Schwarzschild Radius Calculator

Calculate the Schwarzschild radius — the critical radius at which a mass becomes a black hole. If an object is compressed within this radius, not even light can escape its gravitational pull.

Enter the mass of the object you want to analyze.

Formula

rs = 2GM / c²

  • rs — Schwarzschild radius (m)
  • G — Gravitational constant = 6.67430 × 10⁻¹¹ m³ kg⁻¹ s⁻²
  • M — Mass of the object (kg)
  • c — Speed of light in vacuum = 2.99792458 × 10⁸ m/s

This formula is derived from Karl Schwarzschild's 1916 exact solution to Einstein's field equations of general relativity for a non-rotating, spherically symmetric mass.

Assumptions & References

  • The object is assumed to be non-rotating and uncharged (Schwarzschild metric). Rotating black holes require the Kerr metric; charged ones require the Reissner–Nordström metric.
  • The result is the event horizon radius — the boundary inside which escape velocity exceeds the speed of light.
  • Gravitational constant G = 6.67430 × 10⁻¹¹ m³ kg⁻¹ s⁻² (NIST CODATA 2018).
  • Speed of light c = 299,792,458 m/s (exact, by SI definition).
  • 1 Solar Mass (M☉) = 1.98892 × 10³⁰ kg; 1 Earth Mass (M⊕) = 5.97219 × 10²⁴ kg.
  • The Schwarzschild radius of the Sun ≈ 2.953 km; of the Earth ≈ 8.871 mm.
  • Reference: Schwarzschild, K. (1916). Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie. Sitzungsberichte der Königlich Preußischen Akademie der Wissenschaften.

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