Isotopes of barium
Encyclopedia
Naturally occurring barium
(Ba) is a mix of six stable isotope
s and one very long-lived radioactive primordial isotope, barium-130, recently identified as being unstable by geochemical means (from analysis of the presence of its daughter xenon-130 in rocks). This nuclide decays by double-electron capture
(absorbing two electrons and emitting two neutrinos) with a half-life of 70 trillion years (about 5,000 times the age of the universe).
There are a total of thirty-three known radioisotopes in addition to 130Ba, but most of these are highly radioactive with half-lives
in the several millisecond to several minute range. and thus never encountered in nature. The only notable exceptions are 133Ba which has a half-life of 10.51 years, and 137mBa (2.55 minutes), which is the decay product of 137Cs
(30.17 years, and a common fission product
).
Barium-114 is the lightest nuclide known to undergo cluster decay
, emitting a nucleus of stable 12C
to produce 102Sn in .0034% of decays.
Standard atomic mass: 137.327(7) u
Barium
Barium is a chemical element with the symbol Ba and atomic number 56. It is the fifth element in Group 2, a soft silvery metallic alkaline earth metal. Barium is never found in nature in its pure form due to its reactivity with air. Its oxide is historically known as baryta but it reacts with...
(Ba) is a mix of six stable isotope
Isotope
Isotopes are variants of atoms of a particular chemical element, which have differing numbers of neutrons. Atoms of a particular element by definition must contain the same number of protons but may have a distinct number of neutrons which differs from atom to atom, without changing the designation...
s and one very long-lived radioactive primordial isotope, barium-130, recently identified as being unstable by geochemical means (from analysis of the presence of its daughter xenon-130 in rocks). This nuclide decays by double-electron capture
Electron capture
Electron capture is a process in which a proton-rich nuclide absorbs an inner atomic electron and simultaneously emits a neutrino...
(absorbing two electrons and emitting two neutrinos) with a half-life of 70 trillion years (about 5,000 times the age of the universe).
There are a total of thirty-three known radioisotopes in addition to 130Ba, but most of these are highly radioactive with half-lives
Half-life
Half-life, abbreviated t½, is the period of time it takes for the amount of a substance undergoing decay to decrease by half. The name was originally used to describe a characteristic of unstable atoms , but it may apply to any quantity which follows a set-rate decay.The original term, dating to...
in the several millisecond to several minute range. and thus never encountered in nature. The only notable exceptions are 133Ba which has a half-life of 10.51 years, and 137mBa (2.55 minutes), which is the decay product of 137Cs
Caesium-137
Caesium-137 is a radioactive isotope of caesium which is formed as a fission product by nuclear fission.It has a half-life of about 30.17 years, and decays by beta emission to a metastable nuclear isomer of barium-137: barium-137m . Caesium-137 is a radioactive isotope of caesium which is formed...
(30.17 years, and a common fission product
Fission product
Nuclear fission products are the atomic fragments left after a large atomic nucleus fissions. Typically, a large nucleus like that of uranium fissions by splitting into two smaller nuclei, along with a few neutrons and a large release of energy in the form of heat , gamma rays and neutrinos. The...
).
Barium-114 is the lightest nuclide known to undergo cluster decay
Cluster decay
Cluster decay is a type of nuclear decay in which a parent atomic nucleus with A nucleons and Z protons emits a cluster of Ne neutrons and Ze protons heavier than an alpha particle but lighter than a typical binary fission fragment Cluster decay (also named heavy particle radioactivity or heavy...
, emitting a nucleus of stable 12C
Carbon-12
Carbon-12 is the more abundant of the two stable isotopes of the element carbon, accounting for 98.89% of carbon; it contains 6 protons, 6 neutrons, and 6 electrons....
to produce 102Sn in .0034% of decays.
