History of the periodic table
Adapted from Wikipedia · Discoverer experience
The periodic table is a special chart that organizes all the building blocks of matter, called chemical elements. It arranges these elements based on their tiny parts called atomic number and how their electrons are arranged, which affects how they react with each other. In the table, elements are listed in order of their atomic number, and they are placed in rows and columns so that elements with similar properties line up.
The story of how the periodic table was created spans more than two hundred years. Many smart people helped shape our understanding, including Antoine-Laurent de Lavoisier, Johann Wolfgang Döbereiner, John Newlands, Julius Lothar Meyer, Dmitri Mendeleev, and Glenn T. Seaborg. Their work showed patterns in how elements behave, leading to the organized table we use today. This table helps scientists predict how elements will react and is a key tool in chemistry.
Early history
Further information: Classical element
Long ago, in the 5th century BCE, thinkers like Leucippus and Democritus thought that everything in the world is made of tiny, tiny parts called "atoms." They believed these atoms were too small to see, came in many kinds, and had always existed.
Later, around 330 BCE, Aristotle suggested that everything was made from mixes of four basic things: earth, water, air, and fire. Other cultures, like Indian philosophy, had similar ideas but included a fifth element called aether.
Some elements we know today, like carbon, sulfur, iron, and copper, have been known for thousands of years because they can be found in nature. Even more elements were discovered later during the time of alchemy.
First classification
The history of the periodic table is also the history of discovering chemical elements. In 1661, Boyle described elements as simple substances that make up more complex ones.
One of the first people to discover a new element was Hennig Brand, a German merchant. In 1669, his experiments created a glowing white substance called phosphorus. This discovery raised questions about what makes something an element.
In 1789, Antoine Lavoisier wrote the first modern chemistry textbook. He listed elements like oxygen, nitrogen, and hydrogen, and divided them into metals and nonmetals.
Later, scientists like Johann Döbereiner noticed patterns, grouping elements into sets of three with similar properties, called triads. These early attempts helped lay the groundwork for the periodic table we use today.
Comprehensive formalizations
French geologist Alexandre-Émile Béguyer de Chancourtois noticed that when elements are arranged by their atomic weights, they show similar properties at regular intervals. In 1862, he created a three-dimensional chart called the "telluric helix" using the element tellurium. By placing the elements in a spiral on a cylinder, he saw that elements with similar properties lined up vertically.
Later, British chemist John Newlands observed that elements showed recurring trends in their properties every eight elements, similar to notes in a musical scale. However, his ideas were not accepted by others at the time. Around the same time, German chemist Lothar Meyer also studied patterns in the elements. In 1864, he published a version of the periodic table with 28 elements, grouping them by their valence.
In 1869, Russian chemist Dmitri Mendeleev arranged 63 elements by their atomic weights and noticed patterns in their properties. He created a table that helped predict missing elements and correct mistakes in known atomic weights. Mendeleev shared his table widely and continued to improve it over the years.
Priority dispute and recognition
In 1881, a scientist named Mendeleev said he should get credit for creating the periodic table. He believed that the true creator of an idea was the one who could show its real value and make others believe in it.
Mendeleev made guesses about elements that had not yet been discovered. He gave names like eka-boron and eka-aluminium to these missing pieces. Later, these elements were found and named scandium and gallium, which matched his guesses closely. This helped many scientists accept his version of the periodic table.
