Schwarzschild Radius Calculator
Enter an object's mass to compute its Schwarzschild radius — the event horizon size if that mass were compressed into a black hole.
Mass Input
Scientific notation supported (e.g. 1.5e30)
Formula
rs = 2GM / c²
G = 6.67430×10⁻¹¹ m³ kg⁻¹ s⁻²
c = 2.99792458×10⁸ m/s
Select a preset or enter a mass to see the event horizon size.
Schwarzschild Radius
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Meters (m)
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Kilometers (km)
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Light-years (ly)
Density Required to Form a Black Hole
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kg/m³
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× nuclear density
Nuclear density ≈ 2.3×10¹⁷ kg/m³. Values below 1× are less dense than a nucleus.
Scale Comparison
| Reference | Size | vs rs |
|---|
Input: — · rs = 2 × 6.67430×10⁻¹¹ × M / (2.998×10⁸)²
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Summary
Enter an object's mass to compute its Schwarzschild radius — the event horizon size if that mass were compressed into a black hole.
How it works
- Select your mass input unit (kilograms, solar masses, Earth masses, or a preset object).
- Enter the mass value in the input field.
- The calculator applies r = 2GM/c² using G = 6.674×10⁻¹¹ N·m²/kg² and c = 2.998×10⁸ m/s.
- The Schwarzschild radius is displayed in meters, kilometers, and light-years.
- A comparison table shows the result relative to familiar objects like atoms, protons, and the observable universe.
Use cases
- Verify textbook examples in general relativity and astrophysics courses.
- Compare the event horizon sizes of stellar-mass vs. supermassive black holes.
- Illustrate how compressed everyday objects (Earth, Sun) would need to be to form black holes.
- Explore the extreme density required for quantum-gravity thought experiments.
- Support astronomy outreach and science communication projects.
Frequently Asked Questions
Last updated: 2026-07-23 ·
Reviewed by Nham Vu