Timeline of chemical element discoveries facts for kids
Have you ever wondered how scientists found all the amazing building blocks of our universe? This page tells the story of how the 118 chemical elements we know about today were discovered. We'll explore them in the order they were first identified as pure substances. It's often tricky to pinpoint the exact discovery date for many elements. For each element, you'll find its name, its atomic number (which is like its unique ID), the year it was first reported, who discovered it, and interesting facts about its journey to discovery.
Contents
Exploring the Periodic Table by Discovery Time
This table shows the Periodic table with each element colored based on when it was discovered. It helps us see how our understanding of elements grew over time!
| Periodic table by era of discovery | ||||||||||||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | |||||||||||||||||||||||
| Group → | ||||||||||||||||||||||||||||||||||||||||
| ↓ Period | ||||||||||||||||||||||||||||||||||||||||
| 1 | 1 H |
2 He |
||||||||||||||||||||||||||||||||||||||
| 2 | 3 Li |
4 Be |
5 B |
6 C |
7 N |
8 O |
9 F |
10 Ne |
||||||||||||||||||||||||||||||||
| 3 | 11 Na |
12 Mg |
13 Al |
14 Si |
15 P |
16 S |
17 Cl |
18 Ar |
||||||||||||||||||||||||||||||||
| 4 | 19 K |
20 Ca |
21 Sc |
22 Ti |
23 V |
24 Cr |
25 Mn |
26 Fe |
27 Co |
28 Ni |
29 Cu |
30 Zn |
31 Ga |
32 Ge |
33 As |
34 Se |
35 Br |
36 Kr |
||||||||||||||||||||||
| 5 | 37 Rb |
38 Sr |
39 Y |
40 Zr |
41 Nb |
42 Mo |
43 Tc |
44 Ru |
45 Rh |
46 Pd |
47 Ag |
48 Cd |
49 In |
50 Sn |
51 Sb |
52 Te |
53 I |
54 Xe |
||||||||||||||||||||||
| 6 | 55 Cs |
56 Ba |
71 Lu |
72 Hf |
73 Ta |
74 W |
75 Re |
76 Os |
77 Ir |
78 Pt |
79 Au |
80 Hg |
81 Tl |
82 Pb |
83 Bi |
84 Po |
85 At |
86 Rn |
||||||||||||||||||||||
| 7 | 87 Fr |
88 Ra |
103 Lr |
104 Rf |
105 Db |
106 Sg |
107 Bh |
108 Hs |
109 Mt |
110 Ds |
111 Rg |
112 Cn |
113 Nh |
114 Fl |
115 Mc |
116 Lv |
117 Ts |
118 Og |
||||||||||||||||||||||
| 57 La |
58 Ce |
59 Pr |
60 Nd |
61 Pm |
62 Sm |
63 Eu |
64 Gd |
65 Tb |
66 Dy |
67 Ho |
68 Er |
69 Tm |
70 Yb |
|||||||||||||||||||||||||||
| 89 Ac |
90 Th |
91 Pa |
92 U |
93 Np |
94 Pu |
95 Am |
96 Cm |
97 Bk |
98 Cf |
99 Es |
100 Fm |
101 Md |
102 No |
|||||||||||||||||||||||||||
|
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A Visual Journey Through Element Discoveries
This timeline shows when different elements were discovered, from the 1600s all the way to 2026!

How Element Discoveries Grew Over Time
Ancient Discoveries: Elements Known for Ages
Some elements have been known and used by humans since ancient times, long before scientists understood what elements truly were!
