Schwarzschild Radius Calculator
Find how small a mass must be squeezed to become a black hole.
Result
How it is calculated
The Schwarzschild radius of a non-rotating, uncharged mass is Rs = 2GM / c², where M is the mass in kilograms, G = 6.6743×10⁻¹¹ m³ kg⁻¹ s⁻² and c = 299,792,458 m/s. The mass can be entered in kilograms, solar masses (1.98892×10³⁰ kg) or Earth masses (5.972×10²⁴ kg); the tool converts it to kilograms first. The radius is shown in metres (two decimals) and in kilometres (four decimals). The radius grows in direct proportion to the mass, so ten times the mass gives ten times the radius. The mass must be above zero. An unrecognised unit is treated as solar masses.
Worked example
Mass 10 solar masses. In kilograms: 10 × 1.98892×10³⁰ = 1.98892×10³¹ kg. Then 2 × 6.6743×10⁻¹¹ × 1.98892×10³¹ ÷ (299,792,458)² ≈ 29,540.08. The radius is 29,540.08 m, or 29.5401 km. A black hole of ten Suns would have an event horizon about 30 km in radius.
Common mistakes
- Selecting the wrong unit, such as typing 1 for the mass but leaving kg selected. One kilogram has a radius of about 10⁻²⁷ m, which rounds to 0.00 m, while one solar mass gives nearly 3 km.
- Reading the radius as the size of an existing star. It is only the radius an object would have if squeezed into a black hole; the Sun is far larger than its own Schwarzschild radius.
- Confusing the radius with the diameter. The result is the radius; the horizon's diameter is twice as large.
- Using it for a spinning or charged black hole. This formula covers only the non-rotating, uncharged case.
- Expecting a result for Earth in kilometres. Earth gives about 0.01 m, which shows as 0.0000 km, so read the metre value.
About this calculator
This calculator computes the Schwarzschild radius: Rs = 2GM/c², the radius to which any mass must be compressed for its escape velocity to reach the speed of light, forming an event horizon beyond which nothing — not even light — can escape.
Astrophysics students and enthusiasts use it to see how extreme the compression required for black hole formation really is — squeezing Earth's mass into about 9 millimeters, or the Sun's into about 3 kilometers.
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Comments (1)
A useful second step is to set the radius next to the object's real size. A neutron star of 1.4 solar masses has a Schwarzschild radius of about 4.1 km, while such stars measure roughly 10 to 12 km across, so they sit close to the limit without crossing it. The ratio of the two is a rough measure of how compact something is. Which object would you like to test against its real radius?