Scale Guide

From electron to atoms, to scale

Explore the scale

Nuclei occupy femtometers; atoms extend tens of thousands of times farther because their size is set by electron states rather than the nuclear core.

Shared scale

Each step uses a different kind of size

Shared physical scale
385pm
Electron< 1 × 10-19 m
Proton1.68 fm
Neutron~1.72 fm
Plutonium-244 Nucleus15 fm
Hydrogen Atom100 pm
Cesium Atom520 pm
Embed

These values do not all describe hard edges. The electron is represented by an experimental upper bound; nucleon sizes come from scattering measurements; nuclear size describes a distribution of nuclear matter; atomic diameter depends on how the electron cloud is defined.

From the electron’s upper bound to the cesium atom, the lineup spans more than nine powers of ten.

First threshold

The electron has no measured size

No internal structure has been detected in the electron, so its plotted value is an upper limit. Protons and neutrons are composite baryons made of quarks and gluons; scattering experiments resolve their femtometer-scale distributions, although a neutron does not have a simple charged outer surface.

Shared physical scale
1.41fm
Electron< 1 × 10-19 m
Proton1.68 fm
Neutron~1.72 fm

Nuclear scale

A heavy nucleus is only about nine times wider than a proton

The plutonium-244 nucleus holds 94 protons and 150 neutrons, 244 times as many particles as a lone proton. Nucleons pack at nearly constant density, so nuclear radius grows only roughly with the cube root of the nucleon count.

Shared physical scale
12.2fm

Atomic threshold

The biggest jump is from nucleus to atom

A hydrogen atom is one proton and one electron. Its characteristic diameter is about 60,000 times the proton’s, and almost all of that volume is the electron’s probability cloud rather than packed material.

Shared physical scale
79.1pm

Atomic spread

Atomic size depends on the convention

Atomic radii depend on the convention and chemical environment. Under the convention used here, neutral cesium extends much farther than hydrogen because its outer electron occupies a higher shell. A microwave transition in cesium-133—not the atom’s size—defines the SI second.

Shared physical scale
442pm

Scale anchors

Worth remembering

If a hydrogen atom were a stadium

Blow a hydrogen atom up to 120 meters across and its proton would be a grain about 2 millimeters wide at the center.

The nucleus carries almost all the mass

More than 99.9% of an atom’s mass sits in its nucleus, even though the nucleus fills a tiny fraction of the atom’s volume.

Protons and neutrons are nearly the same size

In the values used here, the proton is 1.68 femtometers across and the neutron 1.72, a difference of about 2%.

More protons do not mean a bigger atom

Cesium has 55 protons to hydrogen’s one, and its atom is about five times wider. Uranium, with 92 protons, is smaller than cesium.

Profiles

The six objects, one by one

Definitions, quoted sizes and caveats for each particle, nucleus and atom above.

Particles

Electron

< 1 × 10-19 mupper bound

The electron is the fundamental particle that gives atoms their chemistry and matter its electric currents. Experiments show no evidence of any internal structure, so its size is represented here by an upper bound rather than a measured diameter.

Object class
Lepton
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Particles

Proton

1.68 fmdiameter

The proton is the positively charged particle that gives every atomic nucleus its identity. Less than 1% of a proton’s mass comes from the masses of its quarks; almost all of the rest comes from the energy of quarks and gluons bound by the strong force.

Object class
Baryon
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Particles

Neutron

~1.72 fmdiameter

The neutron is the electrically neutral baryon that, together with the proton, builds atomic nuclei. A free neutron decays by beta-minus decay into a proton, an electron, and an electron antineutrino in about 15 minutes, while neutron-rich matter can persist inside neutron stars.

Object class
Baryon
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Particles

Plutonium-244 Nucleus

15 fmdiameter

The plutonium-244 nucleus is the heavy atomic nucleus of a long-lived plutonium isotope, built from 94 protons and 150 neutrons. It was forged in rare neutron-rich explosions before the Solar System formed, and its 81.3-million-year half-life made it an important extinct radionuclide in early Solar System history.

Object class
Atomic nucleus
Composition
94 protons, 150 neutrons
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Atoms

Hydrogen Atom

100 pmdiameter

Hydrogen is the universe’s simplest and most common atom. Most hydrogen nuclei were forged in the first minutes after the Big Bang, and neutral hydrogen atoms emerged only after the universe cooled enough for electrons and protons to combine about 380,000 years later.

Object class
Atom
Composition
1 proton, 1 electron
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Atoms

Cesium Atom

520 pmdiameter

Cesium is a large alkali-metal atom with a loosely held outer electron. The fixed frequency of a hyperfine transition in cesium-133 defines the SI second, linking atomic physics to every precise measurement of time.

Object class
Atom
Composition
Cs-133: 55 protons, 78 neutrons, 55 electrons
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Chemistry happens at the outer edge of this lineup. Bonds, colors and reactions involve the electrons around atoms, about a tenth of a nanometer out; the nucleus, tens of thousands of times smaller, matters mainly in radioactivity and nuclear reactions.

Continue with another guide or open the full scale.

About

Scale of Space is a scroll-based journey through the universe, placing objects on a single logarithmic scale so you can compare size across an unbroken range.

Guides explain selected parts of that range, while focused views filter the objects by subject.

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