| Z | Element | Earliest use | Oldest existing sample |
Discoverer(s) | Place of oldest sample |
Notes |
|---|---|---|---|---|---|---|
| 79 | Gold | 40000 BC | 4600 BC – 4200 BC | Earliest humans | Varna Necropolis | Humans have known about gold for a very long time! Small pieces of natural gold were found in Spanish caves from around 40,000 BC. The oldest gold jewelry, from about 4600–4200 BC, was found in Bulgaria. Scientists officially recognized it as an element in 1787. |
| 6 | Carbon | 26000 BC | 26000 BC | Earliest humans | Carbon, found in charcoal and soot, was known to early humans. The oldest charcoal paintings are about 28,000 years old! Ancient Egyptians and Sumerians used charcoal to make bronze. Diamonds, another form of carbon, were known by 2500 BC. In 1772, Antoine Lavoisier showed that diamonds, graphite, and charcoal are all made of the same basic substance. It was officially listed as an element in 1787. | |
| 29 | Copper | 9000 BC | 6000 BC | Middle East | Asia Minor | Copper was first found as a natural metal and later extracted from rocks. People in the Middle East likely discovered it around 9000 BC. It was very important during the Stone Age and Bronze Age. Copper beads from 6000 BC were found in Turkey. The oldest evidence of melting copper from rocks dates back to 5000 BC in Serbia. Scientists recognized copper as an element in 1787. |
| 82 | Lead | 7000 BC | 3800 BC | Asia Minor | Abydos, Egypt | People started melting lead from rocks about 9,000 years ago. The oldest lead object, a small statue, was found in Egypt and dates to around 3800 BC. Lead was officially recognized as an element in 1787. |
| 47 | Silver | Before 5000 BC | ca. 4000 BC | Asia Minor | Asia Minor | Silver was likely discovered in Asia Minor soon after copper and gold. It was officially recognized as an element in 1787. |
| 26 | Iron | Before 5000 BC | 4000 BC | Middle East | Egypt | Iron has been known since before 5000 BC. The oldest iron items are beads made from meteoric iron (from space!) in Egypt around 4000 BC. Learning to melt iron from rocks around 3000 BC led to the Iron Age (around 1200 BC), when iron was used for tools and weapons. It was recognized as an element in 1787. |
| 50 | Tin | 3500 BC | 2000 BC | Asia Minor | Kestel | Tin was first melted with copper around 3500 BC to create bronze, starting the Bronze Age. An ancient tin mine in Turkey was used from 3250 to 1800 BC. The oldest tin objects are from about 2000 BC. Tin was officially recognized as an element in 1787. |
| 51 | Antimony | 3000 BC | 3000 BC | Sumerians | Middle East | A very pure antimony artifact, possibly part of a vase, was found in Iraq and dates to about 3000 BC. Ancient writers described accidentally making metallic antimony. The Muslim alchemist Jabir ibn Hayyan (around 850–950 AD) described how to intentionally separate it. In Europe, it was used by 1540. Lavoisier likely recognized it as an element in 1787. |
| 16 | Sulfur | Before 2000 BC | Middle East | Middle East | Sulfur was first used over 4,000 years ago. Ancient Egyptians used sulfur ointment for eye problems. Alchemists in the 8th and 9th centuries thought it was a basic building block of metals. Paracelsus in the 16th century also called it a universal element. Antoine Lavoisier recognized sulfur as a true element in 1777, a discovery confirmed by other scientists later. | |
| 80 | Mercury | 1500 BC | 1500 BC | Egyptians | Egypt | The mineral cinnabar, which contains mercury, was used as a colorful paint since 9000 BC. Small amounts of mercury metal were found in Turkish mines from 8000 years ago. Mercury was also found in Egyptian tombs from 1500 BC. Medieval alchemists and later scientists in 1787 recognized it as an element. |
| 30 | Zinc | Before 1000 BC | 1000 BC | Indian metallurgists | Indian subcontinent | Zinc was used in brass by Indian metalworkers before 1000 BC, though they didn't fully understand it. A 4th-century BC vase from India shows that metallic zinc was known then. Zinc was melted in China and India around 1300 AD. The alchemist Paracelsus named it in 1526. It was fully isolated and described by Andreas Sigismund Marggraf in 1746. |
| 78 | Platinum | c. 600 BC – AD 200 | c. 600 BC – AD 200 | Pre-Columbian South Americans | South America | Ancient South Americans used platinum to make white gold alloys. An Egyptian pharaoh's box from around 650 BC had gold-platinum decorations. Europeans first described this metal in 1557. Antonio de Ulloa observed it in Peru in 1735. William Brownrigg first referred to it as a new metal in 1750. |
| 33 | Arsenic | c. AD 300 | c. AD 300 | Egyptians | Middle East | The Egyptian alchemist Zosimos described using metallic arsenic. The Muslim alchemist Jabir ibn Hayyan (around 850–950 AD) later described how to purify it. In Europe, Johann Schröder prepared metallic arsenic in 1641. It was recognized as an element in 1787. |
| 83 | Bismuth | c. 1500 | c. 1500 | European alchemists and Inca civilisation | Europe and South America | Bismuth was known in ancient times but often confused with tin and lead. The Incas used bismuth in a special bronze alloy for knives. Agricola in the 1500s said bismuth was a distinct metal. In 1753, Claude François Geoffroy proved it was different from lead and tin. |
Modern Discoveries: New Elements Found by Scientists
In more recent times, scientists used new methods to discover and isolate elements. Sometimes, elements were known in compounds for a long time before their pure form was found!
