47
Ag
Silver
Atomic Mass 107.8682
Electron Configuration [Kr]5s14d10
Oxidation States +1
Year Discovered Ancient

Identifiers

Element Name Silver
Element Symbol Ag
InChI InChI=1S/Ag
InChIKey BQCADISMDOOEFD-UHFFFAOYSA-N

Properties

Atomic Weight

107.8682(2)

107.8682

107.9

107.8682(2)

Electron Configuration

[Kr]5s14d10

Atomic Radius

Van der Waals Atomic Radius : 172 pm (Van der Waals)

Empirical Atomic Radius : 160pm (Empirical)

Covalent Atomic Radius : 145(5) pm (Covalent)

Oxidation States

+1

-2, -1, 1, 2, 3 ​(an amphoteric oxide)

Ground Level

2S1/2

Ionization Energy

7.576 eV

7.576234 ± 0.000025 eV

Electronegativity

Pauling Scale Electronegativity : 1.93(Pauling Scale)

Allen Scale Electronegativity : 1.87(Allen Scale)

Electron Affinity

1.302eV

2eV

Atomic Spectra

Lines Holdings

Levels Holdings

Physical Description

Solid

Element Classification

Metal

Element Period Number

5

Element Group Number

11

Density

10.501 grams per cubic centimeter

Melting Point

1234.93 K (961.78°C or 1763.20°F)

961.78°C

Boiling Point

2435 K (2162°C or 3924°F)

2162°C

Estimated Crustal Abundance

7.5×10-2 milligrams per kilogram

Estimated Oceanic Abundance

4×10-5 milligrams per liter

History

The name derives from the Anglo-Saxon seofor and siolfur, which is of unknown origin. The symbol Ag derives from the Latin argentum and Sanskrit argunas from "bright". Silver was known in prehistoric times.

Archaeological evidence suggests that people have been using silver for at least 5000 years. Silver can be obtained from pure deposits, from silver ores such as argentite (Ag2S) and horn silver (AgCl), and in conjunction with deposits of ores containing lead, gold or copper.

The Latin word for silver is argentum. Silver has been known since ancient times. It is mentioned in Genesis. Slag dumps in Asia Minor and on islands in the Aegean Sea indicate that man learned to separate silver from lead as early as 3000 B.C.

Historical Atomic Weights

Year Atomic Weight (uncertainty) [u] Reference
1985 107.8682(2) https://doi.org/10.1351/pac198658121677
1981 107.8682(3) https://doi.org/10.1351/pac198355071101
1965 107.868(1) https://doi.org/10.1351/pac196918040569
1961 107.870(3) https://doi.org/10.1021/ja00881a001
1925 107.880 https://doi.org/10.1039/CT9252700913
1909 107.88 https://doi.org/10.1021/ja01931a001
1902 107.93 https://doi.org/10.1007/BF01370337

Historical Isotopic Abundances

Year Isotope Abundance (uncertainty) Reference
1997 107Ag 0.518 39(8) https://doi.org/10.1351/pac199870010217
1997 109Ag 0.481 61(8) https://doi.org/10.1351/pac199870010217
1989 107Ag 0.518 39(7) https://doi.org/10.1351/pac199163070991
1989 109Ag 0.481 61(7) https://doi.org/10.1351/pac199163070991
1975 107Ag 0.5183 https://doi.org/10.1351/pac197647010075
1975 109Ag 0.4817 https://doi.org/10.1351/pac197647010075

Description

Pure silver has a brilliant white metallic luster. It is a little harder than gold and is very ductile and malleable, being exceeded only by gold and perhaps palladium. Pure silver has the highest electrical and thermal conductivity of all metals, and possesses the lowest contact resistance. It is stable in pure air and water, but tarnishes when exposed to ozone, hydrogen sulfide, or air containing sulfur. The alloys of silver are important.

Users

Silver and silver compounds have many uses. Pure silver is the best conductor of heat and electricity of all known metals, so it is sometimes used in making solder, electrical contacts and printed circuit boards. Silver is also the best reflector of visible light known, but silver mirrors must be given a protective coating to prevent them from tarnishing. Silver has also been used to create coins, although today other metals are typically used in its place. Sterling silver, an alloy containing 92.5% silver, is used to make silverware, jewelry and other decorative items. High capacity batteries can be made with silver and zinc and silver and cadmium. Silver nitrate (AgNO3) is light sensitive and is used to make photographic films and papers. Silver iodide (AgI) is used to seed clouds to produce rain.

