Isotopes Of Erbium
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Naturally occurring
erbium Erbium is a chemical element; it has Symbol (chemistry), symbol Er and atomic number 68. A silvery-white solid metal when artificially isolated, natural erbium is always found in chemical combination with other elements. It is a lanthanide, a rare- ...
(68Er) is composed of six stable
isotope Isotopes are distinct nuclear species (or ''nuclides'') of the same chemical element. They have the same atomic number (number of protons in their Atomic nucleus, nuclei) and position in the periodic table (and hence belong to the same chemica ...
s, with 166Er being the most abundant (33.503%
natural abundance In physics, natural abundance (NA) refers to the abundance of isotopes of a chemical element as naturally found on a planet. The relative atomic mass (a weighted average, weighted by mole-fraction abundance figures) of these isotopes is the ato ...
). Thirty-nine
radioisotope A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess numbers of either neutrons or protons, giving it excess nuclear energy, and making it unstable. This excess energy can be used in one of three ...
s have been characterized with between 74 and 112 neutrons, or 142 to 180 nucleons, with the most stable being 169Er with a
half-life Half-life is a mathematical and scientific description of exponential or gradual decay. Half-life, half life or halflife may also refer to: Film * Half-Life (film), ''Half-Life'' (film), a 2008 independent film by Jennifer Phang * ''Half Life: ...
of 9.4 days, 172Er with a half-life of 49.3 hours, 160Er with a half-life of 28.58 hours, 165Er with a half-life of 10.36 hours, and 171Er with a half-life of 7.516 hours. All of the remaining
radioactive Radioactive decay (also known as nuclear decay, radioactivity, radioactive disintegration, or nuclear disintegration) is the process by which an unstable atomic nucleus loses energy by radiation. A material containing unstable nuclei is conside ...
isotopes have half-lives that are less than 3.5 hours, and the majority of these have half-lives that are less than 4 minutes. This element also has numerous
meta state A nuclear isomer is a metastable state of an atomic nucleus, in which one or more nucleons (protons or neutrons) occupy excited state levels (higher energy levels). "Metastable" describes nuclei whose excited states have half-lives of 10−9 s ...
s, with the most stable being 167mEr (t1/2 = 2.269 seconds). The isotopes of erbium range in
atomic weight Relative atomic mass (symbol: ''A''; sometimes abbreviated RAM or r.a.m.), also known by the deprecated synonym atomic weight, is a dimensionless physical quantity defined as the ratio of the average mass of atoms of a chemical element in a giv ...
from 141.9723  u (142Er) to 179.9644 u (180Er). The primary
decay mode Radioactive decay (also known as nuclear decay, radioactivity, radioactive disintegration, or nuclear disintegration) is the process by which an unstable atomic nucleus loses energy by radiation. A material containing unstable nuclei is conside ...
before the most abundant stable isotope, 166Er, is
electron capture Electron capture (K-electron capture, also K-capture, or L-electron capture, L-capture) is a process in which the proton-rich nucleus of an electrically neutral atom absorbs an inner atomic electron, usually from the K or L electron shells. Th ...
, and the primary mode after is
beta decay In nuclear physics, beta decay (β-decay) is a type of radioactive decay in which an atomic nucleus emits a beta particle (fast energetic electron or positron), transforming into an isobar of that nuclide. For example, beta decay of a neutron ...
. The primary
decay product In nuclear physics, a decay product (also known as a daughter product, daughter isotope, radio-daughter, or daughter nuclide) is the remaining nuclide left over from radioactive decay. Radioactive decay often proceeds via a sequence of steps ( d ...
s before 166Er are
holmium Holmium is a chemical element; it has symbol Ho and atomic number 67. It is a rare-earth element and the eleventh member of the lanthanide series. It is a relatively soft, silvery, fairly corrosion-resistant and malleable metal. Like many other ...
isotopes, and the primary products after are
thulium Thulium is a chemical element; it has symbol Tm and atomic number 69. It is the thirteenth element in the lanthanide series of metals. It is the second-least abundant lanthanide in the Earth's crust, after radioactively unstable promethium. It i ...
isotopes. All isotopes of erbium are either radioactive or
observationally stable Stable nuclides are isotopes of a chemical element whose nucleons are in a configuration that does not permit them the surplus energy required to produce a radioactive emission. The nuclei of such isotopes are not radioactive and unlike radionuc ...
