Isotopes of cerium
Encyclopedia
Naturally occurring cerium
(Ce) is composed of 4 stable isotope
s: 136Ce, 138Ce, 140Ce, and 142Ce with 140Ce being the most abundant (88.48% natural abundance
); 136Ce, 138Ce, and 142Ce are predicted to undergo double beta decay but this process has never been observed. 35 radioisotopes have been characterized with the most stable being 144Ce with a half-life of 284.893 days, 139Ce with a half-life of 137.640 days, and 141Ce with a half-life of 32.501 days. All of the remaining radioactive isotopes have half-lives that are less than 4 days and the majority of these have half-lives that are less than 10 minutes. This element also has 10 meta states.
The isotopes of cerium range in atomic weight
from 119 u
(119Ce) to 157 u (157Ce).
Standard atomic mass: 140.116(1) u
Cerium
Cerium is a chemical element with the symbol Ce and atomic number 58. It is a soft, silvery, ductile metal which easily oxidizes in air. Cerium was named after the dwarf planet . Cerium is the most abundant of the rare earth elements, making up about 0.0046% of the Earth's crust by weight...
(Ce) is composed of 4 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: 136Ce, 138Ce, 140Ce, and 142Ce with 140Ce being the most abundant (88.48% natural abundance
Natural abundance
In chemistry, natural abundance refers to the abundance of isotopes of a chemical element as naturally found on a planet. The relative atomic mass of these isotopes is the atomic weight listed for the element in the periodic table...
); 136Ce, 138Ce, and 142Ce are predicted to undergo double beta decay but this process has never been observed. 35 radioisotopes have been characterized with the most stable being 144Ce with a half-life of 284.893 days, 139Ce with a half-life of 137.640 days, and 141Ce with a half-life of 32.501 days. All of the remaining radioactive isotopes have half-lives that are less than 4 days and the majority of these have half-lives that are less than 10 minutes. This element also has 10 meta states.
The isotopes of cerium range in atomic weight
Atomic weight
Atomic weight is a dimensionless physical quantity, the ratio of the average mass of atoms of an element to 1/12 of the mass of an atom of carbon-12...
from 119 u
Atomic mass unit
The unified atomic mass unit or dalton is a unit that is used for indicating mass on an atomic or molecular scale. It is defined as one twelfth of the rest mass of an unbound neutral atom of carbon-12 in its nuclear and electronic ground state, and has a value of...
(119Ce) to 157 u (157Ce).
Standard atomic mass: 140.116(1) 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-life | decay mode(s)Abbreviations: 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 |
nuclear spin |
representative isotopic composition (mole fraction) |
range of natural variation (mole fraction) |
---|---|---|---|---|---|---|---|---|---|
excitation energy | |||||||||
119Ce | 58 | 61 | 118.95276(64)# | 200# ms | 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... |
119La | 5/2+# | ||
120Ce | 58 | 62 | 119.94664(75)# | 250# ms | β+ | 120La | 0+ | ||
121Ce | 58 | 63 | 120.94342(54)# | 1.1(1) s | β+ | 121La | (5/2)(+#) | ||
122Ce | 58 | 64 | 121.93791(43)# | 2# s | β+ | 122La | 0+ | ||
β+, 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... |
121Ba | ||||||||
123Ce | 58 | 65 | 122.93540(32)# | 3.8(2) s | β+ | 123La | (5/2)(+#) | ||
β+, p | 122Ba | ||||||||
124Ce | 58 | 66 | 123.93041(32)# | 9.1(12) s | β+ | 124La | 0+ | ||
125Ce | 58 | 67 | 124.92844(21)# | 9.3(3) s | β+ | 125La | (7/2-) | ||
