Isotopes of silver
   HOME

TheInfoList



OR:

Naturally occurring
silver Silver is a chemical element with the symbol Ag (from the Latin ', derived from the Proto-Indo-European ''h₂erǵ'': "shiny" or "white") and atomic number 47. A soft, white, lustrous transition metal, it exhibits the highest electrical ...
(47Ag) is composed of the two stable
isotope Isotopes are two or more types of atoms that have the same atomic number (number of protons in their nuclei) and position in the periodic table (and hence belong to the same chemical element), and that differ in nucleon numbers (mass numb ...
s 107Ag and 109Ag in almost equal proportions, with 107Ag being slightly more abundant (51.839%
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 atomi ...
). 40
radioisotope A radionuclide (radioactive nuclide, radioisotope or radioactive isotope) is a nuclide that has excess nuclear energy, making it unstable. This excess energy can be used in one of three ways: emitted from the nucleus as gamma radiation; transferr ...
s have been characterized with the most stable being 105Ag with a
half-life Half-life (symbol ) is the time required for a quantity (of substance) to reduce to half of its initial value. The term is commonly used in nuclear physics to describe how quickly unstable atoms undergo radioactive decay or how long stable at ...
of 41.29 days, 111Ag with a half-life of 7.43 days, and 112Ag with a half-life of 3.13 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 consi ...
isotopes have half-lives that are less than an hour, and the majority of these have half-lives that are less than 3 minutes. This element 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 higher energy levels than in the ground state of the same nucleus. "Metastable" describes nuclei whose excited states have ...
s, with the most stable being 108mAg (half-life 439 years), 110mAg (half-life 249.86 days) and 106mAg (half-life 8.28 days). Isotopes of silver 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 91.960  u (92Ag) to 132.969 u (133Ag). The primary decay mode before the most abundant stable isotope, 107Ag, 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. Thi ...
and the primary mode after is
beta decay In nuclear physics, beta decay (β-decay) is a type of radioactive decay in which a beta particle (fast energetic electron or positron) is emitted from an atomic nucleus, transforming the original nuclide to an isobar of that nuclide. For ...
. The primary decay products before 107Ag are
palladium Palladium is a chemical element with the symbol Pd and atomic number 46. It is a rare and lustrous silvery-white metal discovered in 1803 by the English chemist William Hyde Wollaston. He named it after the asteroid Pallas, which was itself na ...
(element 46) isotopes and the primary products after are
cadmium Cadmium is a chemical element with the symbol Cd and atomic number 48. This soft, silvery-white metal is chemically similar to the two other stable metals in group 12, zinc and mercury. Like zinc, it demonstrates oxidation state +2 in most of ...
(element 48) isotopes. The palladium
isotope Isotopes are two or more types of atoms that have the same atomic number (number of protons in their nuclei) and position in the periodic table (and hence belong to the same chemical element), and that differ in nucleon numbers (mass numb ...
107Pd decays by beta emission to 107Ag with a half-life of 6.5 million years.
Iron Iron () is a chemical element with Symbol (chemistry), symbol Fe (from la, Wikt:ferrum, ferrum) and atomic number 26. It is a metal that belongs to the first transition series and group 8 element, group 8 of the periodic table. It is, Abundanc ...
meteorites are the only objects with a high enough palladium/silver ratio to yield measurable variations in 107Ag abundance.
Radiogenic A radiogenic nuclide is a nuclide that is produced by a process of radioactive decay. It may itself be radioactive (a radionuclide) or stable (a stable nuclide). Radiogenic nuclides (more commonly referred to as radiogenic isotopes) form some ...
107Ag was first discovered in the Santa Clara meteorite in 1978. The discoverers suggest that the coalescence and differentiation of iron-cored small
planet A planet is a large, rounded astronomical body that is neither a star nor its remnant. The best available theory of planet formation is the nebular hypothesis, which posits that an interstellar cloud collapses out of a nebula to create a you ...
s may have occurred 10 million years after a
nucleosynthetic Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons (protons and neutrons) and nuclei. According to current theories, the first nuclei were formed a few minutes after the Big Bang, through nuclear reactions in ...
event. 107Pd versus 107Ag correlations observed in bodies, which have clearly been melted since the accretion of the
Solar System The Solar System Capitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Solar ...