, meaning that they are predicted to be radioactive but no actual decay has been observed.


List of isotopes

, -id=Erbium-143 , 143Er , style="text-align:right" , 68 , style="text-align:right" , 75 , 142.96655(43)# , 200# ms , , , 9/2−# , , , -id=Erbium-144 , 144Er , style="text-align:right" , 68 , style="text-align:right" , 76 , 143.96070(21)# , 400# ms
200 ns, , , 0+ , , , -id=Erbium-145 , rowspan=2, 145Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 77 , rowspan=2, 144.95787(22)# , rowspan=2, 900(200) ms , β+ , 145Ho , rowspan=2, 1/2+# , rowspan=2, , rowspan=2, , - , β+, p (?%) , 144Dy , -id=Erbium-145m , rowspan=2 style="text-indent:1em" , 145mEr , rowspan=2 colspan="3" style="text-indent:2em" , 205(4)# keV , rowspan=2, 1.0(3) s , β+ , 145Ho , rowspan=2, (11/2-) , rowspan=2, , rowspan=2, , - , β+, p (?%) , 144Dy , -id=Erbium-146 , rowspan=2, 146Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 78 , rowspan=2, 145.952418(7) , rowspan=2, 1.7(6) s , β+ , 146Ho , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β+, p (?%) , 145Dy , -id=Erbium-147 , rowspan=2, 147Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 79 , rowspan=2, 146.94996(4)# , rowspan=2, 3.2(12) s , β+ , 147Ho , rowspan=2, (1/2+) , rowspan=2, , rowspan=2, , - , β+, p (?%) , 146Dy , -id=Erbium-147m , rowspan=2 style="text-indent:1em" , 147mErOrder of ground state and isomer is uncertain. , rowspan=2 colspan="3" style="text-indent:2em" , 100(50)# keV , rowspan=2, 1.6(2) s , β+ , 147Ho , rowspan=2, (11/2−) , rowspan=2, , rowspan=2, , - , β+, p (?%) , 146Dy , -id=Erbium-148 , rowspan=2, 148Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 80 , rowspan=2, 147.944735(11)# , rowspan=2, 4.6(2) s , β+ (99.85%) , 148Ho , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β+, p (0.15%) , 147Dy , -id=Erbium-148m , style="text-indent:1em" , 148mEr , colspan="3" style="text-indent:2em" , 2.9132(4) MeV , 13(3) μs , IT , 148Er , (10+) , , , -id=Erbium-149 , rowspan=2, 149Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 81 , rowspan=2, 148.94231(3) , rowspan=2, 4(2) s , β+ (93%) , 149Ho , rowspan=2, (1/2+) , rowspan=2, , rowspan=2, , - , β+, p (7%) , 148Dy , -id=Erbium-149m1 , rowspan=3 style="text-indent:1em" , 149m1Er , rowspan=3 colspan="3" style="text-indent:2em" , 741.8(2) keV , rowspan=3, 8.9(2) s , β+ (96.3%) , 149Ho , rowspan=3, (11/2−) , rowspan=3, , rowspan=3, , - , IT (3.5%) , 149Er , - , β+, p (0.18%) , 148Dy , -id=Erbium-149m2 , style="text-indent:1em" , 149m2Er , colspan="3" style="text-indent:2em" , 2.6111(3) MeV , 0.61(8) μs , IT , 149Er , (19/2+) , , , -id=Erbium-149m3 , style="text-indent:1em" , 149m3Er , colspan="3" style="text-indent:2em" , 3.302(7) MeV , 4.8(1) μs , IT , 149Er , (27/2−) , , , -id=Erbium-150 , 150Er , style="text-align:right" , 68 , style="text-align:right" , 82 , 149.937916(18) , 18.5(7) s , β+ , 150Ho , 0+ , , , -id=Erbium-150m , style="text-indent:1em" , 150mEr , colspan="3" style="text-indent:2em" , 2.7965(5) MeV , 2.55(10) μs , IT , 150Er , 10+ , , , -id=Erbium-151 , 151Er , style="text-align:right" , 68 , style="text-align:right" , 83 , 150.937449(18) , 23.5(20) s , β+ , 151Ho , (7/2−) , , , -id=Erbium-151m1 , rowspan=2 style="text-indent:1em" , 151m1Er , rowspan=2 colspan="3" style="text-indent:2em" , 2.5860(5) MeV , rowspan=2, 580(20) ms , IT (95.3%) , 151Er , rowspan=2, (27/2−) , rowspan=2, , rowspan=2, , - , β+ (4.7%) , 151Ho , -id=Erbium-151m2 , style="text-indent:1em" , 151m2Er , colspan="3" style="text-indent:2em" , 10.2866(10) MeV , 0.42(5) μs , IT , 151Er , (65/2-, 61/2+) , , , -id=Erbium-152 , rowspan=2, 152Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 84 , rowspan=2, 151.935050(9) , rowspan=2, 10.3(1) s , α (90%) , 148Dy , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , β+ (10%) , 152Ho , -id=Erbium-153 , rowspan=2, 153Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 85 , rowspan=2, 152.935086(10) , rowspan=2, 37.1(2) s , α (53%) , 149Dy , rowspan=2, 7/2− , rowspan=2, , rowspan=2, , - , β+ (47%) , 153Ho , -id=Erbium-153m1 , style="text-indent:1em" , 153m1Er , colspan="3" style="text-indent:2em" , 2.7982(10) MeV , 373(9) ns , IT , 153Er , (27/2-) , , , -id=Erbium-153m2 , style="text-indent:1em" , 153m2Er , colspan="3" style="text-indent:2em" , 5.2481(10) MeV , 248(32) ns , IT , 153Er , (41/2-) , , , -id=Erbium-154 , rowspan=2, 154Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 86 , rowspan=2, 153.932791(5) , rowspan=2, 3.73(9) min , β+ (99.53%) , 154Ho , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , α (0.47%) , 150Dy , -id=Erbium-155 , rowspan=2, 155Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 87 , rowspan=2, 154.933216(7) , rowspan=2, 5.3(3) min , β+ (99.978%) , 155Ho , rowspan=2, 7/2− , rowspan=2, , rowspan=2, , - , α (0.022%) , 151Dy , -id=Erbium-156 , rowspan=2, 156Er , rowspan=2 style="text-align:right" , 68 , rowspan=2 style="text-align:right" , 88 , rowspan=2, 155.931066(26) , rowspan=2, 19.5(10) min , β+ , 156Ho , rowspan=2, 0+ , rowspan=2, , rowspan=2, , - , α (1.2%) , 152Dy , -id=Erbium-157 , 157Er , style="text-align:right" , 68 , style="text-align:right" , 89 , 156.931923(28) , 18.65(10) min , β+ , 157Ho , 3/2− , , , -id=Erbium-157m , style="text-indent:1em" , 157mEr , colspan="3" style="text-indent:2em" , 155.4(3) keV , 76(6) ms , IT , 157Er , 9/2+ , , , -id=Erbium-158 , 158Er , style="text-align:right" , 68 , style="text-align:right" , 90 , 157.929893(27) , 2.29(6) h , EC , 158Ho , 0+ , , , -id=Erbium-159 , 159Er , style="text-align:right" , 68 , style="text-align:right" , 91 , 158.930691(4) , 36(1) min , β+ , 159Ho , 3/2− , , , -id=Erbium-159m1 , style="text-indent:1em" , 159m1Er , colspan="3" style="text-indent:2em" , 182.602(24) keV , 337(14) ns , IT , 159Er , 9/2+ , , , -id=Erbium-159m2 , style="text-indent:1em" , 159m2Er , colspan="3" style="text-indent:2em" , 429.05(3) keV , 590(60) ns , IT , 159Er , 11/2− , , , -id=Erbium-160 , 160Er , style="text-align:right" , 68 , style="text-align:right" , 92 , 159.929077(26) , 28.58(9) h , EC , 160Ho , 0+ , , , -id=Erbium-161 , 161Er , style="text-align:right" , 68 , style="text-align:right" , 93 , 160.930004(9) , 3.21(3) h , β+ , 161Ho , 3/2− , , , -id=Erbium-161m , style="text-indent:1em" , 161mEr , colspan="3" style="text-indent:2em" , 396.44(4) keV , 7.5(7) μs , IT , 161Er , 11/2− , , , -id=Erbium-162 , 162Er , style="text-align:right" , 68 , style="text-align:right" , 94 , 161.9287873(8) , colspan=3 align=center,
Observationally Stable Stable nuclides are isotopes of a chemical element whose nucleons are in a configuration that does not permit them the surplus energy required to produce a radioactive emission. The nuclei of such isotopes are not radioactive and unlike radionuc ...
