The periodic table of the chemical elements (also periodic table of the elements or just the periodic table) is a tabular display of the chemical elements. Although precursors to this table exist, its invention is generally credited to Russian chemist Dmitri Mendeleev in 1869, who intended the table to illustrate recurring ("periodic") trends in the properties of the elements. The layout of the table has been refined and extended over time, as new elements have been discovered, and new theoretical models have been developed to explain chemical behavior.[1]
The periodic table is now ubiquitous within the academic discipline of chemistry, providing a useful framework to classify, systematize, and compare all of the many different forms of chemical behavior. The table has found many applications in chemistry, physics, biology, and engineering, especially chemical engineering. The current standard table contains 118 elements to date. (elements 1–118).
This common arrangement of the periodic table separates the lanthanoids and actinoids (the f-block) from other elements. The wide periodic table incorporates the f-block. The extended periodic table adds the 8th and 9th periods, incorporating the f-block and adding the theoretical g-block.
Elements of the Periodic Table
Elements Sorted by Name
Name | Symbol | Atomic Number | Atomic Weight | Group | Date Discovered | Discovered By |
Actinium | Ac | 89 | (227) | Actinide series | 1899 | André Debierne |
Aluminum | Al | 13 | 26.9815 | Other metals | 1824 | Hans Oersted (also attributed to Friedrich Wöhler 1827) |
Americium | Am | 95 | 243 | Actinide series | 1944 | Glenn Seaborg, Ralph James, Leon Morgan, and Albert Ghiorso |
Antimony | Sb | 51 | 121.760 | Other metals | prehistoric | unknown |
Argon | Ar | 18 | 39.948 | Noble gases | 1894 | John Rayleigh and William Ramsay |
Arsenic | As | 33 | 74.9216 | Nonmetals | prehistoric | unknown |
Astatine | At | 85 | (210) | Halogens | 1940 | Dale R. Corson, K. R. MacKenzie, and Emilio Segrè |
Barium | Ba | 56 | 137.328 | Alkaline earth metals | 1808 | Humphry Davy |
Berkelium | Bk | 97 | (247) | Actinide series | 1949 | Glenn Seaborg, Stanley Thompson, and Albert Ghiorso |
Beryllium | Be | 4 | 9.0122 | Alkaline earth metals | 1798 | Louis-Nicolas Vauquelin (isolated by Friedrich Wöhler and Antoine-Alexandre-Brutus Bussy 1828) |
Bismuth | Bi | 83 | 208.9804 | Other metals | prehistoric | unknown |
Bohrium | Bh | 107 | (262) | Transition metals | 1976 | Georgii Flerov and Yuri Oganessian (confirmed by German scientist Peter Armbruster and coworkers) |
Boron | B | 5 | 10.81 | Nonmetals | 1808 | Humphry Davy, and independently by Joseph Gay-Lussac and Louis-Jacques Thénard |
Bromine | Br | 35 | 79.904 | Halogens | 1826 | Antoine-Jérôme Balard |
Cadmium | Cd | 48 | 112.412 | Transition metals | 1817 | Friedrich Strohmeyer |
Calcium | Ca | 20 | 40.078 | Alkaline earth metals | 1808 | Humphry Davy |
Californium | Cf | 98 | (251) | Actinide series | 1950 | Glenn Seaborg, Stanley Thompson, Kenneth Street, Jr., and Albert Ghiorso |
Carbon | C | 6 | 12.011 | Nonmetals | prehistoric | unknown |
Cerium | Ce | 58 | 140.115 | Lanthanide series | 1804 | Jöns Berzelius and Wilhelm Hisinger, and independently by Martin Klaproth |
Cesium | Cs | 55 | 132.9054 | Alkali metals | 1860 | Robert Bunsen and Gustav Kirchhoff |
Chlorine | Cl | 17 | 35.4528 | Halogens | 1774 | Karl Scheele |