| Z | Element | Observed | Isolated (widely known) | Notes | ||
|---|---|---|---|---|---|---|
| Year | By | Year | By | |||
| 15 | Phosphorus | 1669 | H. Brand | 1669 | H. Brand | Hennig Brand prepared and isolated phosphorus from urine. It was the first element whose discovery date and discoverer are clearly recorded. Antoine Lavoisier later recognized it as an element. |
| 1 | Hydrogen | 1671 | R. Boyle | 1671 | R. Boyle | Robert Boyle made hydrogen by mixing iron filings with acid. Henry Cavendish in 1766 was the first to realize it was a unique gas. Lavoisier named it in 1783. |
| 11 | Sodium | 1702 | G. E. Stahl | 1807 | H. Davy | Georg Ernst Stahl suggested that sodium and potassium salts were different in 1702. Humphry Davy isolated both sodium and potassium metals in 1807 using electricity. |
| 19 | Potassium | 1702 | G. E. Stahl | 1807 | H. Davy | |
| 27 | Cobalt | 1735 | G. Brandt | 1735 | G. Brandt | Georg Brandt proved that the blue color in glass came from a new metal, not bismuth as people thought. |
| 20 | Calcium | 1739 | J. H. Pott | 1808 | H. Davy | Lime was known for centuries, but its chemical nature was understood in the 18th century. Scientists suggested it was an element's oxide in 1787. Humphry Davy isolated the metal using electricity in 1808. |
| 14 | Silicon | 1739 | J. H. Pott | 1823 | J. Berzelius | Silicon compounds like rock crystals were known to ancient people. In 1739, Johann Heinrich Pott recognized silica as a unique "earth." Lavoisier thought the element must exist. Jöns Jakob Berzelius obtained the pure element in 1823. |
| 13 | Aluminium | 1746 | J. H. Pott | 1825 | H.C.Ørsted | Paracelsus recognized "alumina" as different from other substances in 1570. Lavoisier predicted in 1787 that alumina was the oxide of an undiscovered element. Hans Christian Ørsted was the first to isolate metallic aluminium in 1825. |
| 28 | Nickel | 1751 | F. Cronstedt | 1751 | F. Cronstedt | Axel Fredrik Cronstedt found nickel while trying to get copper from a mineral called "fake copper." |
| 12 | Magnesium | 1755 | J. Black | 1808 | H. Davy | Joseph Black noticed that "magnesia alba" (MgO) was different from lime (CaO) in 1755. Humphry Davy isolated the metal using electricity in 1808. |
| 25 | Manganese | 1770 | T. O. Bergman | 1774 | J. G. Gahn | Torbern Olof Bergman identified a new metal in a mineral but couldn't get it out. Johan Gottlieb Gahn isolated it in 1774 by heating its oxide with carbon. |
| 9 | Fluorine | 1771 | W. Scheele | 1886 | H. Moissan | Carl Wilhelm Scheele studied fluorspar and realized it was a salt of a new acid. Lavoisier listed a "fluorine radical" in 1789. Many tried to isolate it, and Henri Moissan finally succeeded in 1886. |
| 8 | Oxygen | 1771 | W. Scheele | 1771 | W. Scheele | Carl Wilhelm Scheele made oxygen in 1771 by heating certain compounds, but published later. Joseph Priestley also made it in 1774. Antoine Lavoisier was the first to recognize it as a true element and named it in 1777. |
| 7 | Nitrogen | 1772 | D. Rutherford | 1772 | D. Rutherford | Daniel Rutherford discovered nitrogen while studying air. He showed that air, even after removing carbon dioxide, couldn't support burning. Lavoisier named it in 1775–76. |
| 56 | Barium | 1772 | W. Scheele | 1808 | H. Davy | Carl Wilhelm Scheele found a new "earth" (barium oxide) in a mineral in 1772. Humphry Davy isolated the metal using electricity in 1808. |
| 17 | Chlorine | 1774 | W. Scheele | 1774 | W. Scheele | Carl Wilhelm Scheele obtained chlorine from hydrochloric acid but thought it was an oxide. In 1810, Humphry Davy correctly identified it as an element. |
| 42 | Molybdenum | 1778 | W. Scheele | 1788 | J. Hjelm | Carl Wilhelm Scheele recognized molybdenum as a metal in a mineral. Peter Jacob Hjelm isolated it in 1788. |