Sterling silver is used for jewelry, silverware, etc. where appearance is paramount. This alloy contains 92.5% silver, the remainder being copper or some other metal. Silver is of the utmost importance in photography, about 30% of the U.S. industrial consumption going into this application. It is used for dental alloys. Silver is used in making solder and brazing alloys, electrical contacts, and high capacity silver-zinc and silver-cadmium batteries. Silver paints are used for making printed circuits. It is used in mirror production and may be deposited on glass or metals by chemical deposition, electrode position, or by evaporation. When freshly deposited, it is the best reflector of visible light known, but is rapidly tarnished and loses much of its reflectance. It is a poor reflector of ultraviolet. Silver fulminate, a powerful explosive, is sometimes formed during the silvering process. Silver iodide is used in seeding clouds to produce rain. Silver chloride has interesting optical properties as it can be made transparent; it also is a cement for glass. Silver nitrate, or lunar caustic, the most important silver compound, is used extensively in photography. Silver for centuries has been used traditionally for coinage by many countries of the world. In recent times, however, consumption of silver has greatly exceeded the output.

Sources

Silver occurs natively and in ores such as argentite (Ag2S) and horn silver (AgCl); lead, lead-zinc, copper, gold, and copper-nickel ores are principal sources. Mexico, Canada, Peru, and the U.S. are the principal silver producers in the western hemisphere.

Compounds

See more information at the Silver compound page.

Element Forms

CID Name Formula SMILES Molecular Weight
23954 silver Ag [Ag] 107.868
104755 silver(1+) Ag+ [Ag+] 107.868
104828 silver-110 Ag [110Ag] 109.90611
161148 silver-111 Ag [111Ag] 110.90530
167088 silver-108 Ag [108Ag] 107.90595
167204 silver-105 Ag [105Ag] 104.90653
177527 silver-103 Ag [103Ag] 102.90896
177563 silver-104 Ag [104Ag] 103.90862
178186 silver-112 Ag [112Ag] 111.90705
178190 silver-109 Ag [109Ag] 108.90476
181324 silver-110(1+) Ag+ [110Ag+] 109.90611
167414 silver-115 Ag [115Ag] 114.9088
177478 silver-102 Ag [102Ag] 101.91170
178189 silver-106 Ag [106Ag] 105.90666
3082060 silver-107 Ag [107Ag] 106.90509
10290765 silver-113 Ag [113Ag] 112.9066

Handling And Storage

While silver itself is not considered to be toxic, most of its salts are poisonous. Exposure to silver (metal and soluble compounds, as Ag) in air should not exceed 0.01 mg/m3, (8-hour time-weighted average - 40 hour week). Silver compounds can be absorbed in the circulatory system and reduced silver deposited in the various tissues of the body. A condition, known as argyria, results with a grayish pigmentation of the skin and mucous membranes. Silver has germicidal effects and kills many lower organisms effectively without harm to higher animals.

Isotopes

Stable Isotope Count 2

Isotopes in Earth/Planetary Science

The measurement of relative amounts of 107Ag and 109Ag is used to study the processes responsible for the isotopic fractionation of silver isotopes in ore deposits, which depends on the specific minerals and environmental conditions. This is currently an area of active research and it is thought that the relative amounts of the isotopes of silver are altered during the formation of the ore [351], [352].

[351] Y. Luo, E. Dabek-Zlotorzynska, V. Celo, D. C. Muir, L. Yang. Anal. Chem.82, 3922 (2010).
[352] A. V. Chugaev, I. V. Chernyshev. Geochim. Cosmochim. Acta Suppl.73, A225 (2009).