β+, p | 124Ba | ||||||||
126Ce | 58 | 68 | 125.92397(3) | 51.0(3) s | β+ | 126La | 0+ | ||
127Ce | 58 | 69 | 126.92273(6) | 29(2) s | β+ | 127La | 5/2+# | ||
128Ce | 58 | 70 | 127.91891(3) | 3.93(2) min | β+ | 128La | 0+ | ||
129Ce | 58 | 71 | 128.91810(3) | 3.5(3) min | β+ | 129La | (5/2+) | ||
130Ce | 58 | 72 | 129.91474(3) | 22.9(5) min | β+ | 130La | 0+ | ||
130mCe | 2453.6(3) keV | 100(8) ns | (7-) | ||||||
131Ce | 58 | 73 | 130.91442(4) | 10.2(3) min | β+ | 131La | (7/2+) | ||
131mCe | 61.8(1) keV | 5.0(10) min | β+ | 131La | (1/2+) | ||||
132Ce | 58 | 74 | 131.911460(22) | 3.51(11) h | β+ | 132La | 0+ | ||
132mCe | 2340.8(5) keV | 9.4(3) ms | 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.... |
132Ce | (8-) | ||||
133Ce | 58 | 75 | 132.911515(18) | 97(4) min | β+ | 133La | 1/2+ | ||
133mCe | 37.1(8) keV | 4.9(4) h | β+ | 133La | 9/2- | ||||
134Ce | 58 | 76 | 133.908925(22) | 3.16(4) d | EC Electron capture Electron capture is a process in which a proton-rich nuclide absorbs an inner atomic electron and simultaneously emits a neutrino... |
134La | 0+ | ||
135Ce | 58 | 77 | 134.909151(12) | 17.7(3) h | β+ | 135La | 1/2(+) | ||
135mCe | 445.8(2) keV | 20(1) s | IT | 135Ce | (11/2-) | ||||
136Ce | 58 | 78 | 135.907172(14) | Observationally StableTheorized to undergo β+β+ decay to 136Ba 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 38×1015 years |
0+ | 0.00185(2) | 0.00185-0.00186 | ||
136mCe | 3095.5(4) keV | 2.2(2) µs | 10+ | ||||||
137Ce | 58 | 79 | 136.907806(14) | 9.0(3) h | β+ | 137La | 3/2+ | ||
137mCe | 254.29(5) keV | 34.4(3) h | IT (99.22%) | 137Ce | 11/2- | ||||
β+ (.779%) | 137La | ||||||||
138Ce | 58 | 80 | 137.905991(11) | Observationally StableTheorized to undergo β+β+ decay to 138Ba with a half-life over 150×1012 years | 0+ | 0.00251(2) | 0.00251-0.00254 | ||
138mCe | 2129.17(12) keV | 8.65(20) ms | IT | 138Ce | 7- | ||||
139Ce | 58 | 81 | 138.906653(8) | 137.641(20) d | EC | 139La | 3/2+ | ||
139mCe | 754.24(8) keV | 56.54(13) s | IT | 139Ce | 11/2- | ||||
140CeFission 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... |
58 | 82 | 139.9054387(26) | 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+ | 0.88450(51) | 0.88446-0.88449 | ||
140mCe | 2107.85(3) keV | 7.3(15) µs | 6+ | ||||||
141Ce | 58 | 83 | 140.9082763(26) | 32.508(13) d | β- | 141Pr | 7/2- | ||
142Ce | 58 | 84 | 141.909244(3) | Observationally StableTheorized to undergo β-β- decay to 142Nd with a half-life over 50×1015 years | 0+ | 0.11114(51) | 0.11114-0.11114 | ||
143Ce | 58 | 85 | 142.912386(3) | 33.039(6) h | β- | 143Pr | 3/2- | ||
144Ce | 58 | 86 | 143.913647(4) | 284.91(5) d | β- | 144mPr | 0+ | ||
145Ce | 58 | 87 | 144.91723(4) | 3.01(6) min | β- | 145Pr | (3/2-) | ||
146Ce | 58 | 88 | 145.91876(7) | 13.52(13) min | β- | 146Pr | 0+ | ||
147Ce | 58 | 89 | 146.92267(3) | 56.4(10) s | β- | 147Pr | (5/2-) | ||
148Ce | 58 | 90 | 147.92443(3) | 56(1) s | β- | 148Pr | 0+ | ||
149Ce | 58 | 91 | 148.9284(1) | 5.3(2) s | β- | 149Pr | (3/2-)# | ||
150Ce | 58 | 92 | 149.93041(5) | 4.0(6) s | β- | 150Pr | 0+ | ||
151Ce | 58 | 93 | 150.93398(11) | 1.02(6) s | β- | 151Pr | 3/2-# | ||
152Ce | 58 | 94 | 151.93654(21)# | 1.4(2) s | β- | 152Pr | 0+ | ||
153Ce | 58 | 95 | 152.94058(43)# | 500# ms [>300 ns] | β- | 153Pr | 3/2-# | ||
154Ce | 58 | 96 | 153.94342(54)# | 300# ms [>300 ns] | β- | 154Pr | 0+ | ||
155Ce | 58 | 97 | 154.94804(64)# | 200# ms [>300 ns] | β- | 155Pr | 5/2-# | ||
156Ce | 58 | 98 | 155.95126(64)# | 150# ms | β- | 156Pr | 0+ | ||
157Ce | 58 | 99 | 156.95634(75)# | 50# ms | β- | 157Pr | 7/2+# |