At first, not everyone agreed about who should get credit for the periodic table. Mendeleev worked hard to share his ideas, while another scientist, Meyer, did not push his work as much. Over time, Mendeleev’s table became widely accepted as the standard way to organize the elements. By 1890, everyone knew about Mendeleev’s table and its helpful way of grouping the elements together.
| Name | Atomic weight | Modern name (year of discovery) | |
|---|---|---|---|
| Mendeleev | Modern | ||
| Ether | 0.17 | — | — |
| Coronium | 0.4 | — | — |
| Eka-boron | 44 | 44.6 | Scandium |
| Eka-cerium | 54 | — | — |
| Eka-aluminum | 68 | 69.2 | Gallium |
| Eka-silicon | 72 | 72.0 | Germanium |
| Eka-manganese | 100 | 99 | Technetium (1937) |
| Eka-niobium | 142 | — | — |
| Eka-molybdenum | 146 | — | — |
| Eka-cadmium | 155 | — | — |
| Eka-iodine | 170 | — | — |
| Tri-manganese | 190 | 186 | Rhenium (1925) |
| Eka-caesium | 175 | — | — |
| Dvi-tellurium | 212 | 210 | Polonium (1898) |
| Dvi-caesium | 220 | 223 | Francium (1939) |
| Eka-tantalum | 235 | 231 | Protactinium (1913) |
Inert gases and ether
British chemist Henry Cavendish discovered that air contains more than just nitrogen and oxygen. He found this out in the late 1700s. Later, in 1868, helium was found in sunlight using a special tool called spectroscopy.
In 1894, William Ramsay and Lord Rayleigh discovered a new gas called argon in air. Argon did not react with other elements, which was unusual. This discovery challenged how scientists thought about arranging elements. Later, Ramsay discovered more gases like neon, krypton, and xenon in 1898. These gases, now called noble gases, were added to the periodic table in a new group.
The placement of these gases in the table was debated. Some scientists thought they should go between certain groups of elements. Eventually, they were placed in a new group called group 0. This helped organize the table better and make space for other elements like the rare-earth elements or lanthanides.
At the time, some believed there was a special substance called the ether that filled space. Dmitri Mendeleev, who created the periodic table, thought ether might be a very light gas that did not react with other elements. However, experiments later showed that such a substance did not exist.
Atomic theory and isotopes
Radioactivity and isotopes
Main articles: Radioactive decay and Isotope
In 1907, scientists found that thorium and radiothorium, which come from radioactive decay, looked different but acted the same chemically. This led to the idea that they were the same element but with different weights. These were called isotopes.
When scientists first found radioactive elements like radium, actinium, thorium, and uranium around 1900, they placed them at the bottom of the periodic table because they were heavier than other elements. Over the next ten years, many new radioactive substances were discovered, including radon. By 1912, almost 50 different radioactive substances had been found. Some scientists thought these discoveries might change the periodic table because there wasn’t enough space for all of them.
Rutherford model and atomic number
Main articles: Rutherford model and Atomic number
In 1913, a scientist named Antonius van den Broek suggested that the atomic number decided where elements should go in the periodic table. He guessed the atomic numbers for elements up to tin. However, he couldn’t test his idea.
Later, Henry Moseley tested this idea by studying X-rays from different elements. He found that the atomic number was key to ordering the elements correctly. This helped fix problems where ordering by weight didn’t match chemical properties. For example, he showed that argon should come before potassium and cobalt before nickel.
Electron shell and quantum mechanics
In 1914, Johannes Rydberg noticed patterns in the atomic numbers of noble gases. These patterns helped explain why periods in the periodic table had fixed lengths. This idea led to the modern understanding of electron shells and orbitals.
During the 1910s and 1920s, new ideas about quantum mechanics changed how we understand atoms and the periodic table. These ideas helped explain why elements in the same group behave similarly and why noble gases are unreactive.
Proton and neutron
Main articles: Proton and Neutron
The discovery of protons and neutrons showed that atoms are made of smaller parts. This led to the modern definition of an element as atoms with a certain number of protons, which is the atomic number. It also helped explain some types of radioactive decay.
From short form into long form (into -A and -B groups)
Around 1925, the periodic table was updated by moving some series to the right, creating extra columns called groups. The original groups I to VII were repeated, with "A" and "B" added to them. Group VIII, which had three columns, stayed as it was.
