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Last update: 30 August 2026

How Do We See the Hidden Structure of Atoms?

Seeing Atoms: An Exploration of Atomic Structure

Structure of the helium atom: At the centre, the compact nucleus made of 2 protons and 2 neutrons (scale: 1 femtometre). Around it, the fuzzy electron cloud represents the probability of presence of electrons in their ground state (1s).
Image source: Wikipedia (new window) — public domain.

Scientific abstract

Astronoo's article presents atoms, the fundamental building blocks of matter. It traces the history of their discovery, from antiquity to Rutherford, and explains their structure: a dense nucleus and an electron cloud. Atomic stability, inexplicable in classical physics, is resolved by quantum mechanics and the Schrödinger equation. The article shows images of a gold surface obtained by scanning tunnelling microscopy, illustrating the direct visualisation of atoms, as well as IBM's historic feat in 1990 of positioning atoms one by one. It also covers atomic radii, their variability, and recent advances in atomic force microscopy.

How have scientists managed to see and understand the structure of the atom, that elusive entity?

The article explores atomic structure, from the early hypotheses of the Greek philosophers to the modern images obtained by scanning tunnelling microscopy. It details the size, mass and composition of atoms, as well as the paradox of their stability, resolved by quantum mechanics. The reader discovers that the atom is not indivisible, but is made up of a nucleus and an electron cloud. Technological advances, such as STM, now make it possible to visualise atoms directly, as shown by the gold image, and even to move them one by one, as IBM demonstrated as early as 1990. The article also discusses the quantisation of energy levels and the distribution of nucleons. This journey to the heart of matter reveals the complexity and elegance of the infinitely small, and answers the fundamental question: what do we really know about the atom?

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Structure of the atom

History and discovery of the atom

Everything we see is made up of atoms, lots of atoms from the Greek word "atomos" (indivisible). Long ago, in the 4th century BC, the Greek philosophers Leucippus and Democritus put forward the hypothesis that all matter is composed of tiny particles in perpetual motion, very solid and eternal. Today we have a slightly more precise idea of the atom, because it is not indivisible.

Its approximate size has been known since 1811, when Amedeo Avogadro estimated the size of atoms to be 10-10 metre. In 1911, Ernest Rutherford refined the structure of the atom and gave the atomic nucleus a size of around 10-14 metre.

Size, mass and composition of the atom

As for the size of atoms, we speak of atomic orbitals, i.e. the electron cloud surrounding the nucleus. This cloud has a theoretical diameter ranging from 62 pm (picometres) for the helium atom to 596 pm for the caesium atom. Nothing is simple in the nature of matter, and this tiny distance varies according to the chemical nature of the surrounding atoms.

Although the nucleus contains most of the mass of the atom (99.99%), its mass is also known; for stable atoms, it ranges from 1.674×10-24 g for hydrogen to 3.953×10-22 g for uranium.

Its composition is also known: inside we see a nucleus and an electron cloud that occupies the entire spatial extent of the atom, since it is about 100,000 times larger than its nucleus. Even more astonishing, we even know, to an order of magnitude, the number of atoms in the observable universe: it is estimated at about 1080, i.e. a 1 followed by 80 zeros — a value obtained by combining the estimated number of stars (about 1023) and their average mass converted into an equivalent number of hydrogen atoms.

The stability of atoms

The paradox of classical physics

The stability of the atom cannot be explained by classical physics, because in classical physics, the electron particle, negatively charged, and the proton, positively charged, raise a paradox.

In classical physics, matter should disappear, annihilate itself, because an electron radiating around a nucleus loses energy (Maxwell's theory) and should therefore fall onto the nucleus. This means that the stability of an atom is incomprehensible within the framework of classical theory.

The solution of quantum mechanics

The scientific geniuses of the 20th century resolved this paradox in 1924, thanks to the wave mechanics of Louis de Broglie (1892-1987), generalised in 1926 by Erwin Schrödinger (1887-1961), Nobel Prize in Physics in 1933 with Paul Dirac (1902-1984), for the wave equation called the Schrödinger equation.

