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Helium atomic number, mass, electron configuration and key properties

Helium’s chemical symbol, or abbreviation, is He. It is a colorless gas at ordinary room temperature and pressure; its state changes at cryogenic temperatures.

Atomic number
2
Relative atomic mass
4.002602
Electron configuration
1s²
Ordinary oxidation state
0
Gas density
0.000164 g/cm³
Normal boiling point
4.222 K
Freezing at 1 atm
Does not freeze
Ordinary elemental form
Monatomic gas
ClassificationNoble gas
Reference isotope⁴He
State contextColorless monatomic gas at 20 °C
Evidence noteAtomic and boiling-point values are measured/evaluated. The He I/He II transition is a measured condensed-matter phenomenon. The page explicitly preserves the fact that helium does not have a normal 1-atm freezing point.
Quick answers

Helium: quick answers

How many protons, neutrons and electrons does helium have?

Helium’s atomic number is 2, so every helium atom has 2 protons, and a neutral atom also has 2 electrons. Its most common natural isotope, helium-4, has 2 neutrons (other isotopes have different neutron counts).

What is the symbol for helium?

The chemical symbol for helium is He.

Is helium a solid, liquid or gas at room temperature?

Helium is a gas at room temperature (about 25 °C).

What family (group) is helium in?

Helium is a noble gas, in group 18, period 1 of the periodic table.

How many valence electrons does helium have?

Helium has 2 valence electrons, which fill its only shell, so it is grouped with the noble gases.

What is the electron configuration of helium?

The ground-state electron configuration of helium is 1s².

Connect the facts

From atomic number to chemistry

Read these as a chain of causes, not as isolated facts. Each step links to the concept hub if you want the underlying idea explained.

Common misconceptionHelium’s low boiling point does not mean it simply freezes at a lower temperature at 1 atm; solid helium requires elevated pressure.
Periodic-table position

Helium in its period and family

Helium sits in Group 18 because its only electron shell is filled. Unlike the other noble gases, its filled valence shell is 1s² rather than an ns²np⁶ octet.

Interactive Visual Lab

Helium Visual Lab

Decode helium’s tile, rotate a ⁴He teaching nucleus, inspect the spherical occupied 1s probability cloud, explore the ordinary-pressure cryogenic path through He I and superfluid He II, and connect helium to spectroscopy, natural-gas resources, MRI cooling and space science.

Overview · structure · orbitals · real world
How to read an element tile

Every mark points to one exact feature

12 24.002602 3He 41s² 5Helium 6Monatomic helium gas · ordinary-state model 7Gas
1Atomic numberNumber of protons
2Relative atomic massStandard value or bracketed reference mass
3Chemical symbolHe
4Electron configurationGround-state shorthand or evidence-labelled prediction
5Element nameHelium
6Structure contextMonatomic helium gas · ordinary-state model
7Physical-state contextColorless monatomic gas at 20 °C

The numbered markers explain the same information system used throughout Element Lookup. Unknown or predicted fields remain visibly labelled rather than being replaced with guesses.

Five things worth remembering

Helium in one minute

01

Atomic number 2 means every helium nucleus contains 2 protons.

02

Neutral helium has the closed-shell configuration 1s².

03

Helium boils at about 4.222 K at standard pressure.

04

Below about 2.17 K, liquid helium-4 enters the superfluid He II state.

05

Helium does not freeze at 1 atm merely by cooling; solid helium requires elevated pressure.

Atomic structure teaching model

⁴He nucleus · neutral He

2 p⁺ · 2 n⁰
Nucleus modelNucleon-count teaching view
2 p⁺ + 2 n⁰⁴He · schematic nucleus, not a literal nuclear geometry
Electron-count schematicPrincipal-shell populations

Shell rings organize electron counts. They are not electron trajectories or orbital shapes.

Nucleus, shell count and material structure are deliberately separated so one picture is not mistaken for another.
Connect picture → chemistry

2 electrons

n=12
Why this electron pattern matters

The 1s orbital is spherical and has no directional x/y/z variants. The probability cloud is an isolated-atom model; superfluidity is a collective quantum property of many helium atoms, not an orbital shape.