Standard atomic mass: 137.327(7) u
Table
nuclide symbol |
Z(p Proton The proton is a subatomic particle with the symbol or and a positive electric charge of 1 elementary charge. One or more protons are present in the nucleus of each atom, along with neutrons. The number of protons in each atom is its atomic number.... ) |
N(n Neutron The neutron is a subatomic hadron particle which has the symbol or , no net electric charge and a mass slightly larger than that of a proton. With the exception of hydrogen, nuclei of atoms consist of protons and neutrons, which are therefore collectively referred to as nucleons. The number of... ) |
isotopic mass (u) |
half-lifeBold for isotopes with half-lives longer than the age of the universe (nearly stable) | decay mode(s)Abbreviations: CD: Cluster decay Cluster decay Cluster decay is a type of nuclear decay in which a parent atomic nucleus with A nucleons and Z protons emits a cluster of Ne neutrons and Ze protons heavier than an alpha particle but lighter than a typical binary fission fragment Cluster decay (also named heavy particle radioactivity or heavy... EC: Electron capture Electron capture Electron capture is a process in which a proton-rich nuclide absorbs an inner atomic electron and simultaneously emits a neutrino... IT: Isomeric transition Isomeric transition An isomeric transition is a radioactive decay process that involves emission of a gamma ray from an atom where the nucleus is in an excited metastable state, referred to in its excited state, as a nuclear isomer.... |
daughter isotope(s)Bold for stable isotopes, bold italics for nearly-stable isotopes (half-life longer than the age of the universe Age of the universe The age of the universe is the time elapsed since the Big Bang posited by the most widely accepted scientific model of cosmology. The best current estimate of the age of the universe is 13.75 ± 0.13 billion years within the Lambda-CDM concordance model... ) |
nuclear spin |
representative isotopic composition (mole fraction) |
range of natural variation (mole fraction) |
---|---|---|---|---|---|---|---|---|---|
excitation energy | |||||||||
114Ba | 56 | 58 | 113.95068(15) | 530(230) ms [0.43(+30−15) s] |
β+ Beta decay In nuclear physics, beta decay is a type of radioactive decay in which a beta particle is emitted from an atom. There are two types of beta decay: beta minus and beta plus. In the case of beta decay that produces an electron emission, it is referred to as beta minus , while in the case of a... , p Proton emission Proton emission is a type of radioactive decay in which a proton is ejected from a nucleus. Proton emission can occur from high-lying excited states in a nucleus following a beta decay, in which case the process is known as beta-delayed proton emission, or can occur from the ground state of very... (99.59%) |
113Xe | 0+ | ||
α Alpha decay Alpha decay is a type of radioactive decay in which an atomic nucleus emits an alpha particle and thereby transforms into an atom with a mass number 4 less and atomic number 2 less... (.37%) |
110Xe | ||||||||
β+ (.04%) | 114Cs | ||||||||
