Matter & Energy · Depth 2 · Introductory · 8 min read
Atoms & Chemistry
What atoms are made of, elements and isotopes, how atoms bond, the states of matter, and what happens to mass and energy in reactions.
On this page
- What this part of the map covers
- Inside the atom
- The nucleus
- Electrons and shells
- Elements and the periodic table
- Isotopes
- Chemical bonds
- States of matter
- Conservation of mass
- Energy in chemical reactions
- Catalysts
- The math (optional)
- Common misconceptions
- What this page does not cover yet
- Going further
- Real-life examples
- Evidence & sources
What this part of the map covers
All matter is made of atoms, and atoms can join with other atoms to form molecules.[1] This page looks at what atoms are made of, how elements and isotopes differ, how atoms bond, the states that matter takes, what happens to mass and energy in a reaction, and what catalysts do.
Inside the atom
An atom is a cloud of electrons around a dense nucleus of protons and neutrons, and the nucleus is 100,000 times smaller than the atom.[2] Protons carry a positive electric charge and neutrons carry none.[4, 3] The strong force, the strongest fundamental force known, holds the nucleus together.[4]
Electrons are different: they are elementary particles, not made of anything smaller, and they sit around the nucleus rather than inside it.[5] An atom with more or fewer electrons than protons is an ion: a negative ion is an anion and a positive one a cation.[5]
The nucleus
In 1911, Ernest Rutherford found that every atom has a nucleus at its core.[4] The nucleus takes up much less than 0.01% of an atom’s volume, yet typically holds more than 99.9% of its mass.[4]
Electrons and shells
Scientists once pictured electrons circling the nucleus the way the Moon orbits Earth.[5] Today they describe a cloud divided into shells, where different regions have different chances of holding an electron.[5] An electron that gains energy can become excited, and when it drops back the atom gives off a photon, a particle of light, with wavelengths that are specific to each element.[5]
In 1913, Niels Bohr published three important papers on the structure of atoms.[13] Drawing on quantum ideas from Planck and Einstein, he proposed that an atom can exist only in a set of separate, stable energy states.[13] The story of that quantum revolution, and of how mass and energy relate, is on the Modern Physics page.
Elements and the periodic table
The number of protons, the atomic number (Z), decides which element an atom is.[2, 3] The electrons, meanwhile, determine the element’s chemical properties.[2, 4] An element whose two outer shells are full is much less reactive with other elements.[5]
For more than a century, the periodic table has guided people through the elements by showing where their chemical properties are alike and where they differ.[10] IUPAC, the International Union of Pure and Applied Chemistry, publishes a Periodic Table of the Elements and Isotopes to show students, teachers and the public that isotopes exist and matter.[9]
Isotopes
Isotopes are atoms of one element that share the same number of protons but have different numbers of neutrons, so their mass number (A) differs.[2, 6] Carbon occurs naturally as carbon-12 (6 neutrons), carbon-13 (7) and carbon-14 (8).[6]
Isotopes of one element behave almost identically in chemistry, but their nuclei behave differently.[2] Some are stable and some are unstable, or radioactive, meaning the nucleus may change on its own over time, turning a “parent” into a “daughter” isotope that may belong to another element.[6, 2] The half-life is the time it takes for half of a radioactive material to decay.[2]
Chemical bonds
Gerald Bergtrom of the University of Wisconsin-Milwaukee, in an open university textbook, puts it simply: atoms form bonds to make molecules.[15] The electromagnetic pull that keeps electrons around a nucleus is also what lets bonds form.[14] Atoms are most stable when their outer shell of electrons is filled, and they can get there by sharing electrons or by gaining or losing them.[15]
In a covalent bond, atoms share electrons.[15] In hydrogen gas (H2), one pair of electrons, shared equally, bonds two hydrogen atoms into a molecule.[15] In methane, a carbon atom shares the four electrons of its outer shell with four hydrogen atoms, so the outer shells of all of them are filled at least some of the time.[15] Equal sharing makes a non-polar covalent bond and unequal sharing a polar one.[15] Organic molecules with the same formula but different shapes are called isomers, and one cannot be turned into another without breaking covalent bonds.[17]
Water’s bonds are polar: oxygen’s larger nucleus pulls the shared electrons more strongly than hydrogen does, so the oxygen carries a partial negative charge and each hydrogen a partial positive one.[15] Those charges let water molecules attract one another through hydrogen bonds, a kind of attraction between opposite charges.[16] That polarity also makes water a good solvent, while non-polar fats and oils do not dissolve in it.[16]