Chromium | Cr | 24 | 51.9962 | Transition metals | 1797 | Louis-Nicolas Vauquelin |
Cobalt | Co | 27 | 58.9332 | Transition metals | 1730 | Georg Brandt |
Copper | Cu | 29 | 63.546 | Transition metals | prehistoric | unknown |
Curium | Cm | 96 | (247) | Actinide series | 1944 | Glenn Seaborg, Ralph James, and Albert Ghiorso |
Darmstadtium | Ds | 110 | (271) | Transition metals | 1994 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
Dubnium | Db | 105 | (262) | Transition metals | 1970 | claimed by Albert Ghiorso and coworkers (disputed by Soviet workers) |
Dysprosium | Dy | 66 | 162.500 | Lanthanide series | 1886 | Paul Lecoq de Boisbaudran |
Einsteinium | Es | 99 | (252) | Actinide series | 1952 | Albert Ghiorso and coworkers |
Erbium | Er | 68 | 167.26 | Lanthanide series | 1843 | Carl Mosander |
Europium | Eu | 63 | 151.966 | Lanthanide series | 1901 | Eugène Demarçay |
Fermium | Fm | 100 | (257) | Actinide series | 1955 | Albert Ghiorso and coworkers |
Fluorine | F | 9 | 18.9984 | Halogens | 1771 | Karl Scheele (isolated by Henri Moissan 1886) |
Francium | Fr | 87 | (223) | Alkali metals | 1939 | Marguérite Perey |
Gadolinium | Gd | 64 | 157.25 | Lanthanide series | 1886 | Paul Lecoq de Boisbaudran |
Gallium | Ga | 31 | 69.723 | Other metals | 1875 | Paul Lecoq de Boisbaudran |
Germanium | Ge | 32 | 72.61 | Other metals | 1886 | Clemens Winkler |
Gold | Au | 79 | 196.9665 | Transition metals | prehistoric | unknown |
Hafnium | Hf | 72 | 178.49 | Transition metals | 1913 | Dirk Coster and Georg von Hevesy |
Hassium | Hs | 108 | (263) | Transition metals | 1984 | Peter Armbruster and coworkers |
Helium | He | 2 | 4.0026 | Noble gases | 1868 | Pierre Janssen |
Holmium | Ho | 67 | 164.9303 | Lanthanide series | 1879 | Per Cleve |
Hydrogen | H | 1 | 1.0079 | Nonmetals | 1766 | Henry Cavendish |
Indium | In | 49 | 114.818 | Other metals | 1863 | Ferdinand Reich and Hieronymus Richter |
Iodine | I | 53 | 126.9045 | Halogens | 1811 | Bernard Courtois |
Iridium | Ir | 77 | 192.217 | Transition metals | 1804 | Smithson Tennant |
Iron | Fe | 26 | 55.845 | Transition metals | prehistoric | unknown |
Krypton | Kr | 36 | 83.798 | Noble gases | 1898 | William Ramsay and Morris Travers |
Lanthanum | La | 57 | 138.9055 | Lanthanide series | 1839 | Carl Mosander |
Lawrencium | Lr | 103 | (260) | Transition metals | 1961 | Albert Ghiorso, Torbjørn Sikkeland, Almon Larsh, and Robert Latimer |
Lead | Pb | 82 | 207.2 | Other metals | prehistoric | unknown |
Lithium | Li | 3 | 6.941 | Alkali metals | 1817 | Johan Arfwedson |
Lutetium | Lu | 71 | 174.967 | Transition metals | 1907 | Georges Urbain and Carl von Welsbach, independently of each other |
Magnesium | Mg | 12 | 24.3051 | Alkaline earth metals | 1755 | Joseph Black (oxide isolated by Humphry Davy 1808; pure form isolated by Antoine-Alexandre-Brutus Bussy 1828) |
Manganese | Mn | 25 | 54.938 | Transition metals | 1774 | Johann Gottlieb Gahn |
Meitnerium | Mt | 109 | (268) | Transition metals | 1982 | Peter Armbruster and coworkers |
Mendelevium | Md | 101 | (258) | Actinide series | 1955 | Albert Ghiorso, Bernard G. Harvey, Gregory Choppin, Stanley Thompson, and Glenn Seaborg |
Mercury | Hg | 80 | 200.59 | Transition metals | prehistoric | unknown |
Molybdenum | Mo | 42 | 95.94 | Transition metals | 1781 | named by Karl Scheele (isolated by Peter Jacob Hjelm 1782) |
