2.5: Isotopes and Average Atomic Mass
- Page ID
- 358419
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- Define the atomic mass unit and average atomic mass
- Calculate average atomic mass and isotopic abundance
Isotopes are atoms of the same element that have the same number of protons but different number of neutrons, therefore they have different masses. The symbol for a specific isotope of any element is written by placing the mass number as a superscript to the left of the element symbol (Figure \(\PageIndex{4}\)). The atomic number is sometimes written as a subscript preceding the symbol, but since this number defines the element’s identity, as does its symbol, it is often omitted. For example, magnesium exists as a mixture of three isotopes, each with an atomic number of 12 and with mass numbers of 24, 25, and 26, respectively. These isotopes can be identified as 24Mg, 25Mg, and 26Mg. These isotope symbols are read as “element, mass number” and can be symbolized consistent with this reading. For instance, 24Mg is read as “magnesium 24,” and can be written as “magnesium-24” or “Mg-24.” 25Mg is read as “magnesium 25,” and can be written as “magnesium-25” or “Mg-25.” All magnesium atoms have 12 protons in their nucleus. They differ only because a 24Mg atom has 12 neutrons in its nucleus, a 25Mg atom has 13 neutrons, and a 26Mg has 14 neutrons.

Information about the naturally occurring isotopes of elements with atomic numbers 1 through 10 is given in Table \(\PageIndex{2}\). Note that in addition to standard names and symbols, the isotopes of hydrogen are often referred to using common names and accompanying symbols. Hydrogen-2, symbolized 2H, is also called deuterium and sometimes symbolized D. Hydrogen-3, symbolized 3H, is also called tritium and sometimes symbolized T.
Element | Symbol | Atomic Number | Number of Protons | Number of Neutrons | Mass (amu) | % Natural Abundance |
---|---|---|---|---|---|---|
hydrogen | \(\ce{^1_1H}\) (protium) |
1 | 1 | 0 | 1.0078 | 99.989 |
\(\ce{^2_1H}\) (deuterium) |
1 | 1 | 1 | 2.0141 | 0.0115 | |
\(\ce{^3_1H}\) (tritium) |
1 | 1 | 2 | 3.01605 | — (trace) | |
helium | \(\ce{^3_2He}\) | 2 | 2 | 1 | 3.01603 | 0.00013 |
\(\ce{^4_2He}\) | 2 | 2 | 2 | 4.0026 | 100 | |
lithium | \(\ce{^6_3Li}\) | 3 | 3 | 3 | 6.0151 | 7.59 |
\(\ce{^7_3Li}\) | 3 | 3 | 4 | 7.0160 | 92.41 | |
beryllium | \(\ce{^9_4Be}\) | 4 | 4 | 5 | 9.0122 | 100 |
boron | \(\ce{^{10}_5B}\) | 5 | 5 | 5 | 10.0129 | 19.9 |
\(\ce{^{11}_5B}\) | 5 | 5 | 6 | 11.0093 | 80.1 | |
carbon | \(\ce{^{12}_6C}\) | 6 | 6 | 6 | 12.0000 | 98.89 |
\(\ce{^{13}_6C}\) | 6 | 6 | 7 | 13.0034 | 1.11 | |
\(\ce{^{14}_6C}\) | 6 | 6 | 8 | 14.0032 | — (trace) | |
nitrogen | \(\ce{^{14}_7N}\) | 7 | 7 | 7 | 14.0031 | 99.63 |
\(\ce{^{15}_7N}\) | 7 | 7 | 8 | 15.0001 | 0.37 | |
oxygen | \(\ce{^{16}_8O}\) | 8 | 8 | 8 | 15.9949 | 99.757 |
\(\ce{^{17}_8O}\) | 8 | 8 | 9 | 16.9991 | 0.038 | |
\(\ce{^{18}_8O}\) | 8 | 8 | 10 | 17.9992 | 0.205 | |
fluorine | \(\ce{^{19}_9F}\) | 9 | 9 | 10 | 18.9984 | 100 |
neon | \(\ce{^{20}_{10}Ne}\) | 10 | 10 | 10 | 19.9924 | 90.48 |
\(\ce{^{21}_{10}Ne}\) | 10 | 10 | 11 | 20.9938 | 0.27 | |
\(\ce{^{22}_{10}Ne}\) | 10 | 10 | 12 | 21.9914 | 9.25 |
Atomic Mass
Because each proton and each neutron contribute approximately one amu to the mass of an atom, and each electron contributes far less, the atomic mass of a single atom is approximately equal to its mass number (a whole number). However, the average masses of atoms of most elements are not whole numbers because most elements exist naturally as mixtures of two or more isotopes.
The mass of an element shown in a periodic table or listed in a table of atomic masses is a weighted, average mass of all the isotopes present in a naturally occurring sample of that element. This is equal to the sum of each individual isotope’s mass multiplied by its fractional abundance.
\[\mathrm{average\: mass}=\sum_{i}(\mathrm{fractional\: abundance\times isotopic\: mass})_i\]
For example, the element boron is composed of two isotopes: About 19.9% of all boron atoms are 10B with a mass of 10.0129 amu, and the remaining 80.1% are 11B with a mass of 11.0093 amu. The average atomic mass for boron is calculated to be:
\[\begin{align*}
\textrm{boron average mass} &=\mathrm{(0.199\times10.0129\: amu)+(0.801\times11.0093\: amu)}\\
&=\mathrm{1.99\: amu+8.82\: amu}\\
&=\mathrm{10.81\: amu}
\end{align*}\]
It is important to understand that no single boron atom weighs exactly 10.8 amu; 10.8 amu is the average mass of all boron atoms, and individual boron atoms weigh either approximately 10 amu or 11 amu.