Believed to undergo α decay to 158Dy or β+β+ to 162Dy with a
half-life Half-life is a mathematical and scientific description of exponential or gradual decay. Half-life, half life or halflife may also refer to: Film * Half-Life (film), ''Half-Life'' (film), a 2008 independent film by Jennifer Phang * ''Half Life: ...
over 1.40 years
, 0+ , 0.00139(5) , , -id=Erbium-162m , style="text-indent:1em" , 162mEr , colspan="3" style="text-indent:2em" , 2.02601(13) MeV , 88(16) ns , IT , 162Er , 7(-) , , , -id=Erbium-163 , 163Er , style="text-align:right" , 68 , style="text-align:right" , 95 , 162.930040(5) , 75.0(4) min , β+ , 163Ho , 5/2− , , , -id=Erbium-163m , style="text-indent:1em" , 163mEr , colspan="3" style="text-indent:2em" , 445.5(6) keV , 580(100) ns , IT , 163Er , (11/2−) , , , -id=Erbium-164 , 164Er , style="text-align:right" , 68 , style="text-align:right" , 96 , 163.9292077(8) , colspan=3 align=center, Observationally StableBelieved to undergo α decay to 160Dy or β+β+ to 164Dy , 0+ , 0.01601(3) , , -id=Erbium-165 , 165Er , style="text-align:right" , 68 , style="text-align:right" , 97 , 164.9307335(10) , 10.36(4) h , EC , 165Ho , 5/2− , , , -id=Erbium-165m1 , style="text-indent:1em" , 165m1Er , colspan="3" style="text-indent:2em" , 551.3(6) keV , 250(30) ns , IT , 165Er , 11/2- , , , -id=Erbium-165m2 , style="text-indent:1em" , 165m2Er , colspan="3" style="text-indent:2em" , 1.8230(6) MeV , 370(40) ns , IT , 165Er , (19/2) , , , -id=Erbium-166 , 166Er , style="text-align:right" , 68 , style="text-align:right" , 98 , 165.9303011(4) , colspan=3 align=center, Observationally StableBelieved to undergo α decay to 162Dy , 0+ , 0.33503(36) , , -id=Erbium-167 , 167Er , style="text-align:right" , 68 , style="text-align:right" , 99 , 166.9320562(3) , colspan=3 align=center, Observationally StableBelieved to undergo α decay to 163Dy , 7/2+ , 0.22869(9) , , -id=Erbium-167m , style="text-indent:1em" , 167mEr , colspan="3" style="text-indent:2em" , 207.801(5) keV , 2.269(6) s , IT , 167Er , 1/2− , , , -id=Erbium-168 , 168Er , style="text-align:right" , 68 , style="text-align:right" , 100 , 167.93237828(28) , colspan=3 align=center, Observationally StableBelieved to undergo α decay to 164Dy , 0+ , 0.26978(18) , , -id=Erbium-168m , style="text-indent:1em" , 168mEr , colspan="3" style="text-indent:2em" , 1.0940383(16) MeV , 109.0(7) ns , IT , 168Er , 4- , , , -id=Erbium-169 , 169Er , style="text-align:right" , 68 , style="text-align:right" , 101 , 168.9345984(3) , 9.392(18) d , β , 169Tm , 1/2− , , , -id=Erbium-169m1 , style="text-indent:1em" , 169m1Er , colspan="3" style="text-indent:2em" , 92.05(10) keV , 285(20) ns , IT , 169Er , (5/2)- , , , -id=Erbium-169m2 , style="text-indent:1em" , 169m2Er , colspan="3" style="text-indent:2em" , 243.69(17) keV , 200(10) ns , IT , 169Er , 7/2+ , , , -id=Erbium-170 , 170Er , style="text-align:right" , 68 , style="text-align:right" , 102 , 169.9354719(15) , colspan=3 align=center, Observationally StableBelieved to undergo