In quantum mechanics, it is not possible to know exactly the value of a parameter without measuring it. The mathematical theory describes a state not by a precise pair of velocity and position, but by a wave function (state vector), which allows the probability of finding the particle at a given point to be calculated. Hence the probabilistic nature of quantum mechanics, which predicts that particles are also waves and no longer just material points.

Orbitals and chemical bonds

Electrons occupy atomic orbitals in interaction with the nucleus via the electromagnetic force, while nucleons are held together within the nucleus by the nuclear bond.

The electron cloud is stratified into quantised energy levels around the nucleus, defining electron shells and subshells. Nucleons are also distributed in nuclear shells, although a fairly convenient model popularises the nuclear structure based on the liquid drop model.

Several atoms can form chemical bonds with each other through their electrons, and in general, the chemical properties of atoms are determined by their electronic configuration, which follows from the number of protons in their nucleus. This number, called the atomic number, defines a chemical element.

Visible gold atoms

Observation of gold atoms by scanning tunnelling microscope

At the closest to matter, the surface of a sheet of pure gold (Au 100) is detailed here by a scanning tunnelling microscope. The gold atoms visible in this image are regularly spaced on the crystalline structure of gold. This atomic image was obtained with a low-temperature Omicron STM by Erwin Rossen, Eindhoven University of Technology, in 2006.

Image of pure gold atom seen by scanning tunnelling microscope

Gold atoms viewed by scanning tunnelling microscope (STM): Image of a gold surface Au(100) resolved at the atomic scale (2006). The regular bands visible in the image illustrate the "quasi-hexagonal" surface reconstruction characteristic of this face of the gold crystal: the denser upper atomic layer rearranges into a slightly compressed hexagonal pattern resting on the underlying cubic lattice, producing these rows of atoms with a slight offset.
Image source: Erwin Rossen (new window), Eindhoven University of Technology, 2006 — public domain.

IBM's historic feat: writing with atoms

Seeing atoms is one thing; moving them one by one is another. This is what physicists Donald Eigler and Erhard Schweizer from the IBM Almaden Research Center in California demonstrated in November 1989. Using the tip of a scanning tunnelling microscope as an atomic tweezer, they moved one by one 35 xenon atoms on a nickel surface cooled to 4 kelvins (i.e. -269°C) to form the three letters "IBM". The painstaking operation took about 22 hours. The logo obtained measured only 5 nanometres high by 17 nanometres wide — about 500,000 times smaller than ordinary printed letters. Published in 1990 in the journal Nature, this image has become emblematic of the birth of nanoscience: it proved that the scanning tunnelling microscope could not only observe atoms, but also manipulate them and literally build with the most elementary matter there is. This atom-by-atom manipulation technique remains a laboratory tool rather than an industrial manufacturing process, because the required conditions (high vacuum, near absolute zero temperature) are too restrictive for mass production.

Beyond STM: atomic force microscopy and recent advances

The scanning tunnelling microscope (STM) has a limitation: it requires a conductive surface, because it measures a current of electrons that "tunnel" between the tip and the sample. To study insulating materials or individual molecules, researchers use a complementary technique developed in 1986: atomic force microscopy (AFM), which measures not a current but the interaction force between an ultrafine tip and the atoms on the surface, allowing virtually any material to be probed.

Since the mid-2010s, these techniques have made a leap forward. In 2023, a research team used AFM to directly observe the signature of electron orbitals of single metal atoms within organic molecules, a feat that confirms, at the scale of a single atom, the shapes predicted for a century by the Schrödinger equation. The same year, another team developed a technique based on scanning transmission electron microscopy (STEM) capable of mapping electron density at the atomic scale in two-dimensional materials. These measurements remain indirect — we do not "photograph" an electron as an ordinary object — but they bring theoretical quantum physics a little closer to direct observation every year.

Size of atoms

Atomic radii of elements

Theoretical (calculated) atomic radius of some atoms (size in picometres (10-12 metre). The atomic radius is half the distance between the nuclei of two adjacent atoms. The values given in this table are indicative only.