Teaching boundary: the nucleus uses colored spheres to make proton/neutron counts visible; the shell diagram only summarizes principal-shell populations. Neither is a literal picture of electron motion.
Material / molecular structure viewer

Monatomic helium gas · ordinary-state model

At ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.
Monatomic helium gas · ordinary-state modelAt ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.
What are you seeing?

At ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.. The viewer is evidence-aware: measured structures are identified as such; unknown bulk structures stay unknown.

Teaching visualization; not a literal finite sample or thermal trajectory.
Probability-cloud teaching model

1s orbital

One-electron teaching approximation; dots represent sampled probability density, not individual electrons.
Interpretation

What this model does—and does not—show

The 1s orbital is spherical and has no directional x/y/z variants. The probability cloud is an isolated-atom model; superfluidity is a collective quantum property of many helium atoms, not an orbital shape.

Important: The cloud includes the expected nodal pattern for the named nonrelativistic orbital where applicable. Phase colors are not electric charge. For heavy and superheavy elements, relativistic/many-electron effects make these only teaching approximations.
Real-world archive

Where do I meet helium?

Clickable learning cards connect the element to materials, environment, technology, biology or research - depending on what the evidence actually supports.

Cryo
Cryogenics

Cryogenics

Liquid helium cools superconducting magnets and experiments to temperatures only a few kelvin above absolute zero.

1868During a solar eclipse, spectroscopy revealed an unknown yellow line associated with the Sun; Norman Lockyer proposed a new solar element and named it helium.
1895William Ramsay isolated terrestrial helium from a uranium-bearing mineral, confirming helium on Earth.
1908Heike Kamerlingh Onnes liquefied helium, opening the door to ultralow-temperature physics.
1930sThe superfluid behavior of helium II became a landmark example of macroscopic quantum physics.
Evidence principleAtomic and boiling-point values are measured/evaluated. The He I/He II transition is a measured condensed-matter phenomenon. The page explicitly preserves the fact that helium does not have a normal 1-atm freezing point.
Signature science

Gas -> normal liquid -> superfluid, without a 1-atm solid

Helium’s phase story is unlike an ordinary solid-liquid-gas sequence.

Measured

Monatomic helium

Above about 4.22 K at ordinary pressure, helium is a monatomic gas.

Reference properties

Helium properties: atomic, physical, thermal and chemical

Categories follow the science of this element rather than a fixed decorative template. Each row carries condition/provenance context and an evidence label; unknown values stay unknown.

PropertyValueContext / provenanceEvidence
Atomic number2Source-reviewed; see Sources belowEvaluated
Relative atomic mass4.002602Source-reviewed; see Sources belowEvaluated
Ground-state electron configuration1s²Source-reviewed; see Sources belowEvaluated
Group / period / blockGroup 18 · Period 1 · s-blockPeriodic-table placementEvaluated
ElectronegativityNot assigned on the usual Pauling scaleSource-reviewed; see Sources belowEvaluated
Reference isotope⁴HeSource-reviewed; see Sources belowEvaluated
PropertyValueContext / provenanceEvidence
State contextColorless monatomic gas at 20 °CSource-reviewed; see Sources belowEvaluated
Density0.000164 g/cm³ · gas referenceSource-reviewed; see Sources belowEvaluated
Material / molecular structureMonatomic helium gas · ordinary-state modelAt ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.Measured
ClassificationNoble gasPeriodic-table / chemistry classificationEvaluated
Structure-model scopeAt ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.Teaching visualization; exact crystallographic coordinates are not implied unless stated.Reviewed
PropertyValueContext / provenanceEvidence
Melting / transition referenceNo freezing at 1 atm · solid requires pressureSource-reviewed; see Sources belowEvaluated
Boiling / gas reference4.222 KSource-reviewed; see Sources belowEvaluated
Phase-path contextIn the ordinary-pressure cryogenic teaching path, helium-4 is gaseous above about 4.222 K, liquid He I below the boiling point, and becomes superfluid He II below about 2.17 K. It does not form an ordinary solid at 1 atm; solid helium requires elevated pressure.Shared phase registry drives the slider, regions and markers.Evaluated
Condition warningTemperature and pressure define phase behavior; purity/allotropy may matter.Teaching condition statementReviewed
PropertyValueContext / provenanceEvidence
Common oxidation states0 in ordinary chemistrySource-reviewed; see Sources belowEvaluated
Ion / common ion contextNo common stable ionSource-reviewed; see Sources belowEvaluated
Periodic chemistry contextHelium sits in Group 18 because its only electron shell is filled. Unlike the other noble gases, its filled valence shell is 1s² rather than an ns²np⁶ octet.Element-specific interpretationReviewed
Chemistry cautionElemental form, ions and compounds are distinct chemical objects.Interpretive teaching ruleReviewed
PropertyValueContext / provenanceEvidence
⁴HeStable · overwhelmingly dominant natural heliumTeaching nucleus contains 2 protons and 2 neutrons; the ⁴He nucleus is also an alpha particle.Evaluated
³HeStable · trace natural isotopeImportant in low-temperature physics, neutron detection and specialized research.Evaluated
Helium isotope mixtureTwo stable isotopesThe abundance of ³He is tiny compared with ⁴He, but its quantum properties are profoundly different.Evaluated
Teaching nucleus⁴He · 2 protons + 2 neutronsReference isotope used in the nucleus modelReviewed
PropertyValueContext / provenanceEvidence
Page evidence noteAtomic and boiling-point values are measured/evaluated. The He I/He II transition is a measured condensed-matter phenomenon. The page explicitly preserves the fact that helium does not have a normal 1-atm freezing point.Evidence summary for this guideReviewed
Structure evidenceAt ordinary conditions helium is a monatomic gas. At 1 atm it does not freeze on cooling; solid helium requires elevated pressure, so the ordinary-pressure viewer does not invent a solid crystal.Measured structure, labelled schematic, prediction or explicit unknown as applicable.Reviewed
Map evidence ruleReal pins are reviewed examples; conceptual layers are used when pins would mislead.Geography Explorer 2.0Reviewed
Source set3 primary/reference links listed belowOpen the Sources section for the actual references.Reviewed
Temperature explorer

