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  4. /Bohr Radius Calculator

Bohr Radius Calculator

Last updated: April 5, 2026

The Bohr Radius Calculator computes the orbital radius of an electron in any hydrogen-like atom at any principal quantum number using rₙ = a₀ × n²/Z, where a₀ = 0.529 Å. The Bohr radius is the fundamental unit of atomic length in quantum chemistry — the natural scale of the atom.

Calculator

Results

Bohr Radius Constant

0.000000000053

m

Orbital Radius

0.000000000053

m

Orbital Radius

52.9177

pm

Orbital Radius

0.529177

Å

Energy of Level n

-13.605693

eV

Electron Velocity Ratio

0.00729735

Orbital Diameter

105.8354

pm

Results

Bohr Radius Constant

0.000000000053

m

Orbital Radius

0.000000000053

m

Orbital Radius

52.9177

pm

Orbital Radius

0.529177

Å

Energy of Level n

-13.605693

eV

Electron Velocity Ratio

0.00729735

Orbital Diameter

105.8354

pm

In This Guide

  1. 01Bohr Radius Formula
  2. 02Physical Meaning of the Bohr Radius
  3. 03Comparison to Modern Quantum Mechanical Orbitals

The Bohr radius (a₀ = 5.291 × 10⁻¹¹ m = 0.529 Å) is the most probable distance between the proton and electron in a ground-state hydrogen atom — the natural length scale of the atom. Every other orbital radius in the hydrogen series scales from this value: the n=2 orbit is 4 times larger; n=3 is 9 times larger; the orbit expands as n². The Bohr radius calculator computes any orbital radius for hydrogen-like atoms at any quantum level.

Bohr Radius Formula

rₙ = a₀ × n² / Z

where a₀ = 0.529177 Å = 5.29177 × 10⁻¹¹ m (the Bohr radius constant), n = principal quantum number, Z = atomic number of the nucleus.

Examples for hydrogen (Z=1): r₁ = 0.529 Å; r₂ = 0.529 × 4 = 2.116 Å; r₃ = 0.529 × 9 = 4.762 Å; r₄ = 0.529 × 16 = 8.466 Å. For He⁺ (Z=2, n=1): r₁ = 0.529/2 = 0.265 Å — half the hydrogen radius because the stronger nuclear charge pulls the electron closer. Use this online calculator for any combination. The Bohr model calculator computes energy levels and spectral wavelengths from the same atomic model.

Physical Meaning of the Bohr Radius

In classical mechanics, the Bohr radius represents the exact orbital radius where the electrostatic attraction equals the centripetal force needed for circular orbital motion. In quantum mechanics, it represents the distance from the nucleus at which the 1s electron probability density is maximum — the most likely location to find the electron. The Bohr radius is a natural unit in atomic physics: measuring distances in units of a₀ (atomic units) simplifies equations by eliminating physical constants. At larger scales: a hydrogen atom (n=1) has radius ≈ 1 Å; a Rydberg atom at n=100 has radius ≈ 0.529 × 10,000 Å = 529 nm — roughly the size of a visible light wavelength.

Comparison to Modern Quantum Mechanical Orbitals

The Bohr model predicts fixed orbital radii; quantum mechanics predicts probability distributions (orbitals). Despite this conceptual difference: the most probable radius of the quantum mechanical 1s orbital of hydrogen exactly equals the Bohr radius (0.529 Å); the average radius of the 1s orbital is 1.5 × a₀ (slightly larger due to the asymmetric probability distribution); Bohr radii provide accurate estimates for highly excited (Rydberg) states where the quantum number is large and the classical approximation improves. The physical constants calculators provide complementary atomic unit tools.

Visual Analysis

How It Works

Enter principal quantum number n (1, 2, 3, ...) and atomic number Z (1 for hydrogen, 2 for He⁺, 3 for Li²⁺, etc.). Orbital radius rₙ = a₀ × n²/Z where a₀ = 0.529177 Å = 5.29177 × 10⁻¹¹ m. Result displayed in Å, pm, nm, and meters. Also shows the orbit's energy Eₙ = −13.6 × Z²/n² eV.

Understanding Your Results

The orbital radius gives the Bohr model's predicted distance of the electron from the nucleus, displayed in meters, picometers, and angstroms. The energy is the total (kinetic + potential) energy of the orbital, with negative values indicating a bound state. The velocity ratio v/c indicates how relativistic the electron is — when this exceeds ~0.1, relativistic corrections become important and the simple Bohr model loses accuracy.

Worked Examples

Hydrogen Ground State

Inputs

n1
Z1

Results

a05.292e-11
orbital radius m5.292e-11
orbital radius pm52.92
orbital radius angstrom0.5292
energy eV-13.6057
velocity ratio0.0072974

The hydrogen ground state has radius a₀ = 52.9 pm, energy -13.6 eV, and electron speed of c/137. This is the fundamental reference point for all atomic physics.