A meteorite found in central Indiana contains traces of the noble gas neon picked up from the solar wind during the meteorite’s trip through the solar system. Analysis of a sample of the gas showed that it consisted of 91.84% 20Ne (mass 19.9924 amu), 0.47% 21Ne (mass 20.9940 amu), and 7.69% 22Ne (mass 21.9914 amu). What is the average mass of the neon in the solar wind?
Solution
\[\begin{align*}
\mathrm{average\: mass} &=\mathrm{(0.9184\times19.9924\: amu)+(0.0047\times20.9940\: amu)+(0.0769\times21.9914\: amu)}\\
&=\mathrm{(18.36+0.099+1.69)\:amu}\\
&=\mathrm{20.15\: amu}
\end{align*}\]
The average mass of a neon atom in the solar wind is 20.15 amu. (The average mass of a terrestrial neon atom is 20.1796 amu. This result demonstrates that we may find slight differences in the natural abundance of isotopes, depending on their origin.)
A sample of magnesium is found to contain 78.70% of 24Mg atoms (mass 23.98 amu), 10.13% of 25Mg atoms (mass 24.99 amu), and 11.17% of 26Mg atoms (mass 25.98 amu). Calculate the average mass of a Mg atom.
- Answer
-
24.31 amu
We can also do variations of this type of calculation, as shown in the next example.
Naturally occurring chlorine consists of 35Cl (mass 34.96885 amu) and 37Cl (mass 36.96590 amu), with an average mass of 35.453 amu. What is the percent composition of Cl in terms of these two isotopes?
Solution
The average mass of chlorine is the fraction that is 35Cl times the mass of 35Cl plus the fraction that is 37Cl times the mass of 37Cl.
\[\mathrm{average\: mass=(fraction\: of\: ^{35}Cl\times mass\: of\: ^{35}Cl)+(fraction\: of\: ^{37}Cl\times mass\: of\: ^{37}Cl)}\]
If we let x represent the fraction that is 35Cl, then the fraction that is 37Cl is represented by 1.00 − x.
(The fraction that is 35Cl + the fraction that is 37Cl must add up to 1, so the fraction of 37Cl must equal 1.00 − the fraction of 35Cl.)
Substituting this into the average mass equation, we have:
\[\begin{align*}
\mathrm{35.453\: amu} &=(x\times 34.96885\: \ce{amu})+[(1.00-x)\times 36.96590\: \ce{amu}]\\
35.453 &=34.96885x+36.96590-36.96590x\\
1.99705x &=1.513\\
x&=\dfrac{1.513}{1.99705}=0.7576
\end{align*}\]
So solving yields: x = 0.7576, which means that 1.00 − 0.7576 = 0.2424. Therefore, chlorine consists of 75.76% 35Cl and 24.24% 37Cl.
Naturally occurring copper consists of 63Cu (mass 62.9296 amu) and 65Cu (mass 64.9278 amu), with an average mass of 63.546 amu. What is the percent composition of Cu in terms of these two isotopes?
- Answer
-
69.15% Cu-63 and 30.85% Cu-65

The occurrence and natural abundances of isotopes can be experimentally determined using an instrument called a mass spectrometer. Mass spectrometry (MS) is widely used in chemistry, forensics, medicine, environmental science, and many other fields to analyze and help identify the substances in a sample of material. In a typical mass spectrometer (Figure \(\PageIndex{5}\)), the sample is vaporized and exposed to a high-energy electron beam that causes the sample’s atoms (or molecules) to become electrically charged, typically by losing one or more electrons. These cations then pass through a (variable) electric or magnetic field that deflects each cation’s path to an extent that depends on both its mass and charge (similar to how the path of a large steel ball bearing rolling past a magnet is deflected to a lesser extent that that of a small steel BB). The ions are detected, and a plot of the relative number of ions generated versus their mass-to-charge ratios (a mass spectrum) is made. The height of each vertical feature or peak in a mass spectrum is proportional to the fraction of cations with the specified mass-to-charge ratio. Since its initial use during the development of modern atomic theory, MS has evolved to become a powerful tool for chemical analysis in a wide range of applications.
Video \(\PageIndex{1}\): Watch this video from the Royal Society for Chemistry for a brief description of the rudiments of mass spectrometry.
Summary
Isotopes of an element are atoms with the same atomic number but different mass numbers; isotopes of an element, therefore, differ from each other only in the number of neutrons within the nucleus. When a naturally occurring element is composed of several isotopes, the atomic mass of the element represents the average of the masses of the isotopes involved. A chemical symbol identifies the atoms in a substance using symbols, which are one-, two-, or three-letter abbreviations for the atoms.
Key Equations
- \(\mathrm{average\: mass}=\sum_{i}(\mathrm{fractional\: abundance \times isotopic\: mass})_i\)
Glossary
- atomic mass
- average mass of atoms of an element, expressed in amu
- atomic mass unit (amu)
- (also, unified atomic mass unit, u, or Dalton, Da) unit of mass equal to \(\dfrac{1}{12}\) of the mass of a 12C atom
- atomic number (Z)
- number of protons in the nucleus of an atom
- Dalton (Da)
- alternative unit equivalent to the atomic mass unit
- mass number (A)
- sum of the numbers of neutrons and protons in the nucleus of an atom
- unified atomic mass unit (u)
- alternative unit equivalent to the atomic mass unit
Contributors and Attributions
Paul Flowers (University of North Carolina - Pembroke), Klaus Theopold (University of Delaware) and Richard Langley (Stephen F. Austin State University) with contributing authors. Textbook content produced by OpenStax College is licensed under a Creative Commons Attribution License 4.0 license. Download for free at http://cnx.org/contents/85abf193-2bd...a7ac8df6@9.110).