Theoretical size of atoms in picometers (pm)
(1 pm = 10-12 meter)
ElementSizeElementSizeElementSizeElementSize
H  Hydrogen :
number of electrons per energy level 1
53Ca Calcium :
number of electrons per energy level 2, 8, 8, 2
194Y  Yttrium :
number of electrons per energy level 2, 8, 18, 9, 2
212Hf Hafnium :
number of electrons per energy level 2, 8, 18, 32, 10, 2
208
He Helium :
number of electrons per energy level 2
31Sc Scandium :
number of electrons per energy level 2, 8, 9, 2
184Zr Zirconium :
number of electrons per energy level 2, 8, 18, 10, 2
206Ta Tantalum :
number of electrons per energy level 2, 8, 18, 32, 11, 2
200
Li Lithium :
number of electrons per energy level 2, 1
167Ti Titanium :
number of electrons per energy level 2, 8, 10, 2
176Nb Niobium :
number of electrons per energy level 2, 8, 18, 12, 1
198W  Tungsten :
number of electrons per energy level 2, 8, 18, 32, 12, 2
193
Be Beryllium :
number of electrons per energy level 2, 2
112V  Vanadium :
number of electrons per energy level 2, 8, 11, 2
171Mo Molybdenum :
number of electrons per energy level 2, 8, 18, 13, 1
190Re Rhenium :
number of electrons per energy level 2, 8, 18, 32, 13, 2
188
B  Boron :
number of electrons per energy level 2, 2
87Cr Chromium :
number of electrons per energy level 2, 8, 13, 1
166Tc Technetium :
number of electrons per energy level 2, 8, 18, 13, 2
183Os Osmium :
number of electrons per energy level 2, 8, 18, 32, 14, 2
185
C  Carbon :
number of electrons per energy level 2, 4
67Mn Manganese :
number of electrons per energy level 2, 8, 13, 2
161Ru Ruthenium :
number of electrons per energy level 2, 8, 18, 15, 1
178Ir Iridium :
number of electrons per energy level 2, 8, 18, 32, 15, 2
180
N  Nitrogen :
number of electrons per energy level 2, 5
56Fe Iron :
number of electrons per energy level 2, 8, 14, 2
156Rh Rhodium :
number of electrons per energy level 2, 8, 18, 16, 1
173Pt Platinum :
number of electrons per energy level 2, 8, 18, 32, 17, 1
177
O  Oxygen :
number of electrons per energy level 2, 6
48Co Cobalt :
number of electrons per energy level 2, 8, 15, 2
152Pd Palladium :
number of electrons per energy level 2, 8, 18, 18
169Au Gold :
number of electrons per energy level 2, 8, 18, 32, 18, 1
174
F  Fluorine :
number of electrons per energy level 2, 7
42Ni Nickel :
number of electrons per energy level 2, 8, 16, 2 or 2, 8, 17, 1
149Ag Silver :
number of electrons per energy level 2, 8, 18, 18, 1
165Hg Mercury :
number of electrons per energy level 2, 8, 18, 32, 18, 2
171
Ne Neon :
number of electrons per energy level 2, 8
38Cu Copper :
number of electrons per energy level 2, 8, 18, 1
145Cd Cadmium :
number of electrons per energy level 2, 8, 18, 18, 2
161Tl Thallium :
number of electrons per energy level 2, 8, 18, 32, 18, 3
156
Na Sodium :
number of electrons per energy level 2, 8, 1
190Zn Zinc :
number of electrons per energy level 2, 8, 18, 2
142In Indium :
number of electrons per energy level 2, 8, 18, 18, 3
156Pb Lead :
number of electrons per energy level 2, 8, 18, 32, 18, 4
154
Mg Magnesium :
number of electrons per energy level 2, 8, 2
145Ga Gallium :
number of electrons per energy level 2, 8, 18, 3
136Sn Tin :
number of electrons per energy level 2, 8, 18, 18, 4
145Bi Bismuth :
number of electrons per energy level 2, 8, 18, 32, 18, 5
143
Al Aluminium :
number of electrons per energy level 2, 8, 3
118Ge Germanium :
number of electrons per energy level 2, 8, 18, 4
125Sb Antimony :
number of electrons per energy level 2, 8, 18, 18, 5
133Po Polonium :
number of electrons per energy level 2, 8, 18, 32, 18, 6
135
Si Silicon :
number of electrons per energy level 2, 8, 4
111As Arsenic :
number of electrons per energy level 2, 8, 18, 5
114Te Tellurium :
number of electrons per energy level 2, 8, 18, 18, 6
123At Astatine :
number of electrons per energy level 2, 8, 18, 32, 18, 7
127
P  Phosphorus :
number of electrons per energy level 2, 8, 5
98Se Selenium :
number of electrons per energy level 2, 8, 18, 6
103I  Iodine :
number of electrons per energy level 2, 8, 18, 18, 7
115Rn Radon :
number of electrons per energy level 2, 8, 18, 32, 18, 8
120
S  Sulfur :
number of electrons per energy level 2, 8, 6
88Br Bromine :
number of electrons per energy level 2, 8, 18, 7
94Xe Xenon :
number of electrons per energy level 2, 8, 18, 18, 8
108  
Cl Chlorine :
number of electrons per energy level 2, 8, 7
79Kr Krypton :
number of electrons per energy level 2, 8, 18, 8
88Cs Caesium :
number of electrons per energy level 2, 8, 18, 18, 8, 1
298  
Ar Argon :
number of electrons per energy level 2, 8, 8
71Rb Rubidium :
number of electrons per energy level 2, 8, 18, 8, 1
265Ba Barium :
number of electrons per energy level 2, 8, 18, 18, 8, 2
253  
K  Potassium :
number of electrons per energy level 2, 8, 8, 1
243Sr Strontium :
number of electrons per energy level 2, 8, 18, 8, 2
219Lu Lutetium :
number of electrons per energy level 2, 8, 18, 32, 9, 2
217  