Isotopes in Forensic Science and Anthropology

Silver isotope-amount ratiosn(107Ag)/n(109Ag) along with isotope-amount ratios of copper n(65Cu)/n(63Cu), and isotope-amount ratios of lead (n(206Pb)/n(204Pb), n(207Pb)/n(204Pb) and n(208Pb)/n(204Pb)) have been used to determine origins of European coins and information on the flow of goods in the world market over time (Fig. IUPAC.47.1). Metals from Peru and Mexico and those from European mining have distinct isotopic signatures that enable the origin of the metal to be determined by examining the isotopic compositions of silver, copper, and lead in the coins. Abundant silver sources, mined in Mexico and Peru in the 16 th century, were used to mint coins, but they were not a major influence in the European coin market until the 18 th century (Fig. IUPAC.47.1) [237].

Fig. IUPAC.47.1: Cross plot of lead model age and n(¹⁰⁹Ag)/n(¹⁰⁷Ag) isotope-amount ratio of selected coins (modified from [237]) assuming a n(¹⁰⁹Ag)/n(¹⁰⁷Ag) value of 0.929 04 for the isotopic reference material SRM 981a silver nitrate [237]. The isotopic signatures of the silver, copper, and lead in the metals used to make Spanish coins have been used to trace (see tracer) the origin of the metals to help determine the flow of metal in the global market during the 16 thcentury. The Mexico coins show little variation in the silver mole fraction, although the observed range of isotopic variation is about 30 times the analytical uncertainty. The antique coins have two groups, the oldest on the right and the younger on the left. They are statistically different at the 99-percent confidence level. The Catholic Kings coins are distinct from the rest of the medieval coins.

[237] A. M. Desaulty, P. Telouk, E. Albalat, F. Albarede. Proc. Natl. Acad. Sci.108, 9002 (2011).

Isotopes in Geochronology

The amount ratio n(107Pd)/n(107Ag) is used in geochronology to date major events in the Solar System [344], [345], [346], [347], [348], [353]. Although 107Ag is naturally occurring, it is also the daughter product by beta decay of 107Pd. If both excess 107Ag and 107Pd are present in a sample of extraterrestrial origin, then the material would have formed sometime after 107Pd decayed (i.e. sometime after the 6.5-million-year half-life of 107Pd). The n(107Pd)/n(107Ag) amount ratio can be measured to help determine when the 107Pd decay process began and determine how much time has elapsed since the material was formed.

[344] W. R. Kelly, G. J. Wasserburg. Geophys. Res. Lett.5 1079 (1978).
[345] G. J. Wasserburg, D. A. Papanastassiou. Some Short-Lived Nuclides in the Early Solar-System – A Connection with the Placental ISM, in Essays in Nuclear Astrophysics, C. A. Barnes, D. D. Clayton, and D. N. Schramm. Cambridge University Press, Cambridge, UK (1982).
[346] J. H. Chen, G. J. Wasserburg. Live 107Pd in the Early Solar System and Implications on Planetary Evolution, in Earth Processes: Reading the Isotopic Code, Geophysical Monograph 95, A. Basu and S. Hart. Amer. Geophys. U., Washington (1996).
[347] J. H. Chen, G. J. Wasserburg. Geochim. Cosmochim. Acta54, 1729 (1990).
[348] A. P. Dicken. Radiogenic Isotope Geology, Cambridge University Press, New York (1995).
[353] G. J. Wasserburg. “Short-lived nuclei in the early solar-system”, in Protostars and Planets, D. C. Black, M. S. Matthews (Eds.), Univ. Arizona Press, Tucson, Arizona, USA (1985).

Isotopes in Industry

107Ag is being studied as a possible target for cyclotron production of 103Pd (with a half-life of 17 days) via the 107Ag (p, α n) 103Pd reaction. 103Pd releases X-rays and Auger electrons at the rate of about 80 X-rays and 186 Auger electrons per 100 decays of 103Pd, which makes this isotope an ideal candidate for internal radiotherapy for the treatment of cancers. The production of this isotope in a no-carrier form (not formed in another solution) is important for its medical uses. By using neutrons, photons, and charged particles to force reactions with isotopes of a higher mass number than 103, 103Pd will occur in a fraction of those reactions. The most common methods of 103Pd production use targets of rhodium or other isotopes of palladium. However, 107Ag has also been studied as a feasible option [349], [354]. 109Ag is used to produce the gamma reference source 110mAg to help calibrate gamma detectors [349], [354].