CD Cluster decay Cluster decay is a type of nuclear decay in which a parent atomic nucleus with A nucleons and Z protons emits a cluster of Ne neutrons and Ze protons heavier than an alpha particle but lighter than a typical binary fission fragment Cluster decay (also named heavy particle radioactivity or heavy... (.0034%)Lightest nuclide Nuclide A nuclide is an atomic species characterized by the specific constitution of its nucleus, i.e., by its number of protons Z, its number of neutrons N, and its nuclear energy state.... known to undergo cluster decay |
102Sn, 12C Carbon-12 Carbon-12 is the more abundant of the two stable isotopes of the element carbon, accounting for 98.89% of carbon; it contains 6 protons, 6 neutrons, and 6 electrons.... |
||||||||
115Ba | 56 | 59 | 114.94737(64)# | 0.45(5) s | β+ | 115Cs | (5/2+)# | ||
β+, p | 114Xe | ||||||||
116Ba | 56 | 60 | 115.94138(43)# | 1.3(2) s | β+ | 116Cs | 0+ | ||
β+, p | 115Xe | ||||||||
117Ba | 56 | 61 | 116.93850(32)# | 1.75(7) s | β+ | 117Cs | (3/2)(+#) | ||
β+, α | 113I | ||||||||
β+, p | 116Xe | ||||||||
118Ba | 56 | 62 | 117.93304(21)# | 5.2(2) s | β+ | 118Cs | 0+ | ||
β+, p | 117Xe | ||||||||
119Ba | 56 | 63 | 118.93066(21) | 5.4(3) s | β+ | 119Cs | (5/2+) | ||
β+, p | 118Xe | ||||||||
120Ba | 56 | 64 | 119.92604(32) | 24(2) s | β+ | 120Cs | 0+ | ||
121Ba | 56 | 65 | 120.92405(15) | 29.7(15) s | β+ (99.98%) | 121Cs | 5/2(+) | ||
β+, p (.02%) | 120Xe | ||||||||
122Ba | 56 | 66 | 121.91990(3) | 1.95(15) min | β+ | 122Cs | 0+ | ||
123Ba | 56 | 67 | 122.918781(13) | 2.7(4) min | β+ | 123Cs | 5/2(+) | ||
124Ba | 56 | 68 | 123.915094(13) | 11.0(5) min | β+ | 124Cs | 0+ | ||
125Ba | 56 | 69 | 124.914473(12) | 3.5(4) min | β+ | 125Cs | 1/2(+#) | ||
126Ba | 56 | 70 | 125.911250(13) | 100(2) min | β+ | 126Cs | 0+ | ||
127Ba | 56 | 71 | 126.911094(12) | 12.7(4) min | β+ | 127Cs | 1/2+ | ||
127mBa | 80.33(12) keV | 1.9(2) s | IT Isomeric transition An isomeric transition is a radioactive decay process that involves emission of a gamma ray from an atom where the nucleus is in an excited metastable state, referred to in its excited state, as a nuclear isomer.... |
127Ba | 7/2− | ||||
128Ba | 56 | 72 | 127.908318(11) | 2.43(5) d | β+ | 128Cs | 0+ | ||
129Ba | 56 | 73 | 128.908679(12) | 2.23(11) h | β+ | 129Cs | 1/2+ | ||
129mBa | 8.42(6) keV | 2.16(2) h | β+ | 129Cs | 7/2+# | ||||
IT | 129Ba | ||||||||
130BaPrimordial radioisotope | 56 | 74 | 129.9063208(30) | 7×1013 a | Double EC Double electron capture Double electron capture is a decay mode of atomic nucleus. For a nuclide with number of nucleons A and atomic number Z, double electron capture is only possible if the mass of the nuclide of is lower.... |
130Xe | 0+ | 0.00106(1) | |
130mBa | 2475.12(18) keV | 9.54(14) ms | IT | 130Ba | 8− | ||||
131Ba | 56 | 75 | 130.906941(3) | 11.50(6) d | β+ | 131Cs | 1/2+ | ||
131mBa | 187.14(12) keV | 14.6(2) min | IT | 131Ba | 9/2− | ||||
132Ba | 56 | 76 | 131.9050613(11) | Observationally StableBelieved to undergo β+β+ decay to 132Xe with a half-life Half-life Half-life, abbreviated t½, is the period of time it takes for the amount of a substance undergoing decay to decrease by half. The name was originally used to describe a characteristic of unstable atoms , but it may apply to any quantity which follows a set-rate decay.The original term, dating to... over 300×1018 years |