Is Helium a solid, liquid or gas? State at temperature

In the ordinary-pressure cryogenic teaching path, helium-4 is gaseous above about 4.222 K, liquid He I below the boiling point, and becomes superfluid He II below about 2.17 K. It does not form an ordinary solid at 1 atm; solid helium requires elevated pressure.

Temperature293 K
Move the slider
The shared site-wide phase model controls the track, markers and readout.
Geography and evidence

Where on Earth is Helium found or produced?

World map
Solar spectrum + terrestrial isolationRSC historical context · 1868-1895
Discovery and history

Who discovered Helium, and when?

1868

During a solar eclipse, spectroscopy revealed an unknown yellow line associated with the Sun; Norman Lockyer proposed a new solar element and named it helium.

1895

William Ramsay isolated terrestrial helium from a uranium-bearing mineral, confirming helium on Earth.

1908

Heike Kamerlingh Onnes liquefied helium, opening the door to ultralow-temperature physics.

1930s

The superfluid behavior of helium II became a landmark example of macroscopic quantum physics.

Process / synthesis context

From helium-bearing gas to cryogenic use: a high-level path

1

Commercial helium is commonly recovered from natural-gas streams that contain unusually high helium concentrations.

2

Gas processing separates major components before cryogenic purification concentrates helium; detailed plant-operation guidance is outside this page.

3

Purified helium is distributed for cryogenics, leak detection, controlled atmospheres and specialized industrial/scientific uses.

4

In high-value systems, recovery and reliquefaction can reduce losses of this finite terrestrial resource.

Real-world applications

What is helium used for?

Cryogenic cooling

Helium enables temperatures low enough for superconducting magnets and condensed-matter experiments.

Leak detection

Helium tracer methods can reveal very small leaks in vacuum and pressure systems.

Shielding / inert atmospheres

Helium can provide inert gas environments for selected manufacturing processes.

Aerospace

Low density and inertness support pressurization and purge roles in specialized aerospace systems.

Isotopes

Helium isotopes and natural abundance

⁴He

Stable · overwhelmingly dominant natural helium

Teaching nucleus contains 2 protons and 2 neutrons; the ⁴He nucleus is also an alpha particle.

³He

Stable · trace natural isotope

Important in low-temperature physics, neutron detection and specialized research.

Helium isotope mixture

Two stable isotopes

The abundance of ³He is tiny compared with ⁴He, but its quantum properties are profoundly different.