[349] M. Hussain, S. Sudar, M. N. Aslam, H. A. Shah, R. Ahmad, A. A. Malik, S. M. Qaim. Appl. Radiat. Isot.67, 1842 (2009).
[354] F. G. Perey. Phys. Rev. Lett.131, 745 (1963).

Isotope Mass and Abundance

Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
107Ag 106.905 09(2) 0.518 39(8)
109Ag 108.904 756(9) 0.481 61(8)
Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
107Ag 106.9050916(26) 0.51839(8)
109Ag 108.9047553(14) 0.48161(8)

Atomic Mass, Half Life, and Decay

Nuclide Atomic Mass and Uncertainty [u] Half Life and Uncertainty Discovery Year Decay Modes, Intensities and Uncertainties [%]
92Ag 91.959710 ± 0.000429 [Estimated] 1 ms >400ns [Estimated] 2016 β+ ?; p ?
93Ag 92.950188 ± 0.00043 [Estimated] 228 ns ± 16 1994 p=?; β+ ?; β+p ?
94Ag 93.943744 ± 0.000429 [Estimated] 27 ms ± 2 1994 β+=100%; β+p<0.2%
94Agm 93.943744 ± 0.000429 [Estimated] 470 ms ± 10 1994 β+=100%; β+p=17.0±0.6%
94Agn 93.943744 ± 0.000429 [Estimated] 400 ms ± 40 2002 β+=95.4±0.7%; β+p≈27%; p=4.1±0.6%; 2p=0.5±0.3%
95Ag 94.935688 ± 0.000429 [Estimated] 1.78 s ± 0.06 1994 β+=100%; β+p=2.3±0.2%
95Agm 94.935688 ± 0.000429 [Estimated] <500 ms 2003 IT=100%
95Agn 94.935688 ± 0.000429 [Estimated] <16 ms 2003 IT=100%
95Agp 94.935688 ± 0.000429 [Estimated] <40 ms 2003 IT=100%
96Ag 95.930743903 ± 0.000096708 4.45 s ± 0.03 1982 β+=100%; β+p=4.2±0.4%
96Agm 95.930743903 ± 0.000096708 6.9 s ± 0.5 2003 β+=100%; β+p=14.9±1.8%
96Agn 95.930743903 ± 0.000096708 103.2 us ± 4.5 2011 IT=100%
96Agp 95.930743903 ± 0.000096708 1.561 us ± 0.016 2011 IT=100%
96Agq 95.930743903 ± 0.000096708 132 ns ± 17 2011 IT=100%
97Ag 96.923881400 ± 0.0000129 25.5 s ± 0.3 1978 β+=100%
97Agm 96.923881400 ± 0.0000129 100 ms [Estimated] 2019 IT ?
98Ag 97.921559970 ± 0.000035327 47.5 s ± 0.3 1978 β+=100%; β+p=0.0012±0.5%
98Agm 97.921559970 ± 0.000035327 161 ns ± 7 1998 IT=100%
99Ag 98.917645766 ± 0.000006725 2.07 m ± 0.05 1967 β+=100%
99Agm 98.917645766 ± 0.000006725 10.5 s ± 0.5 1978 IT=100%
100Ag 99.916115443 ± 0.000005367 2.01 m ± 0.09 1970 β+=100%
100Agm 99.916115443 ± 0.000005367 2.24 m ± 0.13 1980 β+=?; IT ?
101Ag 100.912683951 ± 0.000005193 11.1 m ± 0.3 1966 β+=100%
101Agm 100.912683951 ± 0.000005193 3.10 s ± 0.10 1975 IT=100%
102Ag 101.911704538 ± 0.000008771 12.9 m ± 0.3 1960 β+=100%
102Agm 101.911704538 ± 0.000008771 7.7 m ± 0.5 1967 β+=51±0.5%; IT=49±0.5%
103Ag 102.908960558 ± 0.0000044 65.7 m ± 0.7 1954 β+=100%
103Agm 102.908960558 ± 0.0000044 5.7 s ± 0.3 1962 IT=100%
104Ag 103.908623715 ± 0.000004527 69.2 m ± 1.0 1955 β+=100%
104Agm 103.908623715 ± 0.000004527 33.5 m ± 2.0 1959 β+≈100%; IT<0.07%
