Reduced Mass Calculator

Calculate reduced mass μ = m₁m₂/(m₁+m₂) for two or three bodies. Supports kg, amu, electron masses with reference table of common systems.

Reduced Mass (μ)
7.2528e+22
4.3678e+49 amu
μ / m₁
1.2145
Fraction of m₁
μ / m₂
98.7855
Fraction of m₂
Total Mass
6.0454e+24
m₁ + m₂ = 3.6406e+51 amu
Mass Ratio
81.3402
m₁/m₂ = 81.3402
If Masses Equal
2.9860e+24
μ = m/2 for equal masses

Reduced Mass Compared to Individual Masses

m₁
5.972e+24 kg
m₂
7.342e+22 kg
μ
7.253e+22 kg
Systemm₁m₂μμ/m_lighter
Proton–Electron1.673e-279.109e-319.104e-3199.95%
H₂ molecule1.674e-271.674e-278.368e-2850.00%
CO molecule1.994e-262.657e-261.139e-2657.12%
Earth–Moon5.972e+247.342e+227.253e+2298.79%
Sun–Earth1.989e+305.972e+245.972e+24100.00%
Planning notes, formulas, and examples

About the Reduced Mass Calculator

The reduced mass μ = m₁m₂/(m₁+m₂) converts a two-body problem into an equivalent one-body problem. It appears throughout physics, from orbital mechanics and molecular spectroscopy to atomic physics and nuclear scattering.

This calculator handles masses from electrons to stars with six unit options: kg, grams, atomic mass units (amu), pounds, electron masses, and proton masses. For three-body systems, it performs sequential reduction: μ₁₂₃ = (μ₁₂ × m₃)/(μ₁₂ + m₃).

Results include the reduced mass, its percentage of each input mass, total mass, mass ratio, and a visual comparison bar chart. The reference table shows several classic systems and how the reduced mass shifts toward the lighter body when the mass ratio is extreme.

When This Page Helps

Reduced mass is a compact way to reason about relative motion without carrying both bodies through every equation. That matters in problems where one mass is much larger than the other, or where the same relationship keeps showing up in different fields.

The unit conversion support, 3-body extension, and mass-ratio display make it easier to check the numbers and see why the lighter body often dominates the result.

How to Use the Inputs

  1. Select a preset or enter masses manually.
  2. Choose the mass unit (kg, g, amu, lb, electron masses, or proton masses).
  3. Enter m₁ and m₂ (scientific notation accepted, e.g. 5.972e24).
  4. For 3-body problems, switch to "3 bodies" and enter m₃.
  5. View reduced mass, mass ratios, and the comparison bar chart.
Formula used
Reduced mass: μ = m₁m₂/(m₁+m₂) = m₁/(1 + m₁/m₂). For equal masses: μ = m/2. For m₂ >> m₁: μ ≈ m₁. Three-body reduction: μ₁₂₃ = (μ₁₂ × m₃)/(μ₁₂ + m₃).

Example Calculation

Result: μ = 7.253 × 10²² kg

μ = (5.972e24 × 7.342e22) / (5.972e24 + 7.342e22) = 7.253 × 10²² kg ≈ 98.8% of Moon's mass, since Earth is ~81× heavier.

Tips & Best Practices

  • For diatomic molecules, use amu units: H-Cl has μ = 1×35/(1+35) = 0.972 amu.
  • The reduced mass is always ≤ the lighter mass. If your result exceeds either input, check for errors.
  • For hydrogen energy levels, the reduced mass correction shifts the Rydberg constant by about 0.05%.
  • In nuclear physics, reduced mass determines the kinetic energy available for reactions in the center-of-mass frame.
  • Equal masses give μ = m/2, the maximum reduced mass relative to total mass (50%).

Reduced Mass in Different Fields

| Field | Application | Typical μ | |---|---|---| | Atomic physics | Hydrogen energy levels | 0.9995 × m_e | | Molecular spectroscopy | IR vibrational frequencies | 1–20 amu | | Nuclear physics | Scattering cross-sections | ~1 amu | | Orbital mechanics | Two-body orbit calculations | ≈ lighter body | | Gravitational waves | Inspiral chirp mass | 1–50 M_☉ |

Key Relationships

The reduced mass connects to the center of mass (CM) frame: - Total mass: M = m₁ + m₂ - CM velocity: v_CM = (m₁v₁ + m₂v₂)/M - Relative velocity: v_rel = v₁ − v₂ - Kinetic energy in CM frame: KE_rel = ½μv_rel² - Angular momentum in CM frame: L = μ × r × v_rel

The chirp mass in gravitational wave astronomy is: M_chirp = (m₁m₂)^(3/5) / (m₁+m₂)^(1/5) = μ^(3/5) × M^(2/5).

Sources & Methodology

Last updated:

Frequently Asked Questions

  • It simplifies two-body problems: instead of tracking two particles, we solve for one particle of mass μ in the relative coordinate. The mathematics is identical to a one-body problem.