyper Nucleon (J)1.13 x 10-12NucleusНе0.0303855.920687.90 x 10-112.89 x 10-101.41 x 10-121.21 x 10 1256.449140.52846Fe238.00031239.934511.93420

Here the nuclear reaction is 4 11H→ 24He + 2 10e To calculate the amount of energy is released…

Answered: Mass of Nucleus (amu) 4.00150 Mass of…

Chemistry

10th Edition

ISBN:9781305957404

Author:Steven S. Zumdahl, Susan A. Zumdahl, Donald J. DeCoste

Publisher:Steven S. Zumdahl, Susan A. Zumdahl, Donald J. DeCoste

Chapter1: Chemical Foundations

Section: Chapter Questions

Problem 1RQ: Define and explain the differences between the following terms. a. law and theory b. theory and...

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Question

A portion of the Sun’s energy comes from the reaction
⁴ ₁₁H----->⁴₂He + 2 ⁰₁e
which requires a temperature of 10⁶ to 10⁷ K. Use the mass
of the helium-4 nucleus given in Table to determine
how much energy is released per mol of hydrogen atoms.

Mass of Nucleus
(amu)
4.00150
Mass of Individual
Nucleons (amu)
4.03188
Mass Defect
(amu)
Binding
Energy (J)
4.53 x 10-12
Binding Energy
per Nucleon (J)
1.13 x 10-12
Nucleus
Не
0.03038
55.92068
7.90 x 10-11
2.89 x 10-10
1.41 x 10-12
1.21 x 10 12
56.44914
0.52846
Fe
238.00031
239.93451
1.93420

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