α decay to 166Dy or ββ to 170Yb with a half-life over 4.10 years , 0+ , 0.14910(36) , , -id=Erbium-171 , 171Er , style="text-align:right" , 68 , style="text-align:right" , 103 , 170.93803746(15) , 7.516(2) h , β , 171Tm , 5/2− , , , -id=Erbium-171m , style="text-indent:1em" , 171mEr , colspan="3" style="text-indent:2em" , 198.61(9) keV , 210(10) ns , IT , 171Er , 1/2− , , , -id=Erbium-172 , 172Er , style="text-align:right" , 68 , style="text-align:right" , 104 , 171.939363(4) , 49.3(5) h , β , 172Tm , 0+ , , , - , -id=Erbium-172m , style="text-indent:1em" , 172mEr , colspan="3" style="text-indent:2em" , 1.5009(3) MeV , 579(62) ns , IT , 172Er , (6+) , , , -id=Erbium-173 , 173Er , style="text-align:right" , 68 , style="text-align:right" , 105 , 172.94240(21)# , 1.434(17) min , β , 173Tm , (7/2−) , , , -id=Erbium-174 , 174Er , style="text-align:right" , 68 , style="text-align:right" , 106 , 173.94423(32)# , 3.2(2) min , β , 174Tm , 0+ , , , -id=Erbium-174m , style="text-indent:1em" , 174mEr , colspan="3" style="text-indent:2em" , 1.1115(7) MeV , 3.9(3) s , IT , 174Er , 8- , , , -id=Erbium-175 , 175Er , style="text-align:right" , 68 , style="text-align:right" , 107 , 174.94777(43)# , 1.2(3) min , β , 175Tm , 9/2+# , , , -id=Erbium-176 , 176Er , style="text-align:right" , 68 , style="text-align:right" , 108 , 175.94994(43)# , 12# s
300 ns, , , 0+ , , , -id=Erbium-177 , 177Er , style="text-align:right" , 68 , style="text-align:right" , 109 , 176.95399(54)# , 8# s
300 ns, , , 1/2−# , , , -id=Erbium-178 , 178Er , style="text-align:right" , 68 , style="text-align:right" , 110 , 177.95678(64)# , 4# s
300 ns, , , 0+ , , , -id=Erbium-179 , 179Er , style="text-align:right" , 68 , style="text-align:right" , 111 , 178.96127(54)# , 3# s
550 ns), , , 3/2−# , , , -id=Erbium-180 , 180Er , style="text-align:right" , 68 , style="text-align:right" , 112 , 179.96438(54)# , 2# s
550 ns, , , 0+ , ,


See also

Daughter products other than erbium * Isotopes of thulium *
Isotopes of holmium Natural holmium (67Ho) contains one observationally stable isotope, 165Ho. The below table lists 39 isotopes spanning 140Ho through 178Ho as well as 40 nuclear isomers. Among the known synthetic radioactive isotopes; the most stable one is 16 ...
*
Isotopes of dysprosium Naturally occurring dysprosium (66Dy) is composed of 7 stable isotopes, 156Dy, 158Dy, 160Dy, 161Dy, 162Dy, 163Dy and 164Dy, with 164Dy being the most abundant (28.18% natural abundance). Twenty-nine radioisotopes have been characterized, with the ...


References

* Isotope masses from: ** * Isotopic compositions and standard atomic masses from: ** ** ** * Half-life, spin, and isomer data selected from the following sources. ** ** ** {{Navbox element isotopes Erbium
Erbium Erbium is a chemical element; it has Symbol (chemistry), symbol Er and atomic number 68. A silvery-white solid metal when artificially isolated, natural erbium is always found in chemical combination with other elements. It is a lanthanide, a rare- ...