105Ag 104.906525604 ± 0.000004877 41.29 d ± 0.07 1939 β+=100%
105Agm 104.906525604 ± 0.000004877 7.23 m ± 0.16 1969 IT=99.66±0.7%; β+=0.34±0.7%
106Ag 105.906663499 ± 0.000003237 23.96 m ± 0.04 1937 β+≈100%; β- ?
106Agm 105.906663499 ± 0.000003237 8.28 d ± 0.02 1938 β+=100%; IT ?
107Ag 106.905091509 ± 0.000002556 Stable 1924 IS=51.839±0.8%
107Agm 106.905091509 ± 0.000002556 44.3 s ± 0.2 1940 IT=100%
108Ag 107.905950245 ± 0.000002563 2.382 m ± 0.011 1937 β-=97.15±2%; β+=2.85±2%
108Agm 107.905950245 ± 0.000002563 439 y ± 9 1969 β+=91.3±0.9%; IT=8.7±0.9%
109Ag 108.904755778 ± 0.000001381 Stable 1924 IS=48.161±0.8%
109Agm 108.904755778 ± 0.000001381 39.79 s ± 0.21 1967 IT=100%
110Ag 109.906110724 ± 0.00000138 24.56 s ± 0.11 1937 β-≈100%; ε=0.30±0.6%
110Agm 109.906110724 ± 0.00000138 660 ns ± 40 1975 IT=100%
110Agn 109.906110724 ± 0.00000138 249.863 d ± 0.024 1938 β-=98.67±0.8%; IT=1.33±0.8%
111Ag 110.905296827 ± 0.000001565 7.433 d ± 0.010 1937 β-=100%
111Agm 110.905296827 ± 0.000001565 64.8 s ± 0.8 1957 IT=99.3±0.2%; β-=0.7±0.2%
112Ag 111.907048548 ± 0.0000026 3.130 h ± 0.008 1938 β-=100%
113Ag 112.906572865 ± 0.000017866 5.37 h ± 0.05 1949 β-=100%
113Agm 112.906572865 ± 0.000017866 68.7 s ± 1.6 1958 IT=64±0.7%; β-=36±0.7%
114Ag 113.908823029 ± 0.0000049 4.6 s ± 0.1 1958 β-=100%
114Agm 113.908823029 ± 0.0000049 1.50 ms ± 0.05 1990 IT=100%
115Ag 114.908767445 ± 0.000019611 20.0 m ± 0.5 1949 β-=100%
115Agm 114.908767445 ± 0.000019611 18.0 s ± 0.7 1958 β-=79.0±0.3%; IT=21.0±0.3%
116Ag 115.911386809 ± 0.0000035 3.83 m ± 0.08 1958 β-=100%
116Agm 115.911386809 ± 0.0000035 20 s ± 1 2005 β-=93±0.4%; IT=7±0.4%
116Agn 115.911386809 ± 0.0000035 9.3 s ± 0.3 1970 β-=92±0.4%; IT=8±0.4%
117Ag 116.911774086 ± 0.00001457 73.6 s ± 1.4 1958 β-=100%
117Agm 116.911774086 ± 0.00001457 5.34 s ± 0.05 1990 β-=94.0±1.5%; IT=6.0±1.5%
118Ag 117.914595484 ± 0.0000027 3.76 s ± 0.15 1967 β-=100%
118Agm 117.914595484 ± 0.0000027 ~0.1 us 1989 IT=100%
118Agn 117.914595484 ± 0.0000027 2.0 s ± 0.2 1971 β-=59±0.3%; IT=41±0.3%
118Agp 117.914595484 ± 0.0000027 ~0.1 us 1989 IT=100%
119Ag 118.915570309 ± 0.000015783 6.0 s ± 0.5 1975 β-=100%
119Agm 118.915570309 ± 0.000015783 2.1 s ± 0.1 1975 β-=100%
120Ag 119.918784765 ± 0.0000048 1.52 s ± 0.07 1971 β-=100%; β-n<0.003%
120Agm 119.918784765 ± 0.0000048 940 ms ± 100 2012 β-=?; IT ?; β-n ?
120Agn 119.918784765 ± 0.0000048 384 ms ± 22 1971 IT=68±1%; β-=32±1%; β-n ?
121Ag 120.920125279 ± 0.000013 777 ms ± 10 1982 β-=100%; β-n=0.080±1.3%
121Agm 120.920125279 ± 0.000013 200 ms [Estimated] β- ?; IT ?; β-n ?
122Ag 121.923664446 ± 0.000041 529 ms ± 13 1978 β-=100%; β-n=0.186±1%