| 74 | Tungsten | 1781 | W. Scheele | 1783 | J. and F. Elhuyar | Carl Wilhelm Scheele showed that a mineral contained a new acid. The Elhuyar brothers then isolated the element in 1783. It is known as both tungsten and wolfram. |
| 52 | Tellurium | 1782 | F.-J.M. von Reichenstein | 1798 | H. Klaproth | Franz-Joseph Müller von Reichenstein observed tellurium as an impurity in gold ores. Martin Heinrich Klaproth isolated it in 1798. |
| 5 | Boron | 1787 | L. Guyton de Morveau, A. Lavoisier, C. L. Berthollet, and A. de Fourcroy | 1809 | H. Davy | Borax was known for a long time. In 1787, scientists listed a "boron radical." Humphry Davy announced the isolation of boron in 1809. |
| 1789 | A. Lavoisier | Antoine Lavoisier created the first modern list of chemical elements. He also redefined what an "element" truly means. | ||||
| 40 | Zirconium | 1789 | H. Klaproth | 1824 | J. Berzelius | Martin Heinrich Klaproth identified a new oxide in zircon in 1789. Jöns Jakob Berzelius isolated the element in 1824. |
| 92 | Uranium | 1789 | H. Klaproth | 1841 | E.-M. Péligot | Martin Heinrich Klaproth mistakenly identified a uranium oxide as the element itself in 1789 and named it after the planet Uranus. Eugène-Melchior Péligot isolated the pure metal in 1841. |
| 38 | Strontium | 1790 | A. Crawford | 1808 | H. Davy | Adair Crawford found that a mineral called strontianite contained a new "earth" in 1790. Humphry Davy isolated strontium using electricity in 1808. |
| 22 | Titanium | 1791 | W. Gregor | 1875 | D. K. Kirillov | William Gregor found an oxide of a new metal in a mineral in 1791. Martin Heinrich Klaproth independently discovered it in 1795 and named it. Pure metallic titanium was obtained in 1910. |
| 39 | Yttrium | 1794 | J. Gadolin | 1843 | H. Rose | Johan Gadolin discovered a new "earth" in a mineral in 1794. Heinrich Rose correctly isolated the element in 1843. |
| 24 | Chromium | 1797 | N. Vauquelin | 1798 | N. Vauquelin | Louis Nicolas Vauquelin analyzed a mineral in 1797 and then isolated the metal in 1798 by heating its oxide with charcoal. |
| 4 | Beryllium | 1798 | N. Vauquelin | 1828 | F. Wöhler and A. Bussy | Louis Nicolas Vauquelin discovered beryllium oxide in beryl and emerald in 1798. Friedrich Wöhler and Antoine Bussy independently isolated the metal in 1828. |
| 23 | Vanadium | 1801 | A. M. del Río | 1867 | H. E. Roscoe | Andrés Manuel del Río found this metal in 1801, but his claim was initially dismissed. Nils Gabriel Sefström rediscovered it in 1830 and named it vanadium. Henry Enfield Roscoe produced the pure metal in 1867. |
| 41 | Niobium | 1801 | C. Hatchett | 1864 | W. Blomstrand | Charles Hatchett found this element in an ore and named it "columbium." Later, Heinrich Rose proved it was distinct from tantalum and renamed it niobium. Niobium was officially accepted in 1949. |
| 73 | Tantalum | 1802 | G. Ekeberg | 1864 | J.C.G. de Marignac | Anders Gustaf Ekeberg found this element in minerals and named it after Tantalus because it was hard to dissolve. Jean Charles Galissard de Marignac produced relatively pure tantalum in 1864. |
| 46 | Palladium | 1802 | W. H. Wollaston | 1802 | W. H. Wollaston | William Hyde Wollaston discovered palladium in platinum samples from South America. He named it after the newly discovered asteroid Pallas. |
| 58 | Cerium | 1803 | H. Klaproth, W. Hisinger, and J. Berzelius | 1875 | W. F. Hillebrand and T. H. Norton | Wilhelm Hisinger and Jöns Jakob Berzelius discovered a new "earth" in a mineral and named the element after the asteroid Ceres. Martin Heinrich Klaproth also discovered it. Pure cerium was isolated in 1875. |
| 76 | Osmium | 1803 | S. Tennant | 1803 | S. Tennant | Smithson Tennant discovered two new elements, osmium and iridium, in platinum samples. He published his findings in 1804. |
| 77 | Iridium | 1803 | S. Tennant and H.-V. Collet-Descotils | 1803 | S. Tennant | |
