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How much energy must be supplied to break a single \({ }^{21} \mathrm{Ne}\) nucleus into separated protons and neutrons if the nucleus has a mass of \(20.98846\) amu? What is the nuclear binding energy for \(1 \mathrm{~mol}\) of \({ }^{21} \mathrm{Ne}\) ?

Short Answer

Expert verified
The energy required to break a single Ne-21 nucleus into separated protons and neutrons is \(5.3425 \times 10^{-12} J\), and the nuclear binding energy for 1 mol of Ne-21 is \(3.216 \times 10^{12} J\).

Step by step solution

01

Calculate the binding energy of Ne-21 nucleus

First, we need to calculate the mass defect of the nucleus. Mass defect is the difference between the mass of the nucleus and the sum of the masses of its constituent protons and neutrons. Ne-21 has 10 protons and 11 neutrons. Mass of a proton is 1.00728 amu and that of a neutron is 1.00867 amu. Mass of 10 protons = 10 × 1.00728 amu = 10.0728 amu Mass of 11 neutrons = 11 × 1.00867 amu = 11.09537 amu Total mass of protons and neutrons = 10.0728 amu + 11.09537 amu = 21.16817 amu Now, we need to find the mass defect: Mass defect = Total mass of protons and neutrons - Mass of Ne-21 nucleus Mass defect = 21.16817 amu - 20.98846 amu = 0.17971 amu Now, calculate the binding energy for the Ne-21 nucleus: Binding energy (per nucleus) = Mass defect × (1 amu in kg) × (speed of light)^2 The mass of 1 amu in kg is approximately 1.6605 × 10^{-27} kg, and the speed of light is 2.9979 × 10^{8} m/s. Binding energy (per nucleus) = 0.17971 amu × 1.6605 × 10^{-27} kg/amu × (2.9979 × 10^{8} m/s)^{2} Binding energy (per nucleus) = 5.3425 × 10^{-12} J
02

Calculate the nuclear binding energy for 1 mol of Ne-21

Since there are 6.022 × 10^{23} atoms in 1 mol, we now calculate the binding energy for 1 mol of Ne-21: Binding energy (per mol) = Binding energy (per nucleus) × Avogadro's Number Binding energy (per mol) = 5.3425 × 10^{-12} J × 6.022 × 10^{23} Binding energy (per mol) = 3.216 × 10^{12} J So, the nuclear binding energy for 1 mol of Ne-21 is 3.216 × 10^{12} J.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Mass Defect
In the realm of nuclear physics, 'mass defect' is a fundamental phenomenon that refers to the discrepancy between the calculated mass of an atomic nucleus and the sum of the masses of its individual protons and neutrons. When protons and neutrons come together to form a nucleus, the total mass of the nucleus is found to be less than the sum of its parts. This 'missing' mass is actually converted into energy, which is then used to hold the nucleus together; this energy is known as the binding energy.

To put it simply, during the nuclear formation, some mass is transformed into energy following Einstein’s famous equation, \( E = mc^2 \) where \( E \) stands for energy, \( m \) for mass, and \( c \) the speed of light in a vacuum. In the case of \( {}^{21}Ne \) given in the exercise, students are challenged to calculate the mass defect by subtracting the atomic mass unit (amu) of the nucleus from the combined mass of the individual protons and neutrons. Understanding mass defect is crucial for students to comprehend the concept of nuclear stability and the forces at play within an atom's core.
Nuclear Physics
Nuclear physics is the branch of physics that studies the constituents and interactions of atomic nuclei. It encompasses a variety of concepts, including the ones you are learning like mass defect and binding energy. The heart of nuclear physics lies in understanding the forces that hold the nucleus together, despite the repulsive electromagnetic force between the positively charged protons.