He⁺ Ground State

Inputs

n1
Z2

Results

a05.292e-11
orbital radius m2.646e-11
orbital radius pm26.46
orbital radius angstrom0.2646
energy eV-54.4228
velocity ratio0.0145947

He⁺ (Z = 2) has half the radius (26.5 pm), four times the binding energy (54.4 eV), and twice the electron velocity compared to hydrogen. This is the simplest ion after hydrogen.

Frequently Asked Questions

The Bohr radius (symbol a₀) is the most probable distance between the proton and electron in a ground-state hydrogen atom — 5.292 × 10⁻¹¹ meters (0.529 Å or 52.9 pm). It is the natural length scale of atomic physics and one of the fundamental physical constants, derived from: a₀ = ℏ²/(m_e × e² × k_e) where ℏ is the reduced Planck constant, m_e is the electron mass, e is the electron charge, and k_e is Coulomb's constant. The Bohr radius defines the scale of atoms — all atomic and molecular bond lengths are on the order of 1–5 Bohr radii. It is used as a unit of length ('atomic unit of length') in quantum chemistry calculations.
Orbital radius scales as n² for hydrogen: r₁ = 0.529 Å; r₂ = 2.116 Å (4×); r₃ = 4.762 Å (9×); r₄ = 8.466 Å (16×); r₅ = 13.23 Å (25×). The quadratic scaling means that excited states can be much larger than the ground state — a hydrogen atom in the n=10 state has an orbital radius of 52.9 Å (100× the ground state), and a Rydberg atom at n=100 has a radius of 52,900 Å (5.29 micrometers) — roughly the size of a small bacterium. For hydrogen-like ions with atomic number Z, the radius is divided by Z: He⁺ (Z=2) at n=1 has radius 0.265 Å; Li²⁺ (Z=3) at n=1 has radius 0.176 Å.
The Bohr radius (0.529 Å) represents the most probable electron-nucleus distance in ground-state hydrogen. It sets the length scale for all atoms. Atomic radii in chemistry are typically 0.5–3 Å — all within a few Bohr radii of the nucleus. The covalent radius of hydrogen is approximately 0.31 Å (slightly smaller than the Bohr radius because covalent bonding contracts the electron cloud). The van der Waals radius of hydrogen is 1.2 Å (the effective size for non-bonded contacts). For multi-electron atoms, the innermost electrons are closest to the nucleus (inner shell at approximately 1 Bohr radius × 1/Z), while valence electrons are at larger distances. The Bohr model accurately predicts inner-shell radii in multi-electron atoms using hydrogen-like formulas with effective nuclear charge.
The Bohr radius is derived by balancing the electrostatic attraction force with the centripetal force for circular orbit, combined with the quantization condition that angular momentum is an integer multiple of ℏ. For an electron at radius r orbiting a proton: electrostatic force = k_e × e²/r²; centripetal force = m_e × v²/r. Setting these equal and applying the quantization mvr = nℏ yields: rₙ = a₀ × n², where a₀ = ℏ²/(m_e × k_e × e²) = 5.292 × 10⁻¹¹ m. This derivation is a cornerstone of quantum mechanics pedagogy because it illustrates how quantization of angular momentum naturally leads to discrete energy levels and orbital radii.
Rydberg atoms are atoms with electrons excited to very high principal quantum numbers (n = 50–300 or higher). Their properties scale dramatically with n: orbital radius scales as n² (Rydberg atoms can be micrometers in size — far larger than ordinary atoms); energy spacing between levels scales as n⁻³ (levels become very close together, making transitions easily driven by microwave photons); lifetime scales as n³ (Rydberg states can persist for milliseconds vs. nanoseconds for low-n excited states). Rydberg atoms are important in: quantum computing (long coherence times; strong dipole-dipole interactions for entanglement); precision spectroscopy (level spacings allow extremely accurate measurements of fundamental constants); astrophysics (Rydberg transitions produce radio-frequency emission in the interstellar medium).
For hydrogen-like ions (one electron), the ground-state orbital radius is rₙ = a₀/Z, where Z is the nuclear charge. He⁺ (Z=2): r₁ = 0.265 Å; Li²⁺ (Z=3): r₁ = 0.176 Å; C⁵⁺ (Z=6): r₁ = 0.088 Å. The orbit contracts because stronger nuclear charge pulls the electron closer. For multi-electron atoms, the concept of an 'effective Bohr radius' uses Z_eff (effective nuclear charge after screening by other electrons). The ground-state 1s orbital in helium has a mean radius of approximately 0.33 Å (between the Z=1 and Z=2 hydrogen-like values) because each electron partially screens the nuclear charge felt by the other. Slater's rules provide a systematic way to estimate Z_eff for any electron in any atom.

Sources & Methodology

Bohr, N. (1913). On the Constitution of Atoms and Molecules. Philosophical Magazine, 26. NIST CODATA (2018). Bohr radius: a₀ = 5.29177210903 × 10⁻¹¹ m. Griffiths, D.J. (2018). Introduction to Quantum Mechanics, 3rd ed.

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