Atoms that fill their outer shell by gaining or losing electrons become stable ions.[15] Sodium can give one electron to chlorine, making Na+ and Cl− ions, and the attraction of their opposite charges, an ionic bond, holds them together in crystals of salt.[15] Ionic bonds are weaker than covalent ones.[15]
States of matter
Matter normally exists as a solid, a liquid or a gas.[1] A solid keeps its own shape and volume, while a gas fills whatever container holds it; liquids and gases can flow, so both are called fluids.[1] If atoms gain enough energy, electrons break free and mix with ions to form a fourth state, plasma.[5, 1]
Conservation of mass
In a chemical reaction the bonds between atoms are broken and rebuilt, joining the atoms into new molecules.[7] The total number of atoms stays the same, and so mass is conserved.[11, 12]
Energy in chemical reactions
Chemistry is a matter of electrons: in a reaction, atoms can share, gain or lose electrons, but they never gain or lose protons or neutrons.[15]
Bergtrom sorts energy into two broad kinds: potential (stored) and kinetic, which includes heat, electricity, sound and light.[18] Chemical energy is a form of potential energy.[18]
A reaction that releases heat is exothermic; one that absorbs heat is endothermic.[19] Either way, no energy is created or destroyed: it can only be moved from one place to another or converted from one form to another.[19]
Catalysts
A catalyst speeds up a chemical reaction, or lowers the temperature or pressure needed to start it, without being used up.[7] It does this by lowering the activation energy, the energy barrier a reaction has to get over.[7] People have used them for thousands of years, and newer catalysts have led to biodegradable plastics, new medicines and cleaner fuels and fertilizers.[7]
Even without a catalyst, adding more reactants or raising the temperature speeds a reaction up, because the molecules collide more often.[20]
The math (optional)
Isotopes are written as the element’s name or symbol, a hyphen and the mass number, as in carbon-14 or C-14; a trailing “m”, as in technetium-99m, marks a metastable state of the nucleus.[2]
Electron arrangements are written as configurations. NIST lists hydrogen as 1s1 and carbon as [He] 2s2 2p2, where [He] means every subshell belonging to helium is full.[8]
In a chemical formula, subscripts count the atoms of each element in a molecule, and in a reaction, coefficients count the molecules.[11]
Common misconceptions
“Electrons orbit the nucleus like tiny planets.” That was the older picture; scientists now describe shells in which electrons are found with different probabilities.[5]
“Every isotope is radioactive.” Isotopes come in two main types, stable and radioactive, and carbon-12, for one, never decays.[6]
“An element’s atomic weight is a fixed constant.” IUPAC stresses that atomic weights are not constants of nature, and for elements whose atomic weight varies in a well-documented way, the standard value is given as an interval.[10, 9]
“Boiling or freezing water makes a new substance.” Changes of state are physical changes, not chemical ones: water vapour, liquid water and ice are all H2O.[1]
What this page does not cover yet
We have not yet found sources good enough for these subjects, so this page leaves them out for now: metallic bonds, electronegativity, double and triple bonds, bond energies, worked examples of balancing chemical equations, types of reaction such as combustion or decomposition, reaction rates in numbers, acids, bases and pH, and the history of the periodic table and the periodic law.
Going further
Start with Electric Charge, then see Modern Physics for the quantum atom and mass-energy, Heat & Thermodynamics and Light & Waves.
Real-life examples
Dating old things with carbon-14
Carbon-14 is radioactive with a half-life of about 5,730 years, so the amount left in an object works like a clock that shows its age.[6]
Isotopes in hospitals
Strontium-82 decays to rubidium-82 with a half-life of 25 days, which makes it useful in generators that supply rubidium-82 for heart scans by positron emission tomography (PET).[2]
Ice, water and steam
Under standard atmospheric conditions, water turns to ice below 0 degrees Celsius (32 °F) and to vapour above 100 degrees Celsius (212 °F), yet a molecule of each is still H2O.[1]
Making bread
The yeast in bread dough contains enzymes, natural catalysts that help turn flour into bread.[7]
Air and water on the space station
On the International Space Station, recycled water is split by electrolysis to make fresh oxygen for the crew, an example NASA's education team uses to teach the conservation of mass.[12]
Instant cold packs
Squeeze a chemical cold pack and the reaction inside starts absorbing heat from its surroundings, so the temperature around it drops: an endothermic reaction.[19]
Connected across the map
- Electric ChargeThe basic property behind all electricity: two kinds of charge that attract or repel, and are moved around but never created or destroyed.
