INGENIA

REL-26

Schwarzschild radius

Event-horizon scale.

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GoverningSchwarzschild radius

Governing equation

Rs=2GM/c2R_s=2GM/c^2

where

M
M (Msun)
Rs
Schwarzschild radius (km)

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-26 — Schwarzschild radius) is the form associated with Schwarzschild radius. Working symbols: MM \rightarrow RsRs. Event-horizon scale. Pedagogical SI sheet with a live model and a swept parameter.

Purpose

Purpose: compute RsRs from MM in Relativity via Rs=2GM/c2R_s=2GM/c^2 Event-horizon scale. 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=1.000MsunM = 1.000\,\mathrm{Msun}, the governing relation Rs=2GM/c2R_s=2GM/c^2 yields Rs=2.948kmRs = 2.948\,\mathrm{km}. One governing identity, SI units, a single sweep on the sheet. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Schwarzschild radius Rs2.948 km
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REL-26 · orbit
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Narration of this film

One governing identity, SI units, a single sweep on the sheet.

Event-horizon scale. Pedagogical SI sheet with a live model and a swept parameter.

Reading speed

Watch on YouTube