0+ | 0.00101(1) | |||
133Ba | 56 | 77 | 132.9060075(11) | 10.51(5) a | EC | 133Cs | 1/2+ | ||
133mBa | 288.247(9) keV | 38.9(1) h | IT (99.99%) | 133Ba | 11/2− | ||||
EC (.0096%) | 133Cs | ||||||||
134Ba | 56 | 78 | 133.9045084(4) | Observationally StableTheoretically capable of spontaneous fission Spontaneous fission Spontaneous fission is a form of radioactive decay characteristic of very heavy isotopes. Because the nuclear binding energy reaches a maximum at a nuclear mass greater than about 60 atomic mass units , spontaneous breakdown into smaller nuclei and single particles becomes possible at heavier masses... |
0+ | 0.02417(18) | |||
135Ba | 56 | 79 | 134.9056886(4) | Observationally Stable | 3/2+ | 0.06592(12) | |||
135mBa | 268.22(2) keV | 28.7(2) h | IT | 135Ba | 11/2− | ||||
136Ba | 56 | 80 | 135.9045759(4) | Observationally Stable | 0+ | 0.07854(24) | |||
136mBa | 2030.466(18) keV | 308.4(19) ms | IT | 136Ba | 7− | ||||
137Ba | 56 | 81 | 136.9058274(5) | Observationally Stable | 3/2+ | 0.11232(24) | |||
137m1Ba | 661.659(3) keV | 2.552(1) min | IT | 137Ba | 11/2− | ||||
137m2Ba | 2349.1(4) keV | 0.59(10) µs | (17/2−) | ||||||
138BaFission product Fission product Nuclear fission products are the atomic fragments left after a large atomic nucleus fissions. Typically, a large nucleus like that of uranium fissions by splitting into two smaller nuclei, along with a few neutrons and a large release of energy in the form of heat , gamma rays and neutrinos. The... |
56 | 82 | 137.9052472(5) | Observationally Stable | 0+ | 0.71698(42) | |||
138mBa | 2090.54(6) keV | 800(100) ns | 6+ | ||||||
139Ba | 56 | 83 | 138.9088413(5) | 83.06(28) min | β- | 139La | 7/2− | ||
140Ba | 56 | 84 | 139.910605(9) | 12.752(3) d | β- | 140La | 0+ | ||
141Ba | 56 | 85 | 140.914411(9) | 18.27(7) min | β- | 141La | 3/2− | ||
142Ba | 56 | 86 | 141.916453(7) | 10.6(2) min | β- | 142La | 0+ | ||
143Ba | 56 | 87 | 142.920627(14) | 14.5(3) s | β- | 143La | 5/2− | ||
144Ba | 56 | 88 | 143.922953(14) | 11.5(2) s | β- (96.4%) | 144La | 0+ | ||
β+ (3.59%) | 144Cs | ||||||||
145Ba | 56 | 89 | 144.92763(8) | 4.31(16) s | β- | 145La | 5/2− | ||
146Ba | 56 | 90 | 145.93022(8) | 2.22(7) s | β- (99.98%) | 146La | 0+ | ||
β-, n Neutron emission Neutron emission is a type of radioactive decay of atoms containing excess neutrons, in which a neutron is simply ejected from the nucleus. Two examples of isotopes which emit neutrons are helium-5 and beryllium-13... (.02%) |
145La | ||||||||
147Ba | 56 | 91 | 146.93495(22)# | 0.893(1) s | β- (99.94%) | 147La | (3/2+) | ||
β-, n (.06%) | 146La | ||||||||
148Ba | 56 | 92 | 147.93772(9) | 0.612(17) s | β- (99.6%) | 148La | 0+ | ||
β-, n (.4%) | 147La | ||||||||
149Ba | 56 | 93 | 148.94258(21)# | 344(7) ms | β- (99.57%) | 149La | 3/2−# | ||
β-, n (.43%) | 148La | ||||||||
150Ba | 56 | 94 | 149.94568(43)# | 300 ms | β- | 150La | 0+ | ||
β-, n (rare) | 149La | ||||||||
151Ba | 56 | 95 | 150.95081(43)# | 200# ms [>300 ns] | β- | 151La | 3/2−# | ||
152Ba | 56 | 96 | 151.95427(54)# | 100# ms | β- | 152La | 0+ | ||
153Ba | 56 | 97 | 152.95961(86)# | 80# ms | β- | 153La | 5/2−# |