Isotopes of lanthanum
Encyclopedia
Naturally occurring lanthanum
Lanthanum
Lanthanum is a chemical element with the symbol La and atomic number 57.Lanthanum is a silvery white metallic element that belongs to group 3 of the periodic table and is the first element of the lanthanide series. It is found in some rare-earth minerals, usually in combination with cerium and...

(La) is composed of one stable (139La) and one radioactive (138La) 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...

, with the stable isotope, 139La, being the most abundant (99.91% 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...

). 38 radioisotopes have been characterized with the most stable being 138La 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...

 of 102×109 years, 137La with a half-life of 60,000 years and 140La with a half-life of 1.6781 days. The remaining radioactive isotopes have half-lives that are less than a day and the majority of these have half-lives that are less than 1 minute. This element also has 12 nuclear isomer
Nuclear isomer
A nuclear isomer is a metastable state of an atomic nucleus caused by the excitation of one or more of its nucleons . "Metastable" refers to the fact that these excited states have half-lives more than 100 to 1000 times the half-lives of the other possible excited nuclear states...

s, the longest-lived of which is 132mLa with a half-life of 24.3 minutes.

The isotopes of lanthanum 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 116.95 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...

 (117La) to 154.96 u (155La).

Standard atomic mass: 138.90547(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:
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 near-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
117La 57 60 116.95007(43)# 23.5(26) 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...

117Ba (3/2+,3/2−)
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...

116Ba
117mLa 151(12) keV 10(5) ms (9/2+)
118La 57 61 117.94673(32)# 200# ms β+ 118Ba
119La 57 62 118.94099(43)# 1# s β+ 119Ba 11/2−#
120La 57 63 119.93807(54)# 2.8(2) s β+ 120Ba
β+, p 119Cs
121La 57 64 120.93301(54)# 5.3(2) s β+ 121Ba 11/2−#
β+, p 120Cs
122La 57 65 121.93071(32)# 8.6(5) s β+ 122Ba
β+, p 121Cs
123La 57 66 122.92624(21)# 17(3) s β+ 123Ba 11/2−#
124La 57 67 123.92457(6) 29.21(17) s β+ 124Ba (7−,8−)
124mLa 100(100)# keV 21(4) s low(+#)
125La 57 68 124.920816(28) 64.8(12) s β+ 125Ba (11/2−)
125mLa 107.0(10) keV 390(40) ms (3/2+)
126La 57 69 125.91951(10) 54(2) s β+ 126Ba (5)(+#)
126mLa 210(410) keV 20(20) s (0−,1−,2−)
127La 57 70 126.916375(28) 5.1(1) min β+ 127Ba (11/2−)
127mLa 14.8(12) keV 3.7(4) min β+ 127Ba (3/2+)
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....

127La
128La 57 71 127.91559(6) 5.18(14) min β+ 128Ba (5+)
128mLa 100(100)# keV <1.4 min IT 128La (1+,2−)
129La 57 72 128.912693(22) 11.6(2) min β+ 129Ba 3/2+
129mLa 172.1(4) keV 560(50) ms IT 129La 11/2−
130La 57 73 129.912369(28) 8.7(1) min β+ 130Ba 3(+)
131La 57 74 130.91007(3) 59(2) min β+ 131Ba 3/2+
131mLa 304.52(24) keV 170(10) µs 11/2−
132La 57 75 131.91010(4) 4.8(2) h β+ 132Ba 2−
132mLa 188.18(11) keV 24.3(5) min IT (76%) 132La 6−
β+ (24%) 132Ba
133La 57 76 132.90822(3) 3.912(8) h β+ 133Ba 5/2+
134La 57 77 133.908514(21) 6.45(16) min β+ 134Ba 1+
135La 57 78 134.906977(11) 19.5(2) h β+ 135Ba 5/2+
136La 57 79 135.90764(6) 9.87(3) min β+ 136Ba 1+
136mLa 255(9) keV 114(3) ms IT 136La (8)(−#)
137La 57 80 136.906494(14) 6(2)E×104 a EC
Electron capture
Electron capture is a process in which a proton-rich nuclide absorbs an inner atomic electron and simultaneously emits a neutrino...

137Ba 7/2+
138LaPrimordial
Primordial nuclide
In geochemistry and geonuclear physics, primordial nuclides or primordial isotopes are nuclides found on the earth that have existed in their current form since before Earth was formed. Only 288 such nuclides are known...

 radionuclide
Radionuclide
A radionuclide is an atom with an unstable nucleus, which is a nucleus characterized by excess energy available to be imparted either to a newly created radiation particle within the nucleus or to an atomic electron. The radionuclide, in this process, undergoes radioactive decay, and emits gamma...

57 81 137.907112(4) 1.02(1)×1011 a β+ (66.4%) 138Ba 5+ 9.0(1)×10−4
β- (33.6%) 138Ce
138mLa 72.57(3) keV 116(5) ns (3)+
139LaFission 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...

57 82 138.9063533(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...

7/2+ 0.99910(1)
140La 57 83 139.9094776(26) 1.6781(3) d β- 140Ce 3−
141La 57 84 140.910962(5) 3.92(3) h β- 141Ce (7/2+)
142La 57 85 141.914079(6) 91.1(5) min β- 142Ce 2−
143La 57 86 142.916063(17) 14.2(1) min β- 143Ce (7/2)+
144La 57 87 143.91960(5) 40.8(4) s β- 144Ce (3−)
145La 57 88 144.92165(10) 24.8(20) s β- 145Ce (5/2+)
146La 57 89 145.92579(8) 6.27(10) s β- (99.99%) 146Ce 2−
β-, 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...

(.007%)
145Ce
146mLa 130(130) keV 10.0(1) s β- 146Ce (6−)
147La 57 90 146.92824(5) 4.015(8) s β- (99.96%) 147Ce (5/2+)
β-, n (.04%) 146Ce
148La 57 91 147.93223(6) 1.26(8) s β- (99.85%) 148Ce (2−)
β-, n (.15%) 147Ce
149La 57 92 148.93473(34)# 1.05(3) s β- (98.6%) 149Ce 5/2+#
β-, n (1.4%) 148Ce
150La 57 93 149.93877(43)# 510(30) ms β- (97.3%) 150Ce (3+)
β-, n (2.7%) 149Ce
151La 57 94 150.94172(43)# 300# ms [>300 ns] β- 151Ce 5/2+#
152La 57 95 151.94625(43)# 200# ms [>300 ns] β- 152Ce
153La 57 96 152.94962(64)# 150# ms [>300 ns] β- 153Ce 5/2+#
154La 57 97 153.95450(64)# 100# ms β- 154Ce
155La 57 98 154.95835(86)# 60# ms β- 155Ce 5/2+#

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