INGENIA

REL-06

Schwarzschild radius

Rs = 2 G M / c².

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Black holesSchwarzschild 1916

Governing equation

Rs=2GMc2R_s=\dfrac{2GM}{c^2}

M∈[0.1,1×109]M \in \left[0.1, 1\times 10^{9}\right]

where

M
Mass (suns) (M_\odot)
R_s
Schwarzschild radius (km)

The figure, part by part

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REL-06 · orbit
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①

Governing law — red

Rs=2GMc2R_s=\dfrac{2GM}{c^2}

M∈[0.1,1×109]M \in \left[0.1, 1\times 10^{9}\right]

M=0.1M = 0.1Rs=0.295R_s = 0.295

②

Domain of the variable — blue

Mmin⁡=0.1,Mmax⁡=1×109M_{\min} = 0.1,\quad M_{\max} = 1\times 10^{9}

M∈[0.1,1×109]M \in \left[0.1, 1\times 10^{9}\right]

M=0.1M = 0.1M=0.1M = 0.1

③

Response curve — green

Rs=2GMc2R_s=\dfrac{2GM}{c^2}

M∈[0.1,1×109]M \in \left[0.1, 1\times 10^{9}\right]

M=0.1M = 0.1Rs=0.295R_s = 0.295

④

Rate of change — amber

dRsdM\frac{\mathrm{d}R_s}{\mathrm{d}M}

M∈[0.1,1×109]M \in \left[0.1, 1\times 10^{9}\right]

M=6.29×106M = 6.29\times 10^{6}Rs′=2.953R_s^{\prime} = 2.953

Lecture brief

Historical brief

Einstein’s 1905 Lorentz kinematics and 1915 field equation, then Schwarzschild (1916) and Hawking temperature, recast time, mass and gravity. The lab computes dilation, E=mc² and horizon scales. This sheet (REL-06 — Schwarzschild radius) is the form associated with Schwarzschild 1916. Working symbols: MM →\rightarrow RsR_s. Schwarzschild's vacuum solution of Einstein's equation has a coordinate singularity at r = 2GM/c², the event horizon of a non-rotating black hole.

Purpose

Purpose: compute RsR_s from MM in Relativity via Rs=2GMc2R_s=\dfrac{2GM}{c^2} Rs = 2 G M / c². Use it when a real relativity question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given M=10.000 ModotM = 10.000\,\mathrm{M_odot}, the governing relation Rs=2GMc2R_s=\dfrac{2GM}{c^2} yields Rs=29.533 kmR_s = 29.533\,\mathrm{km}. Non-rotating uncharged mass. Move a slider: the numbers are this situation, not a canned story.

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Inputs

Outputs

  • Schwarzschild radius R_s29.533 km
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Narration of this film

Non-rotating uncharged mass.

Schwarzschild's vacuum solution of Einstein's equation has a coordinate singularity at r = 2GM/c², the event horizon of a non-rotating black hole.

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