Schwarzschild Radius Calculator

Calculate event horizon size from mass, reverse radius into mass, compare objects, explore advanced properties, and export clear scientific results with accurate constants instantly.

Scientific calculator

Enter mass or radius

Decimals and scientific notation are accepted.

Astronomical presets

Advanced black-hole options
Used for the Kerr horizon comparison.
Used for Reissner–Nordström horizons.
Controls time-dilation and escape estimates.
Custom physical constants

Comparison mode

Compare several masses

Local history

Recent calculations

Formula used

Schwarzschild radius equations

Radius from mass

rₛ = 2GM / c²

Here, G is the gravitational constant. M is mass. c is light speed.

Mass from radius

M = rₛc² / 2G

This inverse equation finds the required mass for any chosen radius.


Diameter

d = 2rₛ

Circumference

C = 2πrₛ

Horizon area

A = 4πrₛ²

Average density

ρ = M ÷ [(4/3)πrₛ³]

Photon sphere

r = 1.5rₛ

Schwarzschild ISCO

r = 3rₛ

Instructions

How to use this calculator

  1. Choose mass-to-radius or radius-to-mass mode.
  2. Enter a positive value using decimal or scientific notation.
  3. Select the matching input and preferred output units.
  4. Choose precision, notation, and optional advanced settings.
  5. Select Calculate to generate detailed scientific results.
  6. Copy, print, share, or export the calculation.
  7. Use comparison mode for several objects.
  8. Restore recent entries from local calculation history.
Average enclosed density is a mathematical average. It is not the physical density at a singularity.

Example data

Schwarzschild radius examples

ObjectApproximate massRadiusDiameterScale note
70 kg human70 kg1.04 × 10⁻²⁵ m2.08 × 10⁻²⁵ mFar smaller than a proton.
Earth5.9722 × 10²⁴ kg8.87 mm17.7 mmRoughly marble-sized diameter.
Jupiter1.89813 × 10²⁷ kg2.82 m5.64 mComparable with a small room.
Sun1.98847 × 10³⁰ kg2.953 km5.907 kmMuch smaller than the present Sun.
10 solar masses1.98847 × 10³¹ kg29.53 km59.07 kmTypical stellar black-hole scale.
Sagittarius A*About 4.3 million SunsAbout 12.7 million kmAbout 25.4 million kmApproximate editable preset value.

Assumptions

Model limits and scientific cautions

Basic Schwarzschild assumptions

  • Spherical symmetry
  • No angular momentum
  • No electric charge
  • Vacuum outside the mass
  • Classical general relativity
  • No quantum-gravity correction

Important interpretation

Any mass has a mathematical Schwarzschild radius. Ordinary objects remain much larger. They are therefore not black holes.

Real astrophysical black holes generally rotate. Kerr geometry often describes them better.

Educational guide

Understanding the Schwarzschild radius

What the radius represents

The Schwarzschild radius defines a critical boundary around compact mass. Crossing this boundary prevents signals from reaching distant observers. The boundary is called an event horizon. It is not a solid surface. Its location depends directly on total mass.

Every mass has a calculated Schwarzschild radius. Earth therefore has one mathematically. However, Earth remains enormously larger than that radius. Earth would require extreme compression before becoming a black hole.

Why mass changes the result

The formula shows a linear relationship with mass. Doubling mass doubles the Schwarzschild radius. Ten solar masses produce ten solar Schwarzschild radii. This simple scaling makes comparisons especially useful.

Area does not grow linearly with mass. Horizon area depends on radius squared. Average enclosed density decreases for larger Schwarzschild black holes. This result often surprises new learners.

Radius, singularity, and event horizon

The event horizon surrounds the black hole interior. The classical singularity lies deeper within the solution. These concepts are not interchangeable. The calculator reports horizon geometry, not singularity size.

A distant observer sees strong time effects near the horizon. Proper time remains local for falling observers. Coordinates can describe these experiences differently. General relativity resolves those differences through spacetime geometry.

Rotation and electric charge

The basic equation assumes zero rotation and zero charge. Real black holes can rotate rapidly. Kerr geometry then replaces the Schwarzschild solution. Rotation changes horizon locations and orbital structure.

Charged solutions use Reissner–Nordström geometry. Large net charge is unlikely astrophysically. Surrounding plasma tends to neutralize charge. Charged models remain valuable theoretical examples.

Advanced quantities

Hawking temperature decreases as mass increases. Large black holes are therefore extremely cold. Evaporation time rises rapidly with mass. Stellar black holes survive vastly longer than current cosmic ages.

Surface gravity measures horizon acceleration behavior. Entropy scales with event-horizon area. Photon spheres mark unstable circular light paths. The innermost stable circular orbit guides accretion modeling.

Using results responsibly

This calculator provides educational estimates under explicit assumptions. Custom constants support experiments and classroom demonstrations. Extreme values can exceed ordinary floating-point precision. Exported results should retain units and assumptions.

Use this tool for educational scientific exploration and comparison.

Frequently asked questions

Schwarzschild radius questions

What is the Schwarzschild radius?

It is the event-horizon radius for a spherical, non-rotating, uncharged mass under classical general relativity.

Does every object have this radius?

Every mass has a mathematical Schwarzschild radius. It becomes a black hole only after compression inside that radius.

What is Earth’s Schwarzschild radius?

Using standard values, Earth’s radius is about 8.87 millimetres. Earth remains vastly larger than this.

What is the Sun’s Schwarzschild radius?

The Sun’s radius is approximately 2.95 kilometres. Its current physical radius is much larger.

Why does density fall for larger black holes?

Mass grows with radius, while enclosed volume grows with radius cubed. Therefore average enclosed density decreases.

Is the event horizon a physical surface?

No. It is a causal boundary in spacetime. Matter can cross it without striking a material shell.

Does rotation change the horizon?

Yes. Rotating black holes use Kerr geometry. Their horizon structure depends on mass and angular momentum.

Can I use custom constants?

Yes. Enable custom constants for experiments. Standard calculations should normally retain accepted SI values.

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Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.