Neodymium | Nd | 60 | 144.24 | Lanthanide series | 1885 | Carl von Welsbach |
Neon | Ne | 10 | 20.1798 | Noble gases | 1898 | William Ramsay and Morris Travers |
Neptunium | Np | 93 | (237) | Actinide series | 1940 | Edwin McMillan and Philip Abelson |
Nickel | Ni | 28 | 58.6934 | Transition metals | 1751 | Axel Cronstedt |
Niobium | Nb | 41 | 92.9064 | Transition metals | 1801 | Charles Hatchett |
Nitrogen | N | 7 | 14.0067 | Nonmetals | 1772 | Daniel Rutherford |
Nobelium | No | 102 | (259) | Actinide series | 1958 | Albert Ghiorso, Torbjørn Sikkeland, J. R. Walton, and Glenn Seaborg |
Osmium | Os | 76 | 190.23 | Transition metals | 1804 | Smithson Tennant |
Oxygen | O | 8 | 15.9994 | Nonmetals | 1774 | Joseph Priestley and Karl Scheele, independently of each other |
Palladium | Pd | 46 | 106.42 | Transition metals | 1804 | William Wollaston |
Phosphorus | P | 15 | 30.9738 | Nonmetals | 1674 | Hennig Brand |
Platinum | Pt | 78 | 195.08 | Transition metals | 1557 | Julius Scaliger |
Plutonium | Pu | 94 | (244) | Actinide series | 1940 | Glenn Seaborg, Edwin McMillan, Joseph Kennedy, and Arthur Wahl |
Polonium | Po | 84 | (209) | Other metals | 1898 | Marie and Pierre Curie |
Potassium | K | 19 | 39.0983 | Alkali metals | 1807 | Humphry Davy |
Praseodymium | Pr | 59 | 140.908 | Lanthanide series | 1885 | Carl von Welsbach |
Promethium | Pm | 61 | (145) | Lanthanide series | 1945 | J. A. Marinsky, Lawrence Glendenin, and Charles Coryell |
Protactinium | Pa | 91 | 231.036 | Actinide series | 1913 | Kasimir Fajans and O. Göhring |
Radium | Ra | 88 | (226) | Alkaline earth metals | 1898 | Marie Curie |
Radon | Rn | 86 | (222) | Noble gases | 1900 | Friedrich Dorn |
Rhenium | Re | 75 | 186.207 | Transition metals | 1925 | Walter Noddack, Ida Tacke, and Otto Berg |
Rhodium | Rh | 45 | 102.9055 | Transition metals | 1804 | William Wollaston |
Rubidium | Rb | 37 | 85.4678 | Alkali metals | 1861 | Robert Bunsen and Gustav Kirchhoff |
Ruthenium | Ru | 44 | 101.07 | Transition metals | 1827 | G. W. Osann (isolated by Karl Klaus 1844) |
Rutherfordium | Rf | 104 | (261) | Transition metals | 1969 | claimed by U.S. scientist Albert Ghiorso and coworkers (disputed by Soviet workers) |
Samarium | Sm | 62 | 150.36 | Lanthanide series | 1879 | Paul Lecoq de Boisbaudran |
Scandium | Sc | 21 | 44.9559 | Transition metals | 1876 | Lars Nilson |
Seaborgium | Sg | 106 | (266) | Transition metals | 1974 | claimed by Georgii Flerov and coworkers, and independently by Albert Ghiorso and coworkers |
Selenium | Se | 34 | 78.96 | Nonmetals | 1817 | Jöns Berzelius |
Silicon | Si | 14 | 28.0855 | Nonmetals | 1823 | Johan Arfwedson |
Silver | Ag | 47 | 107.8682 | Transition metals | prehistoric | unknown |
Sodium | Na | 11 | 22.9898 | Alkali metals | 1807 | Humphry Davy |
Strontium | Sr | 38 | 87.62 | Alkaline earth metals | 1808 | Humphry Davy |
Sulfur | S | 16 | 32.067 | Nonmetals | prehistoric | unknown |
Tantalum | Ta | 73 | 180.948 | Transition metals | 1802 | Anders Ekeberg |
Technetium | Tc | 43 | (98) | Transition metals | 1937 | Carlo Perrier and Emilio Segrè |
Tellurium | Te | 52 | 127.60 | Nonmetals | 1782 | Franz Müller |
Terbium | Tb | 65 | 158.9253 | Lanthanide series | 1843 | Carl Mosander |
Thallium | Tl | 81 | 204.3833 | Other metals | 1861 | William Crookes (isolated by William Crookes and Claude August Lamy, independently of each other, in 1862) |
Thorium | Th | 90 | 232.0381 | Actinide series | 1828 | Jöns Berzelius |