, must reflect the presence of live short-lived nuclides in the early Solar System.


List of isotopes

, - , rowspan=2 , 92Ag , rowspan=2 , 47 , rowspan=2 , 45 , rowspan=2 , 91.95971(43)# , rowspan=2, 1# ms
400 ns, β+ , 92Pd , rowspan=2, , rowspan=2, , rowspan=2, , - , p , 91Pd , - , rowspan=3 , 93Ag , rowspan=3 , 47 , rowspan=3 , 46 , rowspan=3 , 92.95019(43)# , rowspan=3, 228(16) ns , β+ , 93Pd , rowspan=3, 9/2+# , rowspan=3, , rowspan=3, , - , p , 92Pd , - , β+, p , 92Rh , - , rowspan=2, 94Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 47 , rowspan=2, 93.94374(43)# , rowspan=2, 27(2) ms , β+ (>99.8%) , 94Pd , rowspan=2, 0+# , rowspan=2, , rowspan=2, , - , β+, p (<0.2%) , 93Rh , - , rowspan=2 style="text-indent:1em" , 94m1Ag , rowspan=2 colspan="3" style="text-indent:2em" , 1350(400)# keV , rowspan=2, 470(10) ms , β+ (83%) , 94Pd , rowspan=2, (7+) , rowspan=2, , rowspan=2, , - , β+, p (17%) , 93Rh , - , rowspan=4 style="text-indent:1em" , 94m2Ag , rowspan=4 colspan="3" style="text-indent:2em" , 6500(550)# keV , rowspan=4, 400(40) ms , β+ (~68.4%) , 94Pd , rowspan=4, (21+) , rowspan=4, , rowspan=4, , - , β+, p (~27%) , 93Rh , - , p (4.1%) , 93Pd , - , 2p (0.5%) , 92Rh , - , rowspan=2, 95Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 48 , rowspan=2, 94.93569(43)# , rowspan=2, 1.78(6) s , β+ (97.7%) , 95Pd , rowspan=2, (9/2+) , rowspan=2, , rowspan=2, , - , β+, p (2.3%) , 94Rh , - , style="text-indent:1em" , 95m1Ag , colspan="3" style="text-indent:2em" , 344.2(3) keV , <0.5 s , IT , 95Ag , (1/2−) , , , - , style="text-indent:1em" , 95m2Ag , colspan="3" style="text-indent:2em" , 2531.3(15) keV , <16 ms , IT , 95Ag , (23/2+) , , , - , style="text-indent:1em" , 95m3Ag , colspan="3" style="text-indent:2em" , 4860.0(15) keV , <40 ms , IT , 95Ag , (37/2+) , , , - , rowspan=2, 96Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 49 , rowspan=2, 95.93074(10) , rowspan=2, 4.45(3) s , β+ (95.8%) , 96Pd , rowspan=2, (8+) , rowspan=2, , rowspan=2, , - , β+, p (4.2%) , 95Rh , - , rowspan=2 style="text-indent:1em" , 96m1Ag , rowspan=2 colspan="3" style="text-indent:2em" , 0(50)# keV , rowspan=2, 6.9(5) s , β+ (85.1%) , 96Pd , rowspan=2, (2+) , rowspan=2, , rowspan=2, , - , β+, p (14.9%) , 95Rh , - , style="text-indent:1em" , 96m2Ag , colspan="3" style="text-indent:2em" , 2461.4(3) keV , 103.2(45) μs , IT , 96Ag , (13-) , , , - , style="text-indent:1em" , 96m3Ag , colspan="3" style="text-indent:2em" , 2686.7(4) keV , 1.561(16) μs , IT , 96Ag , (15+) , , , - , style="text-indent:1em" , 96m4Ag , colspan="3" style="text-indent:2em" , 6951.8(14) keV , 132(17) ns , IT , 96Ag , (19+) , , , - , 97Ag , style="text-align:right" , 47 , style="text-align:right" , 50 , 96.923881(13) , 25.5(3) s , β+ , 97Pd , (9/2+) , , , - , style="text-indent:1em" , 97mAg , colspan="3" style="text-indent:2em" , 