| 45 | Rhodium | 1804 | H. Wollaston | 1804 | H. Wollaston | William Hyde Wollaston discovered and isolated rhodium from crude platinum samples. |
| 53 | Iodine | 1811 | B. Courtois | 1811 | B. Courtois | Bernard Courtois discovered iodine in the ashes of seaweed. Joseph Louis Gay-Lussac named it "iode" in French, and Humphry Davy gave it the English name "iodine." |
| 3 | Lithium | 1817 | A. Arfwedson | 1821 | W. T. Brande | Johan August Arfwedson discovered this alkali metal in a mineral. William Thomas Brande isolated it using electricity in 1821. |
| 48 | Cadmium | 1817 | S. L Hermann, F. Stromeyer, and J.C.H. Roloff | 1817 | S. L Hermann, F. Stromeyer, and J.C.H. Roloff | These three scientists found an unknown metal in a zinc oxide sample. The name given by Friedrich Stromeyer became the accepted one. |
| 34 | Selenium | 1817 | J. Berzelius and G. Gahn | 1817 | J. Berzelius and G. Gahn | While working with lead, Jöns Jakob Berzelius and Johann Gottlieb Gahn discovered a substance they first thought was tellurium, but later realized it was a new element. |
| 35 | Bromine | 1825 | J. Balard and C. Löwig | 1825 | J. Balard and C. Löwig | Both Antoine Jérôme Balard and Carl Jacob Löwig discovered bromine in the autumn of 1825. Balard published his findings first. |
| 90 | Thorium | 1829 | J. Berzelius | 1914 | D. Lely, Jr. and L. Hamburger | Jöns Jakob Berzelius obtained a new "earth" (the oxide of a new element) from a mineral in 1829. |
| 57 | Lanthanum | 1838 | G. Mosander | 1904 | W. Muthmann, L. Weiss | Carl Gustaf Mosander found a new "earth" in ceria samples in 1838. |
| 60 | Neodymium | 1841 | G. Mosander | 1901 | W. Muthmann, H. Hofer, L. Weiss | Carl Gustaf Mosander discovered this element and called it didymium. Later, Carl Auer von Welsbach split didymium into two elements: praseodymium and neodymium. |
| 68 | Erbium | 1843 | G. Mosander | 1934 | W. Klemm and H. Bommer | Carl Gustaf Mosander separated "yttria" into yttria, erbia, and terbia. The names were later swapped due to further research, with erbia becoming the rose-colored earth and terbia the yellow earth. |
| 65 | Terbium | 1843 | G. Mosander | 1937 | W. Klemm and H. Bommer | |
| 44 | Ruthenium | 1844 | K. Claus | 1844 | K. Claus | Gottfried Wilhelm Osann thought he found new metals in Russian platinum in 1826, including ruthenium. In 1844, Karl Ernst Claus confirmed one new metal and reused Osann's name "ruthenium." |
| 55 | Caesium | 1860 | G. R. Kirchhoff and R. Bunsen | 1882 | C. Setterberg | Gustav Kirchhoff and Robert Bunsen discovered caesium using spectrum analysis, noticing its two blue light lines. The pure metal was isolated in 1882 by Carl Setterberg. |
| 37 | Rubidium | 1861 | G. R. Kirchhoff and R. Bunsen | 1863 | R. Bunsen | Gustav Kirchhoff and Robert Bunsen discovered rubidium shortly after caesium, by observing new spectral lines in a mineral. Robert Bunsen isolated the metal around 1863. |
| 81 | Thallium | 1861 | W. Crookes | 1862 | C.-A. Lamy | William Crookes found a new green line in a selenium sample. Later that year, Claude-Auguste Lamy found the element to be metallic. |
| 49 | Indium | 1863 | F. Reich and T. Richter | 1864 | T. Richter | Ferdinand Reich and Hieronymous Theodor Richter identified indium by its bright indigo-blue light emission. Richter isolated the metal the next year. |
| 2 | Helium | 1868 | N. Lockyer | 1895 | W. Ramsay, T. Cleve, and N. Langlet | Pierre Janssen and Joseph Norman Lockyer independently observed a yellow line in the Sun's spectrum that didn't match any known element. Lockyer correctly concluded it was a new element. Years later, it was found on Earth by Sir William Ramsay, Per Theodor Cleve, and Nils Langlet. |
| 1869 | D. I. Mendeleev | Dmitri Mendeleev organized the 63 known elements into the first modern periodic table. He also correctly predicted several new elements. | ||||
