AST-26
Surface gravity
g = G M / R². Surface acceleration of a spherical body.
Governing equation
where
- M
- Mass (M_\odot)
- R
- Radius (R_\odot)
- g
- Gravity (m/s²)
- \log g
- log g (cgs)
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-26 — Surface gravity) is the form associated with Surface gravity. Working symbols: , , . log g in cgs is the stellar-atmosphere parameter. White dwarfs have log g ~ 8.
Purpose
Live realistic example
In symbols
Calculator
Inputs
Outputs
- Gravity g274.208 m/s²
- log g \log g4.438 cgs
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 falling test mass.
log g in cgs is the stellar-atmosphere parameter. White dwarfs have log g ~ 8.
Watch on YouTube