Thulium | Tm | 69 | 168.9342 | Lanthanide series | 1879 | Per Cleve |
Tin | Sn | 50 | 118.711 | Other metals | prehistoric | unknown |
Titanium | Ti | 22 | 47.867 | Transition metals | 1790 | William Gregor |
Tungsten | W | 74 | 183.84 | Transition metals | 1783 | isolated by Juan José Elhuyar and Fausto Elhuyar |
Ununbium | Uub | 112 | (277) | Transition metals | 1996 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
Ununhexium | Uuh | 116 | (292) | Other metals | 2000 | team at the Joint Institute for Nuclear Research, Dubna, Russia |
Ununquadium | Uuq | 114 | (285) | Other metals | 1998 | team at the Joint Institute for Nuclear Research, Dubna, Russia |
Roentgenium | Rg | 111 | (272) | Transition metals | 1994 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
Uranium | U | 92 | 238.0289 | Actinide series | 1789 | Martin Klaproth (isolated by Eugène Péligot 1841) |
Vanadium | V | 23 | 50.9415 | Transition metals | 1801 | Andrés del Rio (disputed), or Nils Sefström 1830 |
Xenon | Xe | 54 | 131.29 | Noble gases | 1898 | William Ramsay and Morris Travers |
Ytterbium | Yb | 70 | 173.04 | Lanthanide series | 1878 | Jean Charles de Marignac |
Yttrium | Y | 39 | 88.906 | Transition metals | 1794 | Johan Gadolin |
Zinc | Zn | 30 | 65.409 | Transition metals | prehistoric | unknown |
Zirconium | Zr | 40 | 91.224 | Transition metals | 1789 | Martin Klaproth |
Elements Sorted by Atomic Number
Atomic Number | Name | Symbol | Atomic Weight | Group | Date Discovered | Discovered By |
1 | Hydrogen | H | 1.0079 | Nonmetals | 1766 | Henry Cavendish |
2 | Helium | He | 4.0026 | Noble gases | 1868 | Pierre Janssen |
3 | Lithium | Li | 6.941 | Alkali metals | 1817 | Johan Arfwedson |
4 | Beryllium | Be | 9.0122 | Alkaline earth metals | 1798 | Louis-Nicolas Vauquelin (isolated by Friedrich Wöhler and Antoine-Alexandre-Brutus Bussy 1828) |
5 | Boron | B | 10.81 | Nonmetals | 1808 | Humphry Davy, and independently by Joseph Gay-Lussac and Louis-Jacques Thénard |
6 | Carbon | C | 12.011 | Nonmetals | prehistoric | unknown |
7 | Nitrogen | N | 14.0067 | Nonmetals | 1772 | Daniel Rutherford |
8 | Oxygen | O | 15.9994 | Nonmetals | 1774 | Joseph Priestley and Karl Scheele, independently of each other |
9 | Fluorine | F | 18.9984 | Halogens | 1771 | Karl Scheele (isolated by Henri Moissan 1886) |
10 | Neon | Ne | 20.1798 | Noble gases | 1898 | William Ramsay and Morris Travers |
11 | Sodium | Na | 22.9898 | Alkali metals | 1807 | Humphry Davy |
12 | Magnesium | Mg | 24.3051 | Alkaline earth metals | 1755 | Joseph Black (oxide isolated by Humphry Davy 1808; pure form isolated by Antoine-Alexandre-Brutus Bussy 1828) |
13 | Aluminum | Al | 26.9815 | Other metals | 1824 | Hans Oersted (also attributed to Friedrich Wöhler 1827) |
14 | Silicon | Si | 28.0855 | Nonmetals | 1823 | Johan Arfwedson |
15 | Phosphorus | P | 30.9738 | Nonmetals | 1674 | Hennig Brand |
16 | Sulfur | S | 32.067 | Nonmetals | prehistoric | unknown |
17 | Chlorine | Cl | 35.4528 | Halogens | 1774 | Karl Scheele |
18 | Argon | Ar | 39.948 | Noble gases | 1894 | John Rayleigh and William Ramsay |
19 | Potassium | K | 39.0983 | Alkali metals | 1807 | Humphry Davy |
20 | Calcium | Ca | 40.078 | Alkaline earth metals | 1808 | Humphry Davy |
21 | Scandium | Sc | 44.9559 | Transition metals | 1876 | Lars Nilson |
22 | Titanium | Ti | 47.867 | Transition metals | 1790 | William Gregor |