This change moved series 4 and 5 to form a new period 4 with groups IA to VIIA, VIII, and IB to VIIB.
| modern (long): | IUPAC group | 1 | 2 | no number | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | × | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | |
| 1900+ (long): | old IUPAC (A–B, Europe) | IA | IIA | IIIA | IVA | VA | VIA | VIIA | VIIIB | IB | IIB | IIIB | IVB | VB | VIB | VIIB | 0 | |||||
| CAS (A–B–A, US) | IA | IIA | IIIB | IVB | VB | VIB | VIIB | VIIIB | IB | IIB | IIIA | IVA | VA | VIA | VIIA | VIIIA | ||||||
| 1871 (short)→ | Gruppe | IA | IIA | [ ] | IIIB | IVB | VB | VIB | VIIB | VIIIB | IB | IIB | IIIB | IVB | VB | VIB | VIIB | 0 | ||||
| Period ① | Reihe 1 | H | He | |||||||||||||||||||
| Period ② | Reihe 2 | Li | Be | B | C | N | O | F | Ne | |||||||||||||
| Period ③ | Reihe 3 | Na | Mg | Al | Si | P | S | Cl | Ar | |||||||||||||
| Period ④ | Reihe 4 | K | Ca | –Sc | Ti | V | Cr | Mn | Fe | Co | Ni | Cu(1st) | ||||||||||
| Reihe 5 | (Cu)(2nd) | Zn | – Ga | – Ge | As | Se | Br | Kr | ||||||||||||||
| Period ⑤ | Reihe 6 | Rb | Sr | Yt[=Y] | Zr | Nb | Mo | –([Tc]) | Ru | Rh | Pd | Ag(1st) | ||||||||||
| Reihe 7 | (Ag)(2nd) | Cd | In | Sn | Sb | Te | J[=I] | Xe | ||||||||||||||
| Period ⑥ | Reihe 8 | Cs | Ba | [La–Lu] | ?Di[La] | ?Ce[Ce] | — | — | — | — | — | — | —(1st) | |||||||||
| Reihe 9 | (—)(2nd) | — | — | — | — | — | — | |||||||||||||||
| Period ⑥ | Reihe 10 | — | — | ?Er Yb ([Lu]) | ?La – ([Hf]) | Ta | W | –([Re]) | Os | Ir | Pt | Au(1st) | ||||||||||
| Reihe 11 | (Au)(2nd) | Hg | Tl | Pb | Bi | —[Po] | —[At] | [Rn] | ||||||||||||||
| Period ⑦ | Reihe 12 | —[Fr] | —Rd[=Ra] | [Ac–Lr] | —[Ac] | Th | —[Pa] | U | — | — | — | — | — | |||||||||
| Bold text | in Periodic Table 1871 |
| Italic text | in Periodic Table 1906 (the last by Mendeleev) |
| Regular text (not bold) | added after 1906 |
| begin–end of 1871 Reihe | |
| – Ga | Element predicted, later proven correct within Mendeleev's lifetime and added by him |
| – (Tc) | Element predicted, later proven correct posthumously |
| – | Element projected, but not predicted |
| strikethrough | Element predicted, later proven wrong due to – not an element ("?Di"), or –wrong position ("[Ac]") because of non-recognition of separate rare earth series |
| [ ] | Added or changed after 1871 |
| Cu(1st) × / (Cu)(2nd) | Element mentioned twice: in Gruppe VIII and I. The 2nd mentioning survived, Gruppe/group VIII was reduced from four columns to three (×) |
| Published 1871, English version: "Reihen" translated as "Series" (that is, arrays with regularity not just rows). Reproduced in Scerri (2007), p. 111 | |
Later expansions and the end of the periodic table
The periodic table has grown over time, especially with the discovery of new elements. Scientists have added elements that sit below the main table, called the actinides. These elements behave in special ways because of how their electrons are arranged.
One scientist, Glenn T. Seaborg, suggested placing these actinides in a special row below the main table. This helped explain why some elements acted differently than expected. As new elements continue to be discovered, scientists are exploring how they might fit into the table and whether the patterns we see today will still work for these very heavy elements.
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