| 31 | Gallium | 1875 | P. E. L. de Boisbaudran | 1878 | P. E. L. de Boisbaudran and E. Jungfleisch | Paul Emile Lecoq de Boisbaudran observed light lines matching an element predicted by Mendeleev. He and Emil Jungfleisch isolated the metal three years later. |
| 70 | Ytterbium | 1878 | J.C.G. de Marignac | 1936 | W. Klemm and H. Bommer | In 1878, Jean Charles Galissard de Marignac reported splitting "erbia" into two new "earths," one of which was ytterbia. |
| 67 | Holmium | 1878 | J.-L. Soret and M. Delafontaine | 1939 | H. Bommer | Jacques-Louis Soret found holmium in a mineral. Later, Per Teodor Cleve separated Marignac's erbia into erbia, thulium, and holmium. |
| 21 | Scandium | 1879 | F. Nilson | 1937 | W. Fischer, K. Brünger, H. Grieneisen | Lars Fredrik Nilson split ytterbia into pure ytterbia and a new element that matched Mendeleev's predicted "eka-boron." |
| 69 | Thulium | 1879 | T. Cleve | 1936 | W. Klemm and H. Bommer | Per Teodor Cleve separated Marignac's erbia into erbia, thulium, and holmium. |
| 62 | Samarium | 1879 | P.E.L. de Boisbaudran | 1903 | W. Muthmann | Paul Emile Lecoq de Boisbaudran noted a new "earth" in a mineral and named it samaria. |
| 64 | Gadolinium | 1880 | J. C. G. de Marignac | 1935 | Félix Trombe | Jean Charles Galissard de Marignac first observed this new "earth." Later, Paul Emile Lecoq de Boisbaudran obtained a pure sample. |
| 59 | Praseodymium | 1885 | C. A. von Welsbach | 1904 | W. Muthmann, L. Weiss | Carl Auer von Welsbach discovered praseodymium in Mosander's didymia. |
| 32 | Germanium | 1886 | C. A. Winkler | 1886 | C. A. Winkler | In 1886, Clemens Winkler found germanium, which matched Mendeleev's predicted "eka-silicon." |
| 66 | Dysprosium | 1886 | P.E.L. de Boisbaudran | 1937 | W. Klemm and H. Bommer | Paul Emile Lecoq de Boisbaudran found a new "earth" in erbia. |
| 18 | Argon | 1894 | Lord Rayleigh and W. Ramsay | 1894 | Lord Rayleigh and W. Ramsay | Lord Rayleigh and William Ramsay discovered argon by comparing the weights of nitrogen from air and nitrogen made chemically. It was the first noble gas found. |
| 63 | Europium | 1896 | E.-A. Demarçay | 1937 | W. Klemm and H. Bommer | Eugène-Anatole Demarçay found spectral lines of a new element in samarium and named it europium in 1901. Metallic europium was isolated in 1937. |
| 36 | Krypton | 1898 | W. Ramsay and W. Travers | 1898 | W. Ramsay and W. Travers | In 1898, William Ramsay and Morris W. Travers separated krypton, a noble gas, from liquid argon. |
| 10 | Neon | 1898 | W. Ramsay and W. Travers | 1898 | W. Ramsay and W. Travers | In June 1898, William Ramsay and Morris W. Travers separated neon, another noble gas, from liquid argon. |
| 54 | Xenon | 1898 | W. Ramsay and W. Travers | 1898 | W. Ramsay and W. Travers | After neon, William Ramsay and Morris W. Travers separated a third noble gas, xenon, from liquid argon. |
| 84 | Polonium | 1898 | P. and M. Curie | 1946 | W. H. Beamer and C. R. Maxwell | In 1898, Pierre Curie and Marie Curie noticed increased radioactivity in uranium from pitchblende, which they linked to an unknown element. They named it polonium. Pure polonium was obtained in 1946. |
| 88 | Radium | 1898 | P. and M. Curie | 1910 | Marie Curie and André-Louis Debierne | The Curies reported a new element, radium, in December 1898. Marie Curie later isolated it from uraninite. In 1910, she and André-Louis Debierne isolated pure radium metal. |
| 86 | Radon | 1899 | E. Rutherford and R. B. Owens | 1910 | W. Ramsay and R. Whytlaw-Gray | Ernest Rutherford and Robert B. Owens discovered a radioactive gas from thorium decay. It was later isolated by William Ramsay and Robert Whytlaw-Gray. |
| 89 | Actinium | 1902 | F. O. Giesel | 1955 | Joseph G. Stites, Murrell L. Salutsky, Bob D. Stone | Friedrich Oskar Giesel obtained a substance from pitchblende similar to lanthanum. André-Louis Debierne had previously reported a new element, actinium. Both had samples containing element 89, and Debierne is generally credited. |