23 | Vanadium | V | 50.9415 | Transition metals | 1801 | Andrés del Rio (disputed), or Nils Sefström 1830 |
24 | Chromium | Cr | 51.9962 | Transition metals | 1797 | Louis-Nicolas Vauquelin |
25 | Manganese | Mn | 54.938 | Transition metals | 1774 | Johann Gottlieb Gahn |
26 | Iron | Fe | 55.845 | Transition metals | prehistoric | unknown |
27 | Cobalt | Co | 58.9332 | Transition metals | 1730 | Georg Brandt |
28 | Nickel | Ni | 58.6934 | Transition metals | 1751 | Axel Cronstedt |
29 | Copper | Cu | 63.546 | Transition metals | prehistoric | unknown |
30 | Zinc | Zn | 65.409 | Transition metals | prehistoric | unknown |
31 | Gallium | Ga | 69.723 | Other metals | 1875 | Paul Lecoq de Boisbaudran |
32 | Germanium | Ge | 72.61 | Other metals | 1886 | Clemens Winkler |
33 | Arsenic | As | 74.9216 | Nonmetals | prehistoric | unknown |
34 | Selenium | Se | 78.96 | Nonmetals | 1817 | Jöns Berzelius |
35 | Bromine | Br | 79.904 | Halogens | 1826 | Antoine-Jérôme Balard |
36 | Krypton | Kr | 83.798 | Noble gases | 1898 | William Ramsay and Morris Travers |
37 | Rubidium | Rb | 85.4678 | Alkali metals | 1861 | Robert Bunsen and Gustav Kirchhoff |
38 | Strontium | Sr | 87.62 | Alkaline earth metals | 1808 | Humphry Davy |
39 | Yttrium | Y | 88.906 | Transition metals | 1794 | Johan Gadolin |
40 | Zirconium | Zr | 91.224 | Transition metals | 1789 | Martin Klaproth |
41 | Niobium | Nb | 92.9064 | Transition metals | 1801 | Charles Hatchett |
42 | Molybdenum | Mo | 95.94 | Transition metals | 1781 | named by Karl Scheele (isolated by Peter Jacob Hjelm 1782) |
43 | Technetium | Tc | (98) | Transition metals | 1937 | Carlo Perrier and Emilio Segrè |
44 | Ruthenium | Ru | 101.07 | Transition metals | 1827 | G. W. Osann (isolated by Karl Klaus 1844) |
45 | Rhodium | Rh | 102.9055 | Transition metals | 1804 | William Wollaston |
46 | Palladium | Pd | 106.42 | Transition metals | 1804 | William Wollaston |
47 | Silver | Ag | 107.8682 | Transition metals | prehistoric | unknown |
48 | Cadmium | Cd | 112.412 | Transition metals | 1817 | Friedrich Strohmeyer |
49 | Indium | In | 114.818 | Other metals | 1863 | Ferdinand Reich and Hieronymus Richter |
50 | Tin | Sn | 118.711 | Other metals | prehistoric | unknown |
51 | Antimony | Sb | 121.760 | Other metals | prehistoric | unknown |
52 | Tellurium | Te | 127.60 | Nonmetals | 1782 | Franz Müller |
53 | Iodine | I | 126.9045 | Halogens | 1811 | Bernard Courtois |
54 | Xenon | Xe | 131.29 | Noble gases | 1898 | William Ramsay and Morris Travers |
55 | Cesium | Cs | 132.9054 | Alkali metals | 1860 | Robert Bunsen and Gustav Kirchhoff |
56 | Barium | Ba | 137.328 | Alkaline earth metals | 1808 | Humphry Davy |
57 | Lanthanum | La | 138.9055 | Lanthanide series | 1839 | Carl Mosander |
58 | Cerium | Ce | 140.115 | Lanthanide series | 1804 | Jöns Berzelius and Wilhelm Hisinger, and independently by Martin Klaproth |
59 | Praseodymium | Pr | 140.908 | Lanthanide series | 1885 | Carl von Welsbach |
60 | Neodymium | Nd | 144.24 | Lanthanide series | 1885 | Carl von Welsbach |
61 | Promethium | Pm | (145) | Lanthanide series | 1945 | J. A. Marinsky, Lawrence Glendenin, and Charles Coryell |
62 | Samarium | Sm | 150.36 | Lanthanide series | 1879 | Paul Lecoq de Boisbaudran |
63 | Europium | Eu | 151.966 | Lanthanide series | 1901 | Eugène Demarçay |
64 | Gadolinium | Gd | 157.25 | Lanthanide series | 1886 | Paul Lecoq de Boisbaudran |
