AST-11
Escape velocity
v_esc = √(2 G M / r). The speed to reach infinity from r.
Governing equation
where
- M
- Mass (M_\odot)
- r
- Radius (R_\odot)
- v_{esc}
- Escape speed (km/s)
The figure, part by part
Each numbered marker wears the color of its card. Hover a card to light the marker. Tap a marker to jump to that card. The slider walks a red point along the curve; Animate drawing traces it like a pen.
Governing law — red
Domain of the variable — blue
Response curve — green
Rate of change — amber
Lecture brief
Historical brief
Hubble expansion, Jeans collapse, Eddington luminosity, Bondi accretion and Stefan–Boltzmann stars are the first astrophysical budgets. The sheets scale a star, a cloud and a horizon. This sheet (AST-11 — Escape velocity) is the form associated with Escape velocity. Working symbols: , . √2 times circular speed. At r_s it equals c — the black-hole edge.
Purpose
Live realistic example
In symbols
Calculator
Inputs
Outputs
- Escape speed v_{esc}617.68 km/s
Watch on YouTube
Free library
Full libraryFree PDF / open book
- University Physics Vol. 3 (optics, modern)OpenStax · CC BY · Free PDF / open book
- College Physics 2eOpenStax · CC BY · Free PDF / open book
- Astronomy 2eOpenStax · CC BY · Free PDF / open book
- LibreTexts PhysicsLibreTexts · CC · Free PDF / open book
YouTube channels
Narration of this film
A world, a departing probe, a v_esc.
√2 times circular speed. At r_s it equals c — the black-hole edge.
Watch on YouTube