Dmitri Mendeleev, a Russian chemist, created the first version of the periodic table in 1869 by arranging elements based on their atomic mass and properties.
Mendeleev’s table left gaps for undiscovered elements and accurately predicted properties of elements like gallium, scandium, and germanium before they were found.
Today’s periodic table is arranged by atomic number (number of protons) rather than atomic mass, a change made after Henry Moseley's work in 1913.
The periodic table is based on Periodic Law, which states that the properties of elements recur periodically when arranged by atomic number.
The noble gases (e.g., helium, neon, argon) were discovered after Mendeleev’s time and initially seemed to break the table’s pattern. Their unique stability led to the creation of a new group.
Hydrogen can behave like elements in both Group 1 (alkali metals) and Group 17 (halogens) due to its unique properties, making its placement a topic of debate.
The heaviest naturally occurring element is uranium (U, atomic number 92). Elements beyond uranium, like plutonium (94), are synthetic and created in labs.
There are 24 synthetic elements on the table (atomic numbers 93–118). These are created in particle accelerators or nuclear reactors.
The periodic table has no more "gaps" left for undiscovered elements up to atomic number 118, though scientists are exploring elements beyond this range, known as the island of stability.
Hydrogen (atomic number 1) is the lightest element, while oganesson (atomic number 118) is currently the heaviest known element.
Elements with atomic numbers above 92 are called transuranium elements, all of which are synthetic and radioactive.
Group 1 elements (alkali metals) like sodium and potassium are so reactive that they can explode when exposed to water.
Noble gases in Group 18 (like helium and neon) are incredibly stable because their outer electron shells are full.
Group 17 elements (halogens) like chlorine, fluorine, and iodine are known for their antibacterial and disinfectant properties.
Gold (Au) is the only metal that doesn’t form a naturally occurring oxide, making it resistant to tarnishing and corrosion.
Transition metals (Groups 3–12) like iron, copper, and gold are widely used due to their malleability, conductivity, and catalytic properties.
These two rows below the main table contain elements that are crucial for modern technologies like smartphones, lasers, and nuclear reactors.
Carbon (C) is the backbone of organic chemistry and life itself, forming millions of compounds and serving as the basis for DNA, proteins, and more.
Many elements are named after scientists (e.g., Einsteinium), places (e.g., Californium), or mythological figures (e.g., Thorium).
Helium is the second most abundant element in the universe but is relatively rare on Earth. It was first discovered in the Sun's spectrum before being found on Earth.
The periodic table’s distinctive "stair-step" shape reflects elements' increasing atomic numbers and their electron configurations.
Periodic tables are often color-coded to represent element groups (e.g., metals, nonmetals, and metalloids) and physical states (solid, liquid, gas).
Oxygen is the most abundant element in the Earth's crust, while hydrogen dominates the universe.
Superheavy elements (like flerovium, atomic number 114) are synthesized in labs, lasting only fractions of a second before decaying.
Scientists are working on expanding the table beyond 118 elements, exploring theoretical elements in the eighth period.