65 | Terbium | Tb | 158.9253 | Lanthanide series | 1843 | Carl Mosander |
66 | Dysprosium | Dy | 162.500 | Lanthanide series | 1886 | Paul Lecoq de Boisbaudran |
67 | Holmium | Ho | 164.9303 | Lanthanide series | 1879 | Per Cleve |
68 | Erbium | Er | 167.26 | Lanthanide series | 1843 | Carl Mosander |
69 | Thulium | Tm | 168.9342 | Lanthanide series | 1879 | Per Cleve |
70 | Ytterbium | Yb | 173.04 | Lanthanide series | 1878 | Jean Charles de Marignac |
71 | Lutetium | Lu | 174.967 | Transition metals | 1907 | Georges Urbain and Carl von Welsbach, independently of each other |
72 | Hafnium | Hf | 178.49 | Transition metals | 1913 | Dirk Coster and Georg von Hevesy |
73 | Tantalum | Ta | 180.948 | Transition metals | 1802 | Anders Ekeberg |
74 | Tungsten | W | 183.84 | Transition metals | 1783 | isolated by Juan José Elhuyar and Fausto Elhuyar |
75 | Rhenium | Re | 186.207 | Transition metals | 1925 | Walter Noddack, Ida Tacke, and Otto Berg |
76 | Osmium | Os | 190.23 | Transition metals | 1804 | Smithson Tennant |
77 | Iridium | Ir | 192.217 | Transition metals | 1804 | Smithson Tennant |
78 | Platinum | Pt | 195.08 | Transition metals | 1557 | Julius Scaliger |
79 | Gold | Au | 196.9665 | Transition metals | prehistoric | unknown |
80 | Mercury | Hg | 200.59 | Transition metals | prehistoric | unknown |
81 | Thallium | Tl | 204.3833 | Other metals | 1861 | William Crookes (isolated by William Crookes and Claude August Lamy, independently of each other, in 1862) |
82 | Lead | Pb | 207.2 | Other metals | prehistoric | unknown |
83 | Bismuth | Bi | 208.9804 | Other metals | prehistoric | unknown |
84 | Polonium | Po | (209) | Other metals | 1898 | Marie and Pierre Curie |
85 | Astatine | At | (210) | Halogens | 1940 | Dale R. Corson, K. R. MacKenzie, and Emilio Segrè |
86 | Radon | Rn | (222) | Noble gases | 1900 | Friedrich Dorn |
87 | Francium | Fr | (223) | Alkali metals | 1939 | Marguérite Perey |
88 | Radium | Ra | (226) | Alkaline earth metals | 1898 | Marie Curie |
89 | Actinium | Ac | (227) | Actinide series | 1899 | André Debierne |
90 | Thorium | Th | 232.0381 | Actinide series | 1828 | Jöns Berzelius |
91 | Protactinium | Pa | 231.036 | Actinide series | 1913 | Kasimir Fajans and O. Göhring |
92 | Uranium | U | 238.0289 | Actinide series | 1789 | Martin Klaproth (isolated by Eugène Péligot 1841) |
93 | Neptunium | Np | (237) | Actinide series | 1940 | Edwin McMillan and Philip Abelson |
94 | Plutonium | Pu | (244) | Actinide series | 1940 | Glenn Seaborg, Edwin McMillan, Joseph Kennedy, and Arthur Wahl |
95 | Americium | Am | 243 | Actinide series | 1944 | Glenn Seaborg, Ralph James, Leon Morgan, and Albert Ghiorso |
96 | Curium | Cm | (247) | Actinide series | 1944 | Glenn Seaborg, Ralph James, and Albert Ghiorso |
97 | Berkelium | Bk | (247) | Actinide series | 1949 | Glenn Seaborg, Stanley Thompson, and Albert Ghiorso |
98 | Californium | Cf | (251) | Actinide series | 1950 | Glenn Seaborg, Stanley Thompson, Kenneth Street, Jr., and Albert Ghiorso |
99 | Einsteinium | Es | (252) | Actinide series | 1952 | Albert Ghiorso and coworkers |
100 | Fermium | Fm | (257) | Actinide series | 1955 | Albert Ghiorso and coworkers |
101 | Mendelevium | Md | (258) | Actinide series | 1955 | Albert Ghiorso, Bernard G. Harvey, Gregory Choppin, Stanley Thompson, and Glenn Seaborg |
