PhysicsNuclear PhysicsMedium

Alpha Decay

Also known as:α-decayAlpha emission

Alpha decay is a type of radioactive decay in which an unstable nucleus emits an alpha particle — a helium-4 nucleus consisting of two protons and two neutrons — thereby reducing its atomic number by 2 and its mass number by 4. This process is common in heavy nuclei (Z > 82) such as uranium and radium, where the nuclear repulsion between protons becomes too great to maintain stability. Alpha particles have low penetrating power and can be stopped by a sheet of paper, but are highly ionising and dangerous if ingested or inhaled.

Key Formula

A_Z X → (A-4)_(Z-2) Y + 4_2 He

LaTeX: {}^{A}_{Z}X \rightarrow {}^{A-4}_{Z-2}Y + {}^{4}_{2}He

SymbolMeaningUnit
AMass number of parent nucleusdimensionless
ZAtomic number of parent nucleusdimensionless
XParent nuclide symbol
YDaughter nuclide symbol
⁴₂HeAlpha particle (helium-4 nucleus)

Worked Example

Problem

Uranium-238 (⁲³⁸₉₂U) undergoes alpha decay. Write the decay equation and identify the daughter nuclide.

Solution

Step 1: Apply conservation of mass number: A_daughter = 238 − 4 = 234. Step 2: Apply conservation of atomic number: Z_daughter = 92 − 2 = 90. Step 3: Element with Z = 90 is Thorium (Th). Step 4: Write the equation: ²³⁸₉₂U → ²³⁴₉₀Th + ⁴₂He.

Answer

The daughter nuclide is Thorium-234 (²³⁴₉₀Th).

Properties of Alpha Particles vs Other Radiation Types

PropertyAlpha (α)Beta (β)Gamma (γ)
CompositionHe-4 nucleus (2p + 2n)Electron or positronHigh-energy photon
Charge+2e±e0
Mass (u)4.00150.0005490
Penetrating powerVery low (cm air)Low (mm Al)High (cm Pb)
Ionising abilityVery highModerateLow
Stopped byPaper / skinAluminium sheetLead / thick concrete

Interactive Tools

PhET Nuclear Decay Simulator

Visualise alpha decay step by step with interactive nucleus models

Open Tool

Khan Academy: Alpha Decay

Structured lessons on writing and balancing alpha decay equations

Open Tool

NIST Nuclear Data

Official reference data for nuclide properties and decay modes

Open Tool
Diagram illustrating alpha decay showing the parent nucleus emitting a helium-4 alpha particle

Wikimedia Commons, CC BY-SA

Related Terms

Physics

Radioactive Decay

Radioactive decay is the spontaneous transformation of an unstable atomic nucleus into a more stable configuration by emitting radiation in the form of particles or electromagnetic waves. This process occurs because the nucleus has too many protons, too many neutrons, or excess energy, making it thermodynamically unstable. It is the foundation of nuclear medicine, radiometric dating, and nuclear power generation.

Physics

Beta Decay

Beta decay is a type of radioactive decay mediated by the weak nuclear force, in which a neutron converts to a proton (beta-minus decay, emitting an electron and an antineutrino) or a proton converts to a neutron (beta-plus decay, emitting a positron and a neutrino). Unlike alpha decay, the mass number of the nucleus remains unchanged, but the atomic number increases or decreases by one. Beta decay is responsible for the natural transmutation of elements and is exploited in positron emission tomography (PET scanning) and food irradiation.

Physics

Nuclear Binding Energy

Nuclear binding energy is the energy required to completely separate a nucleus into its individual protons and neutrons, or equivalently, the energy released when these nucleons combine to form the nucleus. It arises from the strong nuclear force overcoming electromagnetic repulsion between protons, and is directly related to the mass defect — the difference between the mass of the nucleus and the sum of masses of its constituent nucleons via Einstein's E = mc². The binding energy per nucleon peaks around iron-56, explaining why both fusion of light nuclei and fission of heavy nuclei can release energy.

Named "alpha" by Ernest Rutherford in 1899 using the first letter of the Greek alphabet (α), as it was the first type of radiation he identified. Rutherford later established that alpha particles are helium-4 nuclei through spectroscopic analysis in 1909.

alphadecaynuclearheliumradiationheavy-nuclei