This field explains phenomena such as radioactivity, nuclear fission and fusion, and the behavior of nuclei under extreme conditions. As part of studying nuclear physics, students delve into the intricacies of how energy is generated from the nucleus and how it plays a vital role in both natural processes, like the stars shining, and human-made technologies such as nuclear reactors and medical imaging.
Avogadro's Number
Avogadro's number, denoted commonly as \( N_A \) and named after the scientist Amedeo Avogadro, is a constant that represents the number of particles found in one mole of any substance. \( N_A = 6.022 \times 10^{23} \) entities per mole, which can refer to atoms, ions, or molecules depending on the context.

In the exercise you're working through, Avogadro's number is essential for transitioning from the individual nucleus to a larger, more relatable scale - precisely one mole of \( {}^{21}Ne \) nuclei. It’s not only fundamental to nuclear physics but also to chemistry and physics at large, aiding in the understanding of the microscopic world on a macroscopic scale. Avogadro's number bridges the gap between an individual particle and the amount of substance we can measure in the laboratory.
Energy Conversion Calculations
Energy conversion calculations play a critical role in the study of physical systems, where various forms of energy are transformed from one type to another. In the context of our nuclear binding energy exercise, we're specifically focused on the conversion of mass into energy. \( E = mc^2 \) embodies this concept, where a tiny amount of mass can be converted into a significant amount of energy.

In the provided solution, students utilize this conversion calculation to determine the binding energy released from the mass defect, indicative of the strength of the bonds within the nucleus. Performing such calculations is pivotal in physics and engineering, aiding in the design of power plants, understanding of stellar processes, and even the development of medical treatments involving radioactive isotopes.

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Most popular questions from this chapter

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?

