Isotopes

What is an Isotope?

Isotopes are various forms of an element that have the same number of protons but a different number of neutrons. Some elements, such as carbon, potassium, and uranium, have multiple naturally-occurring isotopes. Isotopes are defined first by their element and then by the sum of the protons and neutrons present.

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, as shown in the figure below. 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 instance:

  • Carbon-12 (or 12C) contains six protons, six neutrons, and six electrons; therefore, it has a mass number of 12 amu (six protons and six neutrons).
  • Carbon-14 (or 14C) contains six protons, eight neutrons, and six electrons; its atomic mass is 14 amu (six protons and eight neutrons).

Note that isotope symbols are read as “element, mass number.” For instance, in the case of magnesium, 24Mg is read as “magnesium 24,” and can be written as “magnesium-24” or “Mg-24.” 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.

The symbol for an atom indicates the element via its usual two-letter symbol, the mass number as a left superscript, the atomic number as a left subscript (sometimes omitted), and the charge as a right superscript.

Properties of Isotopes

While the mass of individual isotopes is different, their physical and chemical properties remain mostly unchanged.

Isotopes do differ in their stability. Carbon-12 (12C) is the most abundant of the carbon isotopes, accounting for 98.89% of carbon on Earth. Carbon-14 (14C) is unstable and only occurs in trace amounts. Unstable isotopes most commonly emit alpha particles (He2+) and electrons. Neutrons, protons, and positrons can also be emitted and electrons can be captured to attain a more stable atomic configuration (lower level of potential energy ) through a process called radioactive decay. The new atoms created may be in a high energy state and emit gamma rays which lowers the energy but alone does not change the atom into another isotope. These atoms are called radioactive isotopes or radioisotopes.

Information about the naturally occurring isotopes of elements with atomic numbers 1 through 10 is given in the table below. 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.

ElementSymbolAtomic NumberNumber of ProtonsNumber of NeutronsMass (amu)% Natural Abundance
hydrogen1
1H

(protium)

1101.007899.989
2
1H

(deuterium)

1112.01410.0115
3
1H

(tritium)

1123.01605— (trace)
helium3
2He
2213.016030.00013
4
2He
2224.0026100
lithium6
3Li
3336.01517.59
7
3Li
3347.016092.41
beryllium9
4Be
4459.0122100
boron10
5 B
55510.012919.9
11
5 B
55611.009380.1
carbon12
6 C
66612.000098.89
13
6 C
66713.00341.11
14
6 C
66814.0032— (trace)
nitrogen14
7 N
77714.003199.63
15
7 N
77815.00010.37
oxygen16
8 O
88815.994999.757
17
8 O
88916.99910.038
18
8 O
881017.99920.205
fluorine19
9 F
991018.9984100
neon20
10Ne
10101019.992490.48
21
10Ne
10101120.99380.27
22
10Ne
10101221.99149.25
Nuclear Compositions of Atoms of the Very Light Elements