620(40) keV , 100# ms , , , (1/2-#) , , , - , rowspan=2, 98Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 51 , rowspan=2, 97.92156(4) , rowspan=2, 47.5(3) s , β+ (99.99%) , 98Pd , rowspan=2, (6)+ , rowspan=2, , rowspan=2, , - , β+, p (.0012%) , 97Rh , - , style="text-indent:1em" , 98mAg , colspan="3" style="text-indent:2em" , 107.28(10) keV , 161(7) ns , IT , 98Ag , (4+) , , , - , 99Ag , style="text-align:right" , 47 , style="text-align:right" , 52 , 98.917646(7) , 2.07(5) min , β+ , 99Pd , (9/2)+ , , , - , style="text-indent:1em" , 99mAg , colspan="3" style="text-indent:2em" , 506.2(4) keV , 10.5(5) s , IT , 99Ag , (1/2−) , , , - , 100Ag , style="text-align:right" , 47 , style="text-align:right" , 53 , 99.916115(5) , 2.01(9) min , β+ , 100Pd , (5)+ , , , - , rowspan=2 style="text-indent:1em" , 100mAg , rowspan=2 colspan="3" style="text-indent:2em" , 15.52(16) keV , rowspan=2, 2.24(13) min , IT , 100Ag , rowspan=2, (2)+ , rowspan=2, , rowspan=2, , - , β+ , 100Pd , - , 101Ag , style="text-align:right" , 47 , style="text-align:right" , 54 , 100.912684(5) , 11.1(3) min , β+ , 101Pd , 9/2+ , , , - , style="text-indent:1em" , 101mAg , colspan="3" style="text-indent:2em" , 274.1(3) keV , 3.10(10) s , IT , 101Ag , 1/2− , , , - , 102Ag , style="text-align:right" , 47 , style="text-align:right" , 55 , 101.911705(9) , 12.9(3) min , β+ , 102Pd , 5+ , , , - , rowspan=2 style="text-indent:1em" , 102mAg , rowspan=2 colspan="3" style="text-indent:2em" , 9.40(7) keV , rowspan=2, 7.7(5) min , β+ (51%) , 102Pd , rowspan=2, 2+ , rowspan=2, , rowspan=2, , - , IT (49%) , 102Ag , - , 103Ag , style="text-align:right" , 47 , style="text-align:right" , 56 , 102.908961(4) , 65.7(7) min , β+ , 103Pd , 7/2+ , , , - , style="text-indent:1em" , 103mAg , colspan="3" style="text-indent:2em" , 134.45(4) keV , 5.7(3) s , IT , 103Ag , 1/2− , , , - , 104Ag , style="text-align:right" , 47 , style="text-align:right" , 57 , 103.908624(5) , 69.2(10) min , β+ , 104Pd , 5+ , , , - , rowspan=2 style="text-indent:1em" , 104mAg , rowspan=2 colspan="3" style="text-indent:2em" , 6.90(22) keV , rowspan=2, 33.5(20) min , β+ (>99.93%) , 104Pd , rowspan=2, 2+ , rowspan=2, , rowspan=2, , - , IT (<0.07%) , 104Ag , - , 105Ag , style="text-align:right" , 47 , style="text-align:right" , 58 , 104.906526(5) , 41.29(7) d , β+ , 105Pd , 1/2− , , , - , rowspan=2 style="text-indent:1em" , 105mAg , rowspan=2 colspan="3" style="text-indent:2em" , 25.468(16) keV , rowspan=2, 7.23(16) min , IT (99.66%) , 105Ag , rowspan=2, 7/2+ , rowspan=2, , rowspan=2, , - , β+ (.34%) , 105Pd , - , rowspan=2, 106Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 59 , rowspan=2, 105.906663(3) , rowspan=2, 23.96(4) min , β+ , 106Pd , rowspan=2, 1+ , rowspan=2, , rowspan=2, , - , β (rare) , 106Cd , - , rowspan=2 