102 | Nobelium | No | (259) | Actinide series | 1958 | Albert Ghiorso, Torbjørn Sikkeland, J. R. Walton, and Glenn Seaborg |
103 | Lawrencium | Lr | (260) | Transition metals | 1961 | Albert Ghiorso, Torbjørn Sikkeland, Almon Larsh, and Robert Latimer |
104 | Rutherfordium | Rf | (261) | Transition metals | 1969 | claimed by U.S. scientist Albert Ghiorso and coworkers (disputed by Soviet workers) |
105 | Dubnium | Db | (262) | Transition metals | 1970 | claimed by Albert Ghiorso and coworkers (disputed by Soviet workers) |
106 | Seaborgium | Sg | (266) | Transition metals | 1974 | claimed by Georgii Flerov and coworkers, and independently by Albert Ghiorso and coworkers |
107 | Bohrium | Bh | (262) | Transition metals | 1976 | Georgii Flerov and Yuri Oganessian (confirmed by German scientist Peter Armbruster and coworkers) |
108 | Hassium | Hs | (263) | Transition metals | 1984 | Peter Armbruster and coworkers |
109 | Meitnerium | Mt | (268) | Transition metals | 1982 | Peter Armbruster and coworkers |
110 | Darmstadtium | Ds | (271) | Transition metals | 1994 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
111 | Roentgenium | Rg | (272) | Transition metals | 1994 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
112 | Ununbium | Uub | (277) | Transition metals | 1996 | team at the Heavy-Ion Research Laboratory, Darmstadt, Germany |
114 | Ununquadium | Uuq | (285) | Other metals | 1998 | team at the Joint Institute for Nuclear Research, Dubna, Russia |
116 | Ununhexium | Uuh | (292) | Other metals | 2000 | team at the Joint Institute for Nuclear Research, Dubna, Russia |
Alternative versions
Other alternative periodic tables exist.
Some versions of the table show a dark stair-step line along the metalloids. Metals are to the left of the line and non-metals to the right.[2]
The layout of the periodic table demonstrates recurring ("periodic") chemical properties. Elements are listed in order of increasing atomic number (i.e., the number of protons in the atomic nucleus). Rows are arranged so that elements with similar properties fall into the same columns (groups or families). According to quantum mechanical theories of electron configuration within atoms, each row (period) in the table corresponded to the filling of a quantum shell of electrons. There are progressively longer periods further down the table, grouping the elements into s-, p-, d- and f-blocks to reflect their electron configuration.
In printed tables, each element is usually listed with its element symbol and atomic number; many versions of the table also list the element's atomic mass and other information, such as its abbreviated electron configuration, electronegativity and most common valence numbers.
As of 2010, the table contains 118 chemical elements whose discoveries have been confirmed. Ninety-four are found naturally on Earth, and the rest are synthetic elements that have been produced artificially in particle accelerators. Elements 43 (technetium), 61 (promethium) and all elements greater than 83 (bismuth), beginning with 84 (polonium) have no stable isotopes. The atomic mass of each of these element's isotope having the longest half-life is typically reported on periodic tables with parentheses.[3] Isotopes of elements 43, 61, 93 (neptunium) and 94 (plutonium), first discovered synthetically, have since been discovered in trace amounts on Earth as products of natural radioactive decay processes.