Learn it, don’t just read it

Five-question Helium check

What is helium’s atomic number?

What is helium’s ground-state electron configuration?

What happens to helium-4 below about 2.17 K?

Can helium freeze at 1 atm by cooling alone?

What is ordinary gaseous helium made of?

Questions answered

Helium questions students commonly ask

Each answer starts with the direct fact, then explains the chemistry, evidence or material context so the result is understandable rather than merely memorized.

What is helium’s atomic number?

Short answer: 2.

Atomic number is defined by proton count, so 2 protons are what make an atom helium. A neutral helium atom also has 2 electrons, while isotopes can have different neutron counts without changing the element.

Key point: Atomic number = proton count.

What is helium’s symbol?

Short answer: He.

The symbol He is the standardized chemical abbreviation for element 2. In a chemical formula, He identifies helium atoms; a compound containing He is not automatically the same material as elemental helium.

Key point: He always identifies element 2.

Why is helium a noble gas?

Short answer: Helium is placed in Group 18 because its 1s shell is completely filled (1s²) and it is extraordinarily unreactive under ordinary conditions.

Helium is a useful exception to the classroom “octet” shortcut: its only occupied shell is the first shell, which is complete with two electrons. That closed 1s² configuration is energetically stable and helium has a very high ionization energy. Helium is chemically grouped with the noble gases even though, by electron-configuration block, it is an s-block element.

Key point: Noble-gas behavior comes from a filled valence shell; helium has a filled duet, not an octet.

What is helium used for?

Short answer: Major uses include cryogenic cooling, leak detection, inert atmospheres and specialized aerospace/scientific applications.

Cryogenic cooling: Helium enables temperatures low enough for superconducting magnets and condensed-matter experiments. Leak detection: Helium tracer methods can reveal very small leaks in vacuum and pressure systems. Helium’s famous balloons are only one part of the story. The deeper physics lies near 4 K, where quantum behavior becomes macroscopic in liquid helium.

Key point: Always distinguish the pure element from the compound, alloy, isotope or device material that actually performs the application.

Can helium freeze at 1 atmosphere?

Short answer: No. Helium remains liquid down to very low temperature at 1 atm; forming solid helium requires added pressure.

In the ordinary-pressure cryogenic teaching path, helium-4 is gaseous above about 4.222 K, liquid He I below the boiling point, and becomes superfluid He II below about 2.17 K. It does not form an ordinary solid at 1 atm; solid helium requires elevated pressure.

Key point: Phase statements need temperature, pressure and evidence context.

What is superfluid helium?

Short answer: Below the lambda transition near 2.17 K, liquid helium-4 enters He II, a quantum fluid with extraordinary flow and heat-transport behavior.

Helium is element 2, a closed-shell noble gas with the lowest normal boiling point of any element. Its signature science is cryogenic: liquid helium becomes superfluid below the lambda transition, while solid helium requires pressure rather than simple cooling at 1 atm. Below about 2.17 K, liquid helium-4 enters the superfluid He II state.

Key point: The mechanism matters: connect the observed behavior to electron structure, bonding, phase or the specific material form rather than memorizing the result alone.

Is helium flammable?

Short answer: No. Helium is a nonflammable noble gas. Its main hazards are physical, such as displacement of oxygen in confined spaces and extreme cold when liquefied.

Helium sits in Group 18 because its only electron shell is filled. Unlike the other noble gases, its filled valence shell is 1s² rather than an ns²np⁶ octet. Helium is element 2, a closed-shell noble gas with the lowest normal boiling point of any element. Its signature science is cryogenic: liquid helium becomes superfluid below the lambda transition, while solid helium requires pressure rather than simple cooling at 1 atm.

Key point: The mechanism matters: connect the observed behavior to electron structure, bonding, phase or the specific material form rather than memorizing the result alone.

Scientific sources and provenance

Scientific sources for Helium

Evidence rule: Atomic and boiling-point values are measured/evaluated. The He I/He II transition is a measured condensed-matter phenomenon. The page explicitly preserves the fact that helium does not have a normal 1-atm freezing point.
Keep the curiosity going

Questions to ask next about Helium

A good element lesson should lead to the next useful question, not end after a list of facts.

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