OWLV2 FOR MOORE/STANITSKI'S CHEMISTRY:
OWLV2 FOR MOORE/STANITSKI'S CHEMISTRY:
5th Edition
ISBN: 9781285460369
Author: STANITSKI
Publisher: Cengage Learning
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Chapter 18, Problem 24QRT
Interpretation Introduction

Interpretation:

Binding energy per nucleon for the two isotopes of phosphorus has to be calculated and their stability has to be compared.

Concept Introduction:

Binding energy is a short strong force that is present in the nucleus which holds the protons together by overcoming the electrostatic repulsive forces between them.  Whenever there is a change in energy, a corresponding change in mass is also observed and this can be given by the equation shown below,

    ΔE = (Δm)c2

When more particles combine to form nuclear there is a great change in mass and energy.  The nuclear stabilities can be compared more appropriately by dividing the binding energy of nucleus with the number of nucleons.  The result obtained is the binding energy per nucleon.  Protons and neutrons are known as nucleons.  Binding energy is represented as Eb.

Expert Solution & Answer
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Explanation of Solution

Given equations in the problem statement is,

    15H11 + 15n01 P153015H11 + 16n01 P1531

For P1530:

The change in mass can be calculated as shown below,

Δm = (15×1.00783g/molH11)+(15×1.00867g/moln01)29.97832g/molP1530 = 15.11745g/mol+15.13005g/mol29.97832g/mol = 30.2475g/mol29.97832g/mol = 0.26918g/mol

Nuclear binding energy can be calculated as shown below,

ΔE = (Δm)c2 = (0.26918g1mol×1kg1000g)×(2.99792×108m/s)2×1J1kgm2s-2×1kJ1000J = 2.4192×1010kJ/mol

Binding energy per nucleon can be calculated as shown below,

There is a total of thirty nucleons in phosphorus-30.  Hence, the binding energy per nucleon can be calculated as,

    Eb = 2.4192×1010kJ30molnucleons = 8.064×108kJ/mol

Binding energy per nucleon in P1530 is 8.064×108kJ/mol.

For P1531:

The change in mass can be calculated as shown below,

Δm = (15×1.00783g/molH11)+(16×1.00867g/moln01)30.97376g/molP1531 = 15.11745g/mol+16.13872g/mol30.97376g/mol = 31.25617g/mol30.97376g/mol = 0.28241g/mol

Nuclear binding energy can be calculated as shown below,

ΔE = (Δm)c2 = (0.28241g1mol×1kg1000g)×(2.99792×108m/s)2×1J1kgm2s-2×1kJ1000J = 2.5381×1010kJ/mol

Binding energy per nucleon can be calculated as shown below,

There is a total of thirty one nucleons in phosphorus-11.  Hence, the binding energy per nucleon can be calculated as,

    Eb = 2.5381×1010kJ31molnucleons = 0.0846×1010kJ/mol = 8.46×108kJ/mol

Binding energy per nucleon in P1531 is 8.46×108kJ/mol.

On comparing the binding energy per nucleon for P1530 and P1531, it is found that P1531 has more binding energy per nucleon than P1530.  Hence, P1531 is more stable than P1530.

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Chapter 18 Solutions

OWLV2 FOR MOORE/STANITSKI'S CHEMISTRY:

Ch. 18.4 - Prob. 18.6PSPCh. 18.4 - Prob. 18.7PSPCh. 18.4 - Prob. 18.6ECh. 18.4 - Prob. 18.7CECh. 18.5 - Prob. 18.8ECh. 18.5 - Prob. 18.9CECh. 18.6 - Prob. 18.10ECh. 18.6 - Prob. 18.11ECh. 18.7 - Prob. 18.12ECh. 18.8 - Prob. 18.13ECh. 18.8 - Prob. 18.14ECh. 18.9 - Prob. 18.15ECh. 18 - Prob. 1SPCh. 18 - Prob. 2SPCh. 18 - Prob. 3SPCh. 18 - Prob. 4SPCh. 18 - Prob. 5SPCh. 18 - Prob. 1QRTCh. 18 - Prob. 2QRTCh. 18 - Prob. 3QRTCh. 18 - Prob. 4QRTCh. 18 - Prob. 5QRTCh. 18 - Prob. 6QRTCh. 18 - Prob. 7QRTCh. 18 - Prob. 8QRTCh. 18 - Prob. 9QRTCh. 18 - Complete the table.Ch. 18 - Prob. 11QRTCh. 18 - Prob. 12QRTCh. 18 - Prob. 13QRTCh. 18 - Prob. 14QRTCh. 18 - Prob. 15QRTCh. 18 - Prob. 16QRTCh. 18 - Prob. 17QRTCh. 18 - Prob. 18QRTCh. 18 - Prob. 19QRTCh. 18 - Prob. 20QRTCh. 18 - Prob. 21QRTCh. 18 - Prob. 22QRTCh. 18 - Prob. 23QRTCh. 18 - Prob. 24QRTCh. 18 - Prob. 25QRTCh. 18 - Prob. 26QRTCh. 18 - Prob. 27QRTCh. 18 - Prob. 28QRTCh. 18 - Prob. 29QRTCh. 18 - Prob. 30QRTCh. 18 - Prob. 31QRTCh. 18 - Prob. 32QRTCh. 18 - Prob. 33QRTCh. 18 - Prob. 34QRTCh. 18 - Prob. 35QRTCh. 18 - Prob. 36QRTCh. 18 - Prob. 37QRTCh. 18 - Prob. 38QRTCh. 18 - Prob. 39QRTCh. 18 - Prob. 40QRTCh. 18 - Prob. 41QRTCh. 18 - Prob. 42QRTCh. 18 - Prob. 43QRTCh. 18 - Prob. 44QRTCh. 18 - Prob. 45QRTCh. 18 - Prob. 46QRTCh. 18 - Prob. 47QRTCh. 18 - Prob. 48QRTCh. 18 - Prob. 49QRTCh. 18 - Prob. 50QRTCh. 18 - Prob. 51QRTCh. 18 - Prob. 52QRTCh. 18 - Prob. 53QRTCh. 18 - Prob. 54QRTCh. 18 - Prob. 55QRTCh. 18 - Prob. 56QRTCh. 18 - Prob. 57QRTCh. 18 - Prob. 58QRTCh. 18 - Prob. 59QRTCh. 18 - Prob. 60QRTCh. 18 - Prob. 61QRTCh. 18 - Prob. 62QRTCh. 18 - Prob. 63QRTCh. 18 - Prob. 64QRTCh. 18 - Prob. 65QRTCh. 18 - Prob. 66QRTCh. 18 - Prob. 67QRTCh. 18 - Prob. 68QRTCh. 18 - Prob. 69QRTCh. 18 - Prob. 70QRTCh. 18 - Prob. 71QRTCh. 18 - Prob. 72QRTCh. 18 - Prob. 73QRTCh. 18 - Prob. 74QRTCh. 18 - Prob. 75QRTCh. 18 - Prob. 76QRTCh. 18 - Prob. 77QRTCh. 18 - Prob. 78QRTCh. 18 - Prob. 79QRTCh. 18 - Prob. 80QRTCh. 18 - Prob. 81QRTCh. 18 - Prob. 82QRTCh. 18 - Prob. 83QRTCh. 18 - Prob. 84QRTCh. 18 - Prob. 85QRTCh. 18 - Prob. 86QRTCh. 18 - Prob. 87QRTCh. 18 - Prob. 88QRTCh. 18 - Prob. 89QRTCh. 18 - Prob. 91QRTCh. 18 - Prob. 92QRTCh. 18 - Prob. 93QRTCh. 18 - Prob. 94QRTCh. 18 - Prob. 95QRTCh. 18 - Prob. 96QRTCh. 18 - Prob. 18.ACPCh. 18 - Prob. 18.BCPCh. 18 - Prob. 18.CCPCh. 18 - Prob. 18.DCPCh. 18 - Prob. 18.ECP
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