Calculations Involving Radioactive Decay and Time If we start with \(1.000 \mathrm{~g}\) of strontium- \(90,0.953 \mathrm{~g}\) will remain after \(2.00 \mathrm{yr}\). (a) What is the half-life of strontium- 90 ? (b) How much strontium- 90 will remain after \(5.00 \mathrm{yr}\) ? (c) What is the initial activity of the sample in becquerels and curies? SOLUTION (a) Analyze We are asked to calculate a half-life, \(t_{1 / 2}\) based on data that tell us how much of a radioactive nucleus has decayed in a time interval \(t=2.00 \mathrm{yr}\) and the information \(N_{0}=1.000 \mathrm{~g}, N_{t}=0.953 \mathrm{~g}\). Plan We first calculate the rate constant for the decay, \(k\), and then use that to compute \(t_{1 / 2}\). Solve Equation \(21.19\) is solved for the decay constant, \(k\), and then Equation \(21.20\) is used to calculate half-life, \(t_{1 / 2}\) : $$ \begin{aligned} k &=-\frac{1}{t} \ln \frac{N_{\mathrm{f}}}{N_{0}}=-\frac{1}{2.00 \mathrm{yr}} \ln \frac{0.953 \mathrm{~g}}{1.000 \mathrm{~g}} \\ &=-\frac{1}{2.00 \mathrm{yr}}(-0.0481)=0.0241 \mathrm{yr}^{-1} \\ t_{1 / 2} &=\frac{0.693}{k}=\frac{0.693}{0.0241 \mathrm{yr}^{-1}}=28.8 \mathrm{yr} \end{aligned} $$ (b) Analyze We are asked to calculate the amount of a radionuclide remaining after a given period of time. Plan We need to calculate \(N_{b}\) the amount of strontium present at time \(t\), using the initial quantity, \(N_{0}\), and the rate constant for decay, \(k\), calculated in part (a). Solve Again using Equation \(21.19\), with \(k=0.0241 \mathrm{yr}^{-1}\), we have $$ \ln \frac{N_{t}}{N_{0}}=-k t=-\left(0.0241 \mathrm{yr}^{-1}\right)(5.00 \mathrm{yr})=-0.120 $$ \(N_{t} / N_{0}\) is calculated from \(\ln \left(N_{t} / N_{0}\right)=-0.120\) using the \(e^{x}\) or INV LN function of a calculator: $$ \frac{N_{t}}{N_{0}}=e^{-1.120}=0.887 $$ Because \(N_{0}=1.000 \mathrm{~g}\), we have $$ N_{t}=(0.887) N_{0}=(0.887)(1.000 \mathrm{~g})=0.887 \mathrm{~g} $$ (c) Analyze We are asked to calculate the activity of the sample in becquerels and curies. Plan We must calculate the number of disintegrations per atom per second and then multiply by the number of atoms in the sample. Solve The number of disintegrations per atom per second is given by the decay constant, \(k\) : $$ k=\left(\frac{0.0241}{\mathrm{yr}}\right)\left(\frac{1 \mathrm{yr}}{365 \text { days }}\right)\left(\frac{1 \text { day }}{24 \mathrm{~h}}\right)\left(\frac{\mathrm{lh}}{3600 \mathrm{~s}}\right)=7.64 \times 10^{-10} \mathrm{~s}^{-1} $$ To obtain the total number of disintegrations per second, we calculate the number of atoms in the sample. We multiply this quantity by \(k\), where we express \(k\) as the number of disintegrations per atom per second, to obtain the number of disintegrations per second: $$ \begin{aligned} \left(1.000 \mathrm{~g}^{90} \mathrm{Sr}\right)\left(\frac{1 \mathrm{~mol}^{90} \mathrm{Sr}}{90 \mathrm{~g}^{90} \mathrm{Sr}}\right)\left(\frac{6.022 \times 10^{23} \mathrm{atoms} \mathrm{Sr}}{1 \mathrm{~mol}^{90} \mathrm{Sr}}\right)=6.7 \times 10^{21} \text { atoms }^{90} \mathrm{Sr} \\ \text { Total disintegrations/s } &=\left(\frac{7.64 \times 10^{-10} \text { disintegrations }}{\text { atom }{ }^{2} \mathrm{~s}}\right)\left(6.7 \times 10^{21} \text { atoms }\right) \\ &=5.1 \times 10^{12} \text { disintegrations/s } \end{aligned} $$ Because \(1 \mathrm{~Bq}\) is one disintegration per second, the activity is \(5.1 \times 10^{12} \mathrm{~Bq}\). The activity in curies is given by $$ \left(5.1 \times 10^{12} \text { disintegrations/s }\right)\left(\frac{1 \mathrm{Ci}}{3.7 \times 10^{10} \text { disintegrations/s }}\right)=1.4 \times 10^{2} \mathrm{Ci} $$ We have used only two significant figures in products of these calculations because we do not know the atomic weight of \({ }^{90} \mathrm{Sr}\) to more than two significant figures without looking it up in a special source.

Complete and balance the following nuclear equations by supplying the missing particle: (a) \({ }_{7}^{14} \mathrm{~N}+{ }_{2}^{4} \mathrm{He} \longrightarrow\) ? \(+{ }_{1}^{1} \mathrm{H}\) (b) \({ }_{19}^{40} \mathrm{~K}+{ }_{-1}^{0} \mathrm{c}\) (orbital electron) \(\longrightarrow\) ? (c) \(?+{ }_{2}^{4} \mathrm{He} \longrightarrow{ }_{14}^{30} \mathrm{Si}+{ }_{1}^{1} \mathrm{H}\) (d) \({ }_{26}^{58} \mathrm{Fe}+2{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{27}^{60} \mathrm{Co}+\) ? (e) \({ }_{42}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{54}^{135} \mathrm{Xe}+2{ }_{0}^{1} \mathrm{n}+\) ?

A wooden artifact from a Chinese temple has a \({ }^{14} \mathrm{C}\) activity of \(38.0\) counts per minute as compared with an activity of \(58.2\) counts per minute for a standard of zero age. From the halflife for \({ }^{14} \mathrm{C}\) decay, \(5715 \mathrm{yr}\), determine the age of the artifact.

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, (b) the nuclear binding energy, (c) the nuclear binding energy per nucleon.

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