The primary determinant of an element's chemical properties is its electron configuration, particularly the valence shell electrons. For instance, any atoms with four valence electrons occupying p orbitals will exhibit some similarity. The type of orbital in which the atom's outermost electrons reside determines the "block" to which it belongs. The number of valence shell electrons determines the family, or group, to which the element belongs.
Subshell | S | G | F | D | P |
Period | |||||
1 | 1s | ||||
2 | 2s | 2p | |||
3 | 3s | 3p | |||
4 | 4s | 3d | 4p | ||
5 | 5s | 4d | 5p | ||
6 | 6s | 4f | 5d | 6p | |
7 | 7s | 5f | 6d | 7p | |
8 | 8s | 5g | 6f | 7d | 8p |
The total number of electron shells an atom has determines the period to which it belongs. Each shell is divided into different subshells, which as atomic number increases are filled in roughly this order (the Aufbau principle) (see table). Hence the structure of the table. Since the outermost electrons determine chemical properties, those with the same number of valence electrons are grouped together.
Progressing through a group from lightest element to heaviest element, the outer-shell electrons (those most readily accessible for participation in chemical reactions) are all in the same type of orbital, with a similar shape, but with increasingly higher energy and average distance from the nucleus. For instance, the outer-shell (or "valence") electrons of the first group, headed by hydrogen, all have one electron in an s orbital. In hydrogen, that s orbital is in the lowest possible energy state of any atom, the first-shell orbital (and represented by hydrogen's position in the first period of the table). In francium, the heaviest element of the group, the outer-shell electron is in the seventh-shell orbital, significantly further out on average from the nucleus than those electrons filling all the shells below it in energy. As another example, both carbon and lead have four electrons in their outer shell orbitals.
Note that as atomic number (i.e., charge on the atomic nucleus) increases, this leads to greater spin-orbit coupling between the nucleus and the electrons, reducing the validity of the quantum mechanical orbital approximation model, which considers each atomic orbital as a separate entity.
The elements ununtrium, ununquadium, ununpentium, etc. are elements that have been discovered, but so far have not received a trivial name yet. There is a system for naming them temporarily.
Classification
Groups
Main article: Group (periodic table)
A group or family is a vertical column in the periodic table. Groups are considered the most important method of classifying the elements. In some groups, the elements have very similar properties and exhibit a clear trend in properties down the group. These groups tend to be given trivial (unsystematic) names, e.g., the alkali metals, alkaline earth metals, halogens, pnictogens, chalcogens, and noble gases. Some other groups in the periodic table display fewer similarities and/or vertical trends (for example Group 14), and these have no trivial names and are referred to simply by their group numbers.
Periods
Main article: Period (periodic table)
A period is a horizontal row in the periodic table. Although groups are the most common way of classifying elements, there are some regions of the periodic table where the horizontal trends and similarities in properties are more significant than vertical group trends. This can be true in the d-block (or "transition metals"), and especially for the f-block, where the lanthanides and actinides form two substantial horizontal series of elements.
Main article: Periodic table block
Because of the importance of the outermost shell, the different regions of the periodic table are sometimes referred to as periodic table blocks, named according to the subshell in which the "last" electron resides. The s-block comprises the first two groups (alkali metals and alkaline earth metals) as well as hydrogen and helium. The p-block comprises the last six groups (groups 13 through 18) and contains, among others, all of the semimetals. The d-block comprises groups 3 through 12 and contains all of the transition metals. The f-block, usually offset below the rest of the periodic table, comprises the rare earth metals.
Other
The chemical elements are also grouped together in other ways. Some of these groupings are often illustrated on the periodic table, such as transition metals, poor metals, and metalloids. Other informal groupings exist, such as the platinum group and the noble metals.
Periodicity of chemical properties
The main value of the periodic table is the ability to predict the chemical properties of an element based on its location on the table. It should be noted that the properties vary differently when moving vertically along the columns of the table than when moving horizontally along the rows.
Source by: Wikipedia
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