Black Hole Event Horizon Calculator
Calculate Schwarzschild radius, event horizon, ergosphere, Hawking temperature, and black hole parameters.
About this calculator
This calculator applies the Kerr metric -- the exact general-relativistic solution for a rotating, uncharged black hole -- which reduces to the simpler Schwarzschild solution when Spin Parameter is 0. Schwarzschild Radius follows r_s = 2GM/c^2, the boundary of a non-rotating hole where the escape velocity reaches the speed of light; it depends on Black Hole Mass alone and does not respond to Spin Parameter at all. Event Horizon Radius is the Kerr outer horizon, r+ = GM/c^2 + sqrt((GM/c^2)^2 - a^2(GM/c^2)^2), where a is Spin Parameter (0 = non-rotating, up to 0.99 = nearly maximally spinning); raising Spin Parameter always SHRINKS Event Horizon Radius toward GM/c^2 -- half the Schwarzschild value -- because frame-dragging around a spinning hole lets the horizon retreat closer to the singularity while still trapping light.
Ergosphere Radius reports the EQUATORIAL boundary of the ergosphere, the region outside the horizon where spacetime itself is dragged around fast enough that nothing can stay still relative to distant stars. A well-known and directly derivable fact about the Kerr metric: at the equator this boundary sits at exactly 2GM/c^2 -- identical to the Schwarzschild Radius -- for every spin value, so Ergosphere Radius does not move when Spin Parameter changes (the ergosphere narrows toward the horizon only near the poles, a variation this calculator does not compute). Hawking Temperature and Hawking Lifetime both use Black Hole Mass alone, since Hawking's original non-rotating derivation used here has no spin dependence -- real stellar-mass and supermassive black holes are far colder than the 2.7 K cosmic microwave background and will not evaporate for timescales vastly longer than the current age of the universe.
Inputs
Results
Schwarzschild Radius
2,954.127 m
≈ 9 Eiffel Towers
Event Horizon Radius
2,756.238 m
≈ 8 Eiffel Towers
Hawking Temperature
0.000000062 K
Hawking Lifetime
20,973,585,980,140,658,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000 years
How to Use This Calculator
- Enter the Black Hole Mass in solar masses — stellar black holes are 3–100 M☉, supermassive ones are millions to billions.
- Set the Spin Parameter (0–0.99): 0 is a non-rotating Schwarzschild black hole; values near 1 are maximally spinning Kerr black holes.
- Read the Schwarzschild Radius (m) and Event Horizon Radius (m) — for a spinning hole these differ due to frame-dragging.
- Note the Hawking Temperature (K) — stellar-mass black holes are effectively at absolute zero; only micro black holes radiate detectably.
- Use Hawking Lifetime (years) to understand evaporation timescale — a solar-mass black hole evaporates over ~10⁶⁷ years.
How the result changes with Black Hole Mass
| Black Hole Mass | Schwarzschild Radius | Event Horizon Radius | Hawking Temperature |
|---|---|---|---|
| 0.5 | 1,477.063 m | 1,378.119 m | 0.000000123 K |
| 0.75 | 2,215.595 m | 2,067.178 m | 0.000000082 K |
| 1.5 | 4,431.19 m | 4,134.356 m | 0.000000041 K |
| 2.5 | 7,385.316 m | 6,890.594 m | 0.000000025 K |
What each input means
- Black Hole Mass
- Mass of the black hole
- Spin Parameter
- Angular momentum parameter (0 = non-rotating, <1 = rotating)
How this is calculated
Formula
r_s = 2GM/c² (Schwarzschild Radius)Worked example, using the default values
- Identify Input Parameters2 parametersBlack Hole Mass = 1, Spin Parameter = 0.5 = 2 input(s) provided
- Calculate Schwarzschild RadiusSchwarzschild Radius2954.127 = 2954.127
- Calculate Event Horizon RadiusEvent Horizon Radius2756.238 = 2756.238
- Calculate Hawking TemperatureHawking Temperature6.2e-8 = 6.2e-8
- Calculate Ergosphere RadiusErgosphere Radius2954.127 = 2954.127
Engine last updated . Checked against 4 independently-derived tests — how we verify calculators. Built by Paul Gunder, a software engineer, not a licensed financial, medical, or legal professional.
Frequently Asked Questions
Why does Ergosphere Radius stay the same number when I change Spin Parameter?
Because this calculator reports the ergosphere's EQUATORIAL boundary, and the Kerr metric shows that boundary sits at exactly 2GM/c^2 regardless of spin -- the same formula as the non-rotating Schwarzschild Radius. The ergosphere narrows toward the event horizon only near the poles, a variation this calculator does not compute; the equatorial bulge stays fixed no matter how fast the hole spins, which is a genuine feature of the Kerr metric rather than a rounding coincidence.
Does raising Spin Parameter shrink the black hole itself?
It shrinks the Event Horizon Radius specifically, not the hole's mass or total gravity. A maximally spinning Kerr hole's horizon sits at half the radius of a non-spinning hole of the same mass (GM/c^2 instead of 2GM/c^2), because frame-dragging lets the horizon retreat closer to the singularity while still trapping light. Black Hole Mass, and therefore Hawking Temperature and Hawking Lifetime, are unaffected by Spin Parameter in this model.
Why is Hawking Temperature such an impossibly small number?
Hawking Temperature is inversely proportional to Black Hole Mass, and stellar and supermassive black holes are enormously massive. Even a modest solar-mass black hole computes to a temperature far below a microkelvin -- colder than the 2.7 K cosmic microwave background that bathes all of space -- meaning a real solar-mass black hole absorbs far more radiation than it emits and is still growing, not evaporating, today.
Why does Spin Parameter stop at 0.99 instead of the theoretical maximum of 1.0?
Spin Parameter is the dimensionless Kerr spin a* = Jc/(GM^2). At exactly 1.0 the event horizon and ergosphere coincide and the hole becomes an extremal black hole, a mathematical limiting case current physics doesn't expect any real object to reach. Astrophysical black holes measured via X-ray reflection spectroscopy are typically inferred to have a* well under 1 -- so 0.99 already represents a near-maximal, observationally realistic spin without hitting the singular extremal case.
Why is Hawking Lifetime reported in years when everything else uses SI units?
Hawking Lifetime is computed in seconds from the standard evaporation-time formula and then divided into years purely for readability -- the raw number of seconds in even a solar-mass black hole's lifetime is otherwise unreadable. The conversion doesn't change the underlying physics, which depends on Black Hole Mass through a cube relationship: doubling Black Hole Mass multiplies Hawking Lifetime by eight, not two.
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