| 71 | Lutetium | 1906 | C. A. von Welsbach and G. Urbain | 1937 | W. Klemm and H. Bommer | Carl Auer von Welsbach and Georges Urbain independently proved that ytterbium contained a new element. Urbain named it lutetium, which was adopted by the International Committee of Atomic Weights. |
| 75 | Rhenium | 1908 | M. Ogawa | 1908 | M. Ogawa | Masataka Ogawa found rhenium in a mineral in 1908, but mistakenly identified it. In 1925, Walter Noddack, Ida Tacke, and Otto Berg correctly identified it as element 75 and named it rhenium. |
| 91 | Protactinium | 1913 | K. Fajans and O. H. Göhring | 1934 | A. von Grosse | Kasimir Fajans and Oswald Helmuth Göhring obtained the first isotope of this element in 1913. A longer-lived isotope was found in 1918 by Otto Hahn and Lise Meitner, who named it protactinium. |
| 72 | Hafnium | 1922 | D. Coster and G. von Hevesy | 1924 | Anton Eduard van Arkel and Jan Hendrik de Boer | Dirk Coster and Georg von Hevesy found hafnium using X-ray analysis in zircon. Anton Eduard van Arkel and Jan Hendrik de Boer first prepared metallic hafnium in 1924. It was the last stable element discovered. |
| 43 | Technetium | 1937 | C. Perrier and E. Segrè | 1947 | S. Fried | Carlo Perrier and Emilio Segrè discovered technetium in a molybdenum sample used in a cyclotron. It was the first element discovered by making it in a lab. Small traces were later found on Earth in 1962. |
| 87 | Francium | 1939 | M. Perey | Marguerite Perey discovered francium as a decay product of actinium. It was the last element found in nature, rather than created in a lab. | ||
| 93 | Neptunium | 1940 | E.M. McMillan and H. Abelson | 1945 | S. Fried | Edwin McMillan and Philip H. Abelson created neptunium by shining neutrons on uranium. It was the first element heavier than uranium to be discovered. Natural traces were found in pitchblende in 1952. |
| 85 | Astatine | 1940 | D. R. Corson, K. R. MacKenzie and E. Segrè | Dale R. Corson, Kenneth Ross MacKenzie, and Emilio Segrè made astatine by hitting bismuth with alpha particles. In 1943, Berta Karlik and Traude Bernert found it in nature. | ||
| 94 | Plutonium | 1941 | Glenn T. Seaborg, Arthur C. Wahl, W. Kennedy and E.M. McMillan | 1943 | H. L. Baumbach, S. Fried, P. L. Kirk and, R. S. Rosenfels | Plutonium was made by bombarding uranium with deuterons. Glenn T. Seaborg and Morris L. Perlman later found traces of it in natural pitchblende. The first sample of plutonium metal was created in 1943. |
| 96 | Curium | 1944 | Glenn T. Seaborg, Ralph A. James and Albert Ghiorso | 1950 | J. C. Wallmann, W. W. T. Crane and B. B. Cunningham | Curium was created by bombarding plutonium with alpha particles during the Manhattan Project. Curium metal was produced in 1950. |
| 95 | Americium | 1944 | G. T. Seaborg, R. A. James, O. Morgan and A. Ghiorso | 1951 | Edgar F. Westrum Jr. and LeRoy Eyring | Americium was created by shining neutrons on plutonium during the Manhattan Project. Americium metal was produced in 1951. |
| 61 | Promethium | 1945 | Jacob A. Marinsky, Lawrence E. Glendenin, and Charles D. Coryell | 1963 | F. Weigel | Promethium was isolated during the Manhattan Project in 1945. The metal was later isolated in 1963. It is the most recent element to have been found in trace amounts on Earth. |
| 97 | Berkelium | 1949 | G. Thompson, A. Ghiorso and G. T. Seaborg (University of California, Berkeley) | 1969 | J. R. Peterson, J. A. Fahey, and R. D. Baybarz | Berkelium was created by bombarding americium with alpha particles. |
| 98 | Californium | 1950 | S. G. Thompson, K. Street, Jr., A. Ghiorso and G. T. Seaborg (University of California, Berkeley) | 1974 | R. G. Haire and R. D. Baybarz | Californium was made by bombarding curium with alpha particles. Californium metal was produced in 1974. |