References

FAQ: All about atoms

What is an atom?

An atom is the smallest unit of matter that retains the properties of a chemical element. It consists of a central nucleus, made up of protons and neutrons, around which electrons orbit. The nucleus is dense and positively charged, while the negatively charged electrons occupy a much larger electron cloud. The typical size of an atom is of the order of a tenth of a nanometre (10-10 m).

What is the size of an atom?

The theoretical atomic radius varies according to the element. It is generally between 31 picometres (pm) for helium, the smallest atom, and about 298 pm for caesium, the largest natural atom. The atomic radius is defined as half the distance between the nuclei of two identical bonded atoms. These values depend on the measurement method (theoretical, covalent, metallic, etc.) and the chemical environment. By comparison, an atom is about 100,000 times smaller than a human hair.

How are atoms held together?

Within an atom, electrons are attracted to the nucleus via the electromagnetic force, which holds them in orbit. Inside the nucleus, protons and neutrons are bound by the strong nuclear force, much more powerful than the electrical repulsion between protons. Between atoms, chemical bonds (covalent, ionic or metallic) are formed by sharing or transferring electrons, enabling molecules and crystals to be built.

Why are atoms stable?

Atomic stability is a consequence of quantum mechanics. According to classical theory, an orbiting electron should radiate energy and crash into the nucleus. But the wave nature of the electron and the quantisation of energy levels impose that the electron can only occupy discrete states, without losing energy. The ground state is the most stable, and the atom cannot collapse because the electron is described by a wave function that distributes it in a probability cloud.

Can we see atoms?

Yes, thanks to instruments such as the scanning tunnelling microscope (STM) and the atomic force microscope (AFM). These devices do not work like optical microscopes, but use a very fine tip that scans the surface and measures interactions with atoms. The images obtained, such as the gold one shown in the article, show regular rows of individually resolved atoms. As early as 1990, IBM went even further by moving atoms one by one to form patterns. These technologies have revolutionised nanoscience.

How many atoms are there in the universe?

The total number of atoms in the observable universe is estimated at about 1080 (a 1 followed by 80 zeros). This value is obtained by multiplying the estimated number of stars (about 1023) by their average mass, converted to that of hydrogen atoms. This is a colossal number, but the universe is essentially empty, and ordinary matter (atoms) represents only a tiny fraction of its total content, most of which is dark matter and dark energy.

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