Astronomy and astrophysics Definition
Eddington luminosity
Builds on Newton's law of universal gravitationHydrostatic equilibrium
Definition
Let be the mass of a spherically symmetric body. Let the gas around it have opacity , the cross-section per unit mass for absorption and scattering of radiation. Let be the gravitational constant and the speed of light. The Eddington luminosity of the body is
Remarks
At distance , the radiative force on a unit mass of gas is . The Eddington luminosity is the value of for which it equals the gravitational force given by Newton's law of gravitation. For gravity wins and a static atmosphere in hydrostatic equilibrium is possible. Example: for fully ionized hydrogen the opacity is that of electron scattering, . Here is the Thomson cross-section and the proton mass. Then , about , or solar luminosities, per solar mass. Non-example: a luminosity does not balance gravity, since the radiative force on each unit mass is then twice the gravitational force, and the gas is driven outward. The