Skip to main content
Ch.21 - Nuclear Chemistry
Chapter 21, Problem 54

The isotope 6228Ni has the largest binding energy per nucleon of any isotope. Calculate this value from the atomic mass of nickel-62 (61.928345 amu) and compare it with the value given for iron-56 in Table 21.7.

Verified step by step guidance
1
Step 1: Understand the concept of binding energy per nucleon. Binding energy is the energy required to disassemble a nucleus into its component protons and neutrons. The binding energy per nucleon is the total binding energy divided by the number of nucleons in the nucleus.
Step 2: Calculate the mass defect for nickel-62. The mass defect is the difference between the mass of the completely separated nucleons and the mass of the nucleus. Use the formula: \( \Delta m = Zm_p + Nm_n - m_{\text{nucleus}} \), where \( Z \) is the number of protons, \( N \) is the number of neutrons, \( m_p \) is the mass of a proton, \( m_n \) is the mass of a neutron, and \( m_{\text{nucleus}} \) is the atomic mass of the isotope.
Step 3: Convert the mass defect from atomic mass units (amu) to energy using Einstein’s equation \( E = \Delta mc^2 \), where \( c \) is the speed of light. Note that 1 amu is equivalent to 931.5 MeV/c^2.
Step 4: Calculate the binding energy per nucleon by dividing the total binding energy by the number of nucleons in nickel-62. The number of nucleons is the sum of protons and neutrons, which is 62 for nickel-62.
Step 5: Compare the calculated binding energy per nucleon for nickel-62 with the value given for iron-56 in Table 21.7. This comparison will help you understand why nickel-62 has the largest binding energy per nucleon.
Related Practice
Textbook Question

The atomic masses of nitrogen-14, titanium-48, and xenon-129 are 13.999234 amu, 47.935878 amu, and 128.904779 amu, respectively. For each isotope, calculate (a) the nuclear mass.

653
views
Open Question
The energy from solar radiation falling on Earth is 1.07 * 10^16 kJ/min. (a) How much loss of mass from the Sun occurs in one day from just the energy falling on Earth? (b) If the energy released in the reaction 235U + 10n → 14156Ba + 9236Kr + 310n (235U nuclear mass, 234.9935 amu; 141Ba nuclear mass, 140.8833 amu; 92Kr nuclear mass, 91.9021 amu) is taken as typical of that occurring in a nuclear reactor, what mass of uranium-235 is required to equal 0.10% of the solar energy that falls on Earth in 1.0 day?
Textbook Question

Based on the following atomic mass values: 1H, 1.00782 amu; 2H, 2.01410 amu; 3H, 3.01605 amu; 3He, 3.01603 amu; 4He, 4.00260 amu—and the mass of the neutron given in the text, calculate the energy released per mole in each of the following nuclear reactions, all of which are possibilities for a controlled fusion process:

(a) 21H + 31H → 42He + 10n

(b) 21H + 21H → 32He + 10n

(c) 21H + 32He → 42He + 11H

731
views
Textbook Question

Iodine-131 is a convenient radioisotope to monitor thyroid activity in humans. It is a beta emitter with a half-life of 8.02 days. The thyroid is the only gland in the body that uses iodine. A person undergoing a test of thyroid activity drinks a solution of NaI, in which only a small fraction of the iodide is radioactive. (c) A normal thyroid will take up about 12% of the ingested iodide in a few hours. How long will it take for the radioactive iodide taken up and held by the thyroid to decay to 0.01% of the original amount?

890
views
Textbook Question

Why is it important that radioisotopes used as diagnostic tools in nuclear medicine produce gamma radiation when they decay? Why are alpha emitters not used as diagnostic tools?

672
views
Open Question
(a) Which of the following are required characteristics of an isotope to be used as a fuel in a nuclear power reactor? (i) It must emit gamma radiation. (ii) On decay, it must release two or more neutrons. (iii) It must have a half-life of less than one hour. (iv) It must undergo fission upon the absorption of a neutron. (b) What is the most common fissionable isotope in a commercial nuclear power reactor?