122Agm 121.923664446 ± 0.000041 550 ms ± 50 2000 β-=100%; IT ?; β-n=?
122Agn 121.923664446 ± 0.000041 200 ms ± 50 2000 β-=100%; IT ?; β-n ?
122Agp 121.923664446 ± 0.000041 6.3 us ± 1.0 2013 IT=100%
123Ag 122.925315060 ± 0.000035 294 ms ± 5 1976 β-=100%; β-n=0.56±0.5%
123Agm 122.925315060 ± 0.000035 100 ms [Estimated] 2019 β-=100%; β-n ?
123Agn 122.925315060 ± 0.000035 202 ns ± 20 2013 IT=100%
123Agp 122.925315060 ± 0.000035 393 ns ± 16 2009 IT=100%
124Ag 123.928899227 ± 0.00027 177.9 ms ± 2.6 1984 β-=100%; β-n=1.3±0.9%
124Agm 123.928899227 ± 0.00027 144 ms ± 20 1995 β-=100%; β-n ?
124Agn 123.928899227 ± 0.00027 140 ns ± 50 2012 IT=100%
124Agp 123.928899227 ± 0.00027 1.48 us ± 0.15 2012 IT=100%
125Ag 124.930735000 ± 0.000465 160 ms ± 5 1994 β-=100%; β-n=11.8±1%
125Agm 124.930735000 ± 0.000465 50 ms [Estimated] 2019 β- ?; IT ?; β-n ?
125Agn 124.930735000 ± 0.000465 491 ns ± 20 2009 IT=100%
126Ag 125.934814 ± 0.000215 [Estimated] 52 ms ± 10 1994 β-=100%; β-n=13.7±1.1%
126Agm 125.934814 ± 0.000215 [Estimated] 108.4 ms ± 2.4 1995 β-=100%; IT ?; β-n ?
126Agn 125.934814 ± 0.000215 [Estimated] 27 us ± 6 2012 IT=100%
127Ag 126.937037 ± 0.000215 [Estimated] 89 ms ± 2 1995 β-=100%; β-n=14.6±1.5%
127Agm 126.937037 ± 0.000215 [Estimated] 20 ms [Estimated] β- ?; IT ?
127Agn 126.937037 ± 0.000215 [Estimated] 67.5 ms ± 0.9 2021 β-=91.2±0.8%; IT=8.8±0.8%
128Ag 127.941266 ± 0.000322 [Estimated] 60 ms ± 3 2000 β-=100%; β-n=20±0.5%; β-2n ?
129Ag 128.944315 ± 0.000429 [Estimated] 49.9 ms ± 3.5 2000 β-=100%; β-n<20%
129Agm 128.944315 ± 0.000429 [Estimated] 10 ms [Estimated] β- ?; β-n ?
130Ag 129.950727 ± 0.000455 [Estimated] 40.6 ms ± 4.5 2000 β-=100%; β-n ?; β-2n ?
131Ag 130.956253 ± 0.000537 [Estimated] 35 ms ± 8 2013 β-=100%; β-n ?; β-2n=10%
132Ag 131.963070 ± 0.000537 [Estimated] 30 ms ± 14 2015 β-=100%; β-n ?; β-2n ?
133Ag 132.968781 ± 0.000537 [Estimated] Not-specified β- ?; β-n ?

Information Sources

  1. 1.  PubChem
  2. 2.  Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
  3. 3.  IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
  4. 4.  Jefferson Lab, U.S. Department of Energy
    LICENSE
    Please see citation and linking information https https://www.jlab.org/privacy-and-security-notice
  5. 5.  Los Alamos National Laboratory, U.S. Department of Energy
  6. 6.  NIST Physical Measurement Laboratory
  7. 7.  IUPAC Periodic Table of the Elements and Isotopes (IPTEI)
    LICENSE
    Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
    https://creativecommons.org/licenses/by-nc-nd/4.0/
  8. 8.  PubChem Elements
    Silver

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