- Heat & ThermodynamicsHeat, temperature and the four laws of thermodynamics: how heat moves, why no engine is perfect, and how fridges and heat pumps work.
- Modern PhysicsRelativity and quantum physics: the ideas from about 1900 to 1930 that changed how we understand space, time, light and atoms.
- Light & WavesWhat waves are, how sound travels, the electromagnetic spectrum from radio waves to gamma rays, and how light reflects, bends and interferes.
- GeologyThe science of the solid Earth: its layers, its moving plates, the rocks and minerals it is made of, and the long history its rocks record.
Learn more
Short descriptions are our own summaries. The resources belong to, and are run by, their publishers.
- Build an Atom (interactive simulation) ↗
by PhET
Add protons, neutrons and electrons one at a time and watch the element, charge and mass change: a free browser simulation from the University of Colorado Boulder.
- Isotopes and Atomic Mass (interactive simulation) ↗
by PhET
Change the number of neutrons to make different isotopes of an element, and see how the mix of isotopes sets the average atomic mass.
- States of Matter: Basics (interactive simulation) ↗
by PhET
Heat, cool and squeeze atoms and molecules and watch them change between solid, liquid and gas.
Evidence & sources
Supported by extensive evidence and broad scientific consensus.
Why this level? Atomic structure, isotopes, chemical bonds, the states of matter, the conservation of mass and the energy of reactions are long-established science taught in every introductory course. The atom, isotope, state and mass sections are written from US government science agencies (the Department of Energy and its Isotope Program, NIST and NASA) and IUPAC, the international body for chemistry, with history from MacTutor (University of St Andrews); bonds, reaction energy and reaction rates come from an open university textbook by Gerald Bergtrom (University of Wisconsin-Milwaukee).
Keep in mind: Chemical bonds, the energy of reactions and reaction rates rest on one university textbook, written for cell biology, with no second institution confirming them; the states of matter and the conservation of mass rest on NASA teaching material alone. The page does not cover metallic bonds, electronegativity, double and triple bonds, practice in balancing equations, types of reaction, or acids and bases.
This is a Knowledge Atlas editorial classification of the sources we could find, not a certificate of truth. How we evaluate knowledge
Sources
Based on 20 sources from 6 institutions: NASA, DOE, NIST, IUPAC, MacTutor and 1 more.
Show all 20 sourcesHide the list
- National Aeronautics and Space Administration· Government agencyPhases of MatterOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyNIDC: National Isotope Development CenterOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyDOE Explains...ProtonsOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyDOE Explains...NucleiOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyDOE Explains...ElectronsOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyDOE Explains...IsotopesOpened and checked against this page on 30 Sept 2026
- U.S. Department of Energy· Government agencyDOE Explains...CatalystsOpened and checked against this page on 30 Sept 2026
- National Institute of Standards and Technology· Government agencyElectronic configurations of the elementsOpened and checked against this page on 30 Sept 2026
- International Union of Pure and Applied Chemistry· Professional bodyIUPAC Periodic Table of the Elements and Isotopes (IPTEI) for the Education CommunityOpened and checked against this page on 30 Sept 2026
- International Union of Pure and Applied Chemistry· Professional bodyCommission on Isotopic Abundances and Atomic WeightsOpened and checked against this page on 30 Sept 2026
- National Aeronautics and Space Administration· Government agencynasa-conservation-of-mass-pdfOpened and checked against this page on 30 Sept 2026
- National Aeronautics and Space Administration· Government agencySTEMonstrations: Conservation of Mass - NASAOpened and checked against this page on 30 Sept 2026
- ScholarlyMacTutor History of Mathematics (University of St Andrews)· UniversityNiels Bohr: biography (MacTutor)Opened and checked against this page on 30 Sept 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University2.2: Atoms and Basic ChemistryOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University2.3: Chemical bondsOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University2.4: A Close Look at Water ChemistryOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University2.5: Some Basic Biochemistry- Carbon, Monomers, Polymers and the Synthesis and Degradation of MacromoleculesOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University4.2: Kinds of EnergyOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University4.3: Deriving Simple Energy RelationshipsOpened and checked against this page on 1 Oct 2026
- ScholarlyUniversity of Wisconsin-Milwaukee (G. Bergtrom, Basic Cell and Molecular Biology)· University5.2: EnzymesOpened and checked against this page on 1 Oct 2026