helium-4

E761917

Helium-4 is the most common stable isotope of helium, consisting of two protons and two neutrons, and is a key product of both Big Bang nucleosynthesis and stellar fusion.

All labels observed (1)

Label Occurrences
helium-4 canonical 1

How this entity was disambiguated

Statements (50)

Predicate Object
instanceOf alpha particle ⓘ
boson ⓘ
helium isotope ⓘ
nucleus ⓘ
stable isotope ⓘ
atomicNumber 2 ⓘ
bindingEnergyPerNucleon ≈7.07 MeV ⓘ
boilingPointAt1atm ≈4.22 K ⓘ
bosonicStatistics Bose–Einstein ⓘ
charge +2e (nucleus) ⓘ
chemicalElement helium ⓘ
cosmologicalMassFraction ≈0.24–0.25 of baryonic matter ⓘ
discoveredAsAlphaParticleBy Ernest Rutherford ⓘ
dominantIsotopeOf helium ⓘ
electricCharge +2 elementary charges ⓘ
firstIonizationEnergy same as helium ≈24.6 eV ⓘ
formationProcess Big Bang nucleosynthesis ⓘ
alpha decay of heavier nuclei ⓘ
stellar hydrogen fusion ⓘ
formsSuperfluidPhase true ⓘ
isAlphaParticle true ⓘ
isMagicNucleus true ⓘ
isStable true ⓘ
magicNeutronNumber 2 ⓘ
magicProtonNumber 2 ⓘ
mass ≈4.002602 u ⓘ
≈6.6465×10^-27 kg ⓘ
massNumber 4 ⓘ
meltingPointAt1atm doesNotMelt (solidifies only under pressure) ⓘ
naturalAbundanceInHelium >0.99 ⓘ
neutronNumber 2 ⓘ
neutronSeparationEnergy high ⓘ
nuclearSpin 0 ⓘ
nucleonNumber 4 ⓘ
occursIn Sun ⓘ
interstellar medium ⓘ
main-sequence stars ⓘ
productOf CNO cycle ⓘ
proton–proton chain reaction ⓘ
protonNumber 2 ⓘ
protonSeparationEnergy high ⓘ
radioactive false ⓘ
roleInCosmology key probe of Big Bang nucleosynthesis ⓘ
superfluidTransitionTemperature ≈2.17 K (lambda point) ⓘ
symbol 4He ⓘ
totalBindingEnergy ≈28.3 MeV ⓘ
usedAs carrier gas in some analytical instruments ⓘ
coolant for superconducting magnets ⓘ
cryogenic coolant ⓘ
working fluid in low-temperature physics experiments ⓘ

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.