| 99 | Einsteinium | 1952 | A. Ghiorso et al. (Argonne Laboratory, Los Alamos Laboratory and University of California, Berkeley) | 1979 | R. G. Haire and R. D. Baybarz | Einsteinium was formed in the first thermonuclear explosion in November 1952. It was kept secret for several years. Einsteinium metal was produced in 1979. |
| 100 | Fermium | 1953 | A. Ghiorso et al. (Argonne Laboratory, Los Alamos Laboratory and University of California, Berkeley) | Fermium was also formed in the first thermonuclear explosion in November 1952. It was identified in early 1953 but kept secret for some years. | ||
| 101 | Mendelevium | 1955 | A. Ghiorso, G. Harvey, G. R. Choppin, S. G. Thompson and G. T. Seaborg (Berkeley Radiation Laboratory) | Mendelevium was created by bombarding einsteinium with alpha particles. | ||
| 103 | Lawrencium | 1961 | A. Ghiorso, T. Sikkeland, E. Larsh and M. Latimer (Berkeley Radiation Laboratory) | Lawrencium was first made by bombarding californium with boron atoms. | ||
| 102 | Nobelium | 1965 | E. D. Donets, V. A. Shchegolev and V. A. Ermakov (JINR in Dubna) | Nobelium was first made by bombarding uranium with neon atoms. The first clear report of its detection came in 1966. | ||
| 104 | Rutherfordium | 1969 | A. Ghiorso et al. (Berkeley Radiation Laboratory) and I. Zvara et al. (JINR in Dubna) | Rutherfordium was created by bombarding californium with carbon atoms by Albert Ghiorso's team, and by bombarding plutonium with neon atoms by I. Zvara's team. | ||
| 105 | Dubnium | 1970 | A. Ghiorso et al. (Berkeley Radiation Laboratory) and V. A. Druin et al. (JINR in Dubna) | Dubnium was created by bombarding californium with nitrogen atoms by Ghiorso's team, and by bombarding americium with neon atoms by V. A. Druin's team. | ||
| 106 | Seaborgium | 1974 | A. Ghiorso et al. (Berkeley Radiation Laboratory) | Seaborgium was created by bombarding californium with oxygen atoms. | ||
| 107 | Bohrium | 1981 | G.Münzenberg et al. (GSI in Darmstadt) | Bohrium was made by bombarding bismuth with chromium. | ||
| 109 | Meitnerium | 1982 | G. Münzenberg, P. Armbruster et al. (GSI in Darmstadt) | Meitnerium was created by bombarding bismuth with iron atoms. | ||
| 108 | Hassium | 1984 | G. Münzenberg, P. Armbruster et al. (GSI in Darmstadt) | Hassium was created by bombarding lead with iron atoms. | ||
| 110 | Darmstadtium | 1994 | S. Hofmann et al. (GSI in Darmstadt) | Darmstadtium was created by bombarding lead with nickel. | ||
| 111 | Roentgenium | 1994 | S. Hofmann et al. (GSI in Darmstadt) | Roentgenium was created by bombarding bismuth with nickel. | ||
| 112 | Copernicium | 1996 | S. Hofmann et al. (GSI in Darmstadt) | Copernicium was created by bombarding lead with zinc. | ||
| 114 | Flerovium | 1999 | Y. Oganessian et al. (JINR in Dubna) | Flerovium was created by bombarding plutonium with calcium. | ||
| 116 | Livermorium | 2000 | Y. Oganessian et al. (JINR in Dubna) | Livermorium was created by bombarding curium with calcium. | ||
| 118 | Oganesson | 2002 | Y. Oganessian et al. (JINR in Dubna) | Oganesson was created by bombarding californium with calcium. | ||
| 115 | Moscovium | 2003 | Y. Oganessian et al. (JINR in Dubna) | Moscovium was created by bombarding americium with calcium. | ||
| 113 | Nihonium | 2003–2004 | Y. Oganessian et al. (JINR in Dubna) and K. Morita et al. (RIKEN in Wako, Japan) | Nihonium was created by the decay of moscovium by Oganessian's team, and by bombarding bismuth with zinc by Morita's team. Both teams published their findings in 2004. | ||
| 117 | Tennessine | 2009 | Y. Oganessian et al. (JINR in Dubna) | Tennessine was created by bombarding berkelium with calcium. | ||
See also
- History of the periodic table
- Periodic table
- Extended periodic table
- The Mystery of Matter: Search for the Elements (2014/2015 PBS film)
- Transfermium Wars