style="text-indent:1em" , 106mAg , rowspan=2 colspan="3" style="text-indent:2em" , 89.66(7) keV , rowspan=2, 8.28(2) d , β+ , 106Pd , rowspan=2, 6+ , rowspan=2, , rowspan=2, , - , IT (rare) , 106Ag , - , 107AgUsed to date certain events in the early history of the Solar System , style="text-align:right" , 47 , style="text-align:right" , 60 , 106.9050915(26) , colspan=3 align=center, StableTheoretically capable of spontaneous fission , 1/2− , 0.51839(8) , , - , style="text-indent:1em" , 107mAg , colspan="3" style="text-indent:2em" , 93.125(19) keV , 44.3(2) s , IT , 107Ag , 7/2+ , , , - , rowspan=2, 108Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 61 , rowspan=2, 107.9059502(26) , rowspan=2, 2.382(11) min , β (97.15%) , 108Cd , rowspan=2, 1+ , rowspan=2, , rowspan=2, , - , β+ (2.85%) , 108Pd , - , rowspan=2 style="text-indent:1em" , 108mAg , rowspan=2 colspan="3" style="text-indent:2em" , 109.466(7) keV , rowspan=2, 439(9) y , β+ (91.3%) , 108Pd , rowspan=2, 6+ , rowspan=2, , rowspan=2, , - , IT (8.96%) , 108Ag , - , 109Ag Fission product , style="text-align:right" , 47 , style="text-align:right" , 62 , 108.9047558(14) , colspan=3 align=center, Stable , 1/2− , 0.48161(8) , , - , style="text-indent:1em" , 109mAg , colspan="3" style="text-indent:2em" , 88.0337(10) keV , 39.79(21) s , IT , 109Ag , 7/2+ , , , - , rowspan=2, 110Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 63 , rowspan=2, 109.9061107(14) , rowspan=2, 24.56(11) s , β (99.7%) , 110Cd , rowspan=2, 1+ , rowspan=2, , rowspan=2, , - , EC (.3%) , 110Pd , - , style="text-indent:1em" , 110m1Ag , colspan="3" style="text-indent:2em" , 1.112(16) keV , 660(40) ns , IT , 110Ag , 2− , , , - , rowspan=2 style="text-indent:1em" , 110m2Ag , rowspan=2 colspan="3" style="text-indent:2em" , 117.59(5) keV , rowspan=2, 249.863(24) d , β (98.67%) , 110Cd , rowspan=2, 6+ , rowspan=2, , rowspan=2, , - , IT (1.33%) , 110Ag , - , 111Ag , style="text-align:right" , 47 , style="text-align:right" , 64 , 110.9052968(16) , 7.433(10) d , β , 111Cd , 1/2− , , , - , rowspan=2 style="text-indent:1em" , 111mAg , rowspan=2 colspan="3" style="text-indent:2em" , 59.82(4) keV , rowspan=2, 64.8(8) s , IT (99.3%) , 111Ag , rowspan=2, 7/2+ , rowspan=2, , rowspan=2, , - , β (.7%) , 111Cd , - , 112Ag , style="text-align:right" , 47 , style="text-align:right" , 65 , 111.9070485(26) , 3.130(8) h , β , 112Cd , 2(−) , , , - , 113Ag , style="text-align:right" , 47 , style="text-align:right" , 66 , 112.906573(18) , 5.37(5) h , β , 113mCd , 1/2− , , , - , rowspan=2 style="text-indent:1em" , 113mAg , rowspan=2 colspan="3" style="text-indent:2em" , 43.50(10) keV , rowspan=2, 68.7(16) s , IT (64%) , 113Ag , rowspan=2, 7/2+ , rowspan=2, , rowspan=2, , - , β (36%) , ''113Cd'' , - , 114Ag , style="text-align:right" , 47 , style="text-align:right" , 67 , 113.908823(5) , 4.6(1) s , β , 114Cd , 1+ , , , - , style="text-indent:1em" , 114mAg , colspan="3" style="text-indent:2em" , 198.9(10) keV , 1.50(5) ms , IT , 114Ag , (6+) , , , - , 115Ag , style="text-align:right" , 47 , style="text-align:right" , 68 , 114.908767(20) , 20.0(5) min , β , 115mCd , 1/2− , , , - , rowspan=2 style="text-indent:1em" , 115mAg , rowspan=2 colspan="3" style="text-indent:2em" , 41.16(10) keV , rowspan=2, 18.0(7) s , β (79%) , 115Cd , rowspan=2, 7/2+ , rowspan=2, , rowspan=2, , - , IT (21%) , 115Ag , - , 116Ag , style="text-align:right" , 47 , style="text-align:right" , 69 , 115.911387(4) , 3.83(8) min , β , ''116Cd'' , (0-) , , , - , rowspan=2 style="text-indent:1em" , 116m1Ag , rowspan=2 colspan="3" style="text-indent:2em" , 47.90(10) keV , rowspan=2, 20(1) s , β (93%) , ''116Cd'' , rowspan=2, (3+) , rowspan=2, , rowspan=2, , - , IT (7%) , 116Ag , - , rowspan=2 style="text-indent:1em" , 116m2Ag , rowspan=2 colspan="3" style="text-indent:2em" , 129.80(22) keV , rowspan=2, 9.3(3) s , β (92%) , ''116Cd'' , rowspan=2, (6-) , rowspan=2, , rowspan=2, , - , IT (8%) , 116Ag , - , 117Ag , style="text-align:right" , 47 , style="text-align:right" , 70 , 116.911774(15) , 73.6(14) s , β , 117mCd , 1/2−# , , , - , rowspan=2 style="text-indent:1em" , 117mAg , rowspan=2 colspan="3" style="text-indent:2em" , 28.6(2) keV , rowspan=2, 5.34(5) s , β (94%) , 117mCd , rowspan=2, 7/2+# , rowspan=2, , rowspan=2, , - , IT (6%) , 117Ag , - , 118Ag , style="text-align:right" , 47 , style="text-align:right" , 71 , 117.9145955(27) , 3.76(15) s , β , 118Cd , (2-) , , , - , style="text-indent:1em" , 118m1Ag , colspan="3" style="text-indent:2em" , 45.79(9) keV , ~0.1 µs , IT , 118Ag , 1(−) to 2(−) , , , - , rowspan=2 style="text-indent:1em" , 118m2Ag , rowspan=2 colspan="3" style="text-indent:2em" , 127.63(10) keV , rowspan=2, 2.0(2) s , β (59%) , 118Cd , rowspan=2, (5+) , rowspan=2, , rowspan=2, , - , IT (41%) , 118Ag , - , style="text-indent:1em" , 118m3Ag , colspan="3" style="text-indent:2em" , 279.37(20) keV , ~0.1 µs , IT , 118Ag , (3+) , , , - , 119Ag , style="text-align:right" , 47 , style="text-align:right" , 72 , 118.915570(16) , 6.0(5) s , β , 119mCd , 1/2−# , , , - , style="text-indent:1em" , 119mAg , colspan="3" style="text-indent:2em" , 20(20)# keV , 2.1(1) s , β , 119Cd , 7/2+# , , , - , rowspan=2, 120Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 73 , rowspan=2, 119.918785(5) , rowspan=2, 1.52(7) s , β (>99.997%) , 120Cd , rowspan=2, 4(+) , rowspan=2, , rowspan=2, , - , β, n (<.003%) , 119Cd , - , style="text-indent:1em" , 120m1Ag , colspan="3" style="text-indent:2em" , 0(50)# keV , 940(100) ms , , , (0−, 1-) , , , - , rowspan=2 style="text-indent:1em" , 120m2Ag , rowspan=2 colspan="3" style="text-indent:2em" , 203.0(10) keV , rowspan=2, 384(22) ms , IT (68%) , 120Sn , rowspan=2, 7(−) , rowspan=2, , rowspan=2, , - , β (32%) , 120Cd , - , rowspan=2, 121Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 74 , rowspan=2, 120.920125(13) , rowspan=2, 777(10) ms , β (99.92%) , 121Cd , rowspan=2, 7/2+# , rowspan=2, , rowspan=2, , - , β, n (.076%) , 120Cd , - , style="text-indent:1em" , 121mAg , colspan="3" style="text-indent:2em" , 20(20)# keV , 200# ms , , , 1/2-# , , , - , rowspan=2, 122Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 75 , rowspan=2, 121.92366(4) , rowspan=2, 529(13) ms , β (>99.814%) , 122Cd , rowspan=2, (3+) , rowspan=2, , rowspan=2, , - , β, n (.186%) , 121Cd , - , rowspan=3 style="text-indent:1em" , 122m1Ag , rowspan=3 colspan="3" style="text-indent:2em" , 80(50)# keV , rowspan=3, 550(50) ms , β , 122Cd , rowspan=3, (1-) , rowspan=3, , rowspan=3, , - , β, n (rare) , 121Cd , - , IT (rare) , 122Ag , - , rowspan=3 style="text-indent:1em" , 122m2Ag , rowspan=3 colspan="3" style="text-indent:2em" , 80(50)# keV , rowspan=3, 200(50) ms , β , 122Cd , rowspan=3, (9-) , rowspan=3, , rowspan=3, , - , β, n (rare) , 121Cd , - , IT (rare) , 122Ag , - , style="text-indent:1em" , 122m3Ag , colspan="3" style="text-indent:2em" , 171(50)# keV , 6.3(1) μs , IT , 122Ag , (1+) , , , - , rowspan=2, 123Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 76 , rowspan=2, 122.92532(4) , rowspan=2, 294(5) ms , β (99.44%) , 123Cd , rowspan=2, (7/2+) , rowspan=2, , rowspan=2, , - , β, n (.56%) , 122Cd , - , rowspan=2 style="text-indent:1em" , 123m1Ag , rowspan=2 colspan="3" style="text-indent:2em" , 59.5(5) keV , rowspan=2, 100# ms , β , 123Cd , rowspan=2, (1/2-) , rowspan=2, , rowspan=2, , - , β, n (rare) , 122Cd , - , style="text-indent:1em" , 123m2Ag , colspan="3" style="text-indent:2em" , 1450(14)# keV , 202(20) ns , IT , 123Ag , , , , - , style="text-indent:1em" , 123m3Ag , colspan="3" style="text-indent:2em" , 1472.8(8) keV , 393(16) ns , IT , 123Ag , (17/2-) , , , - , rowspan=2, 124Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 77 , rowspan=2, 123.92890(27)# , rowspan=2, 177.9(26) ms , β (98.7%) , 124Cd , rowspan=2, (2-) , rowspan=2, , rowspan=2, , - , β, n (1.3%) , 123Cd , - , rowspan=2 style="text-indent:1em" , 124m1Ag , rowspan=2 colspan="3" style="text-indent:2em" , 50(50)# keV , rowspan=2, 144(20) ms , β , 124Cd , rowspan=2, 9-# , rowspan=2, , rowspan=2, , - , β, n , 123Cd , - , style="text-indent:1em" , 124m2Ag , colspan="3" style="text-indent:2em" , 155.6(5)# keV , 140(50) ns , IT , 124Ag , (1+) , , , - , style="text-indent:1em" , 124m3Ag , colspan="3" style="text-indent:2em" , 231.1(7)# keV , 1.48(15) μs , IT , 124Ag , (1-) , , , - , rowspan=2, 125Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 78 , rowspan=2, 124.93074(47) , rowspan=2, 160(5) ms , β (88.2%) , 125Cd , rowspan=2, (9/2+) , rowspan=2, , rowspan=2, , - , β, n (11.8%) , 124Cd , - , style="text-indent:1em" , 125m1Ag , colspan="3" style="text-indent:2em" , 97.1(5)# keV , 50# ms , , , (1/2-) , , , - , style="text-indent:1em" , 125m2Ag , colspan="3" style="text-indent:2em" , 97.1(5)# keV , 491(20) ns , , , (17/2-) , , , - , rowspan=2, 126Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 79 , rowspan=2, 125.93481(22)# , rowspan=2, 52(10) ms , β (86.3%) , 126Cd , rowspan=2, 3+# , rowspan=2, , rowspan=2, , - , β, n (13.7%) , 125Cd , - , style="text-indent:1em" , 126m1Ag , colspan="3" style="text-indent:2em" , 100(100)# keV , 108.4(24) ms , , , 9-# , , , - , style="text-indent:1em" , 126m2Ag , colspan="3" style="text-indent:2em" , 97.1(5)# keV , 27(6) μs , IT , 126Ag , 1-# , , , - , rowspan=2, 127Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 80 , rowspan=2, 126.93704(22)# , rowspan=2, 89(2) ms , β (85.4%) , 127Cd , rowspan=2, (9/2+) , rowspan=2, , rowspan=2, , - , β, n (14.6%) , 126Cd , - , style="text-indent:1em" , 127m1Ag , colspan="3" style="text-indent:2em" , 20(20)# keV , 20# ms , , , (1/2-) , , , - , rowspan=2 style="text-indent:1em" , 127m2Ag , rowspan=2 colspan="3" style="text-indent:2em" , 1938(17) keV , rowspan=2, 67.5(9) ms , β (91.2%) , 127Cd , rowspan=2, (27/2+) , rowspan=2, , rowspan=2, , - , IT (8.8%) , 127Ag , - , rowspan=2, 128Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 81 , rowspan=2, 127.94127(32)# , rowspan=2, 60(3) ms , β (80%) , 128Cd , rowspan=2, 3+# , rowspan=2, , rowspan=2, , - , β, n (20%) , 127Cd , - , rowspan=2, 129Ag , rowspan=2 style="text-align:right" , 47 , rowspan=2 style="text-align:right" , 82 , rowspan=2, 128.94432(43)# , rowspan=2, 49.9(35) ms , β (>80%) , 129Cd , rowspan=2, 9/2+# , rowspan=2, , rowspan=2, , - , β, n (<20%) , 128Cd , - , style="text-indent:1em" , 129mAg , colspan="3" style="text-indent:2em" , 20(20)# keV , 10# ms , , , 1/2−# , , , - , 130Ag , style="text-align:right" , 47 , style="text-align:right" , 83 , 129.95073(46)# , 40.6(45) ms , β , 130Cd , 1-# , , , - , rowspan=3, 131Ag , rowspan=3 style="text-align:right" , 47 , rowspan=3 style="text-align:right" , 84 , rowspan=3, 130.95625(54)# , rowspan=3, 35(8) ms , β , 131Cd , rowspan=3, 9/2+# , rowspan=3, , rowspan=3, , - , β, n , 130Cd , - , β, 2n , 129Cd , - , 132Ag , style="text-align:right" , 47 , style="text-align:right" , 85 , 131.96307(54)# , 30(14) ms , β , 132Cd , 6-# , , , - , 133Ag , style="text-align:right" , 47 , style="text-align:right" , 86 , 132.96878(54)# , , , , 6-# , ,


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 Silver
Silver Silver is a chemical element with the symbol Ag (from the Latin ', derived from the Proto-Indo-European ''h₂erǵ'': "shiny" or "white") and atomic number 47. A soft, white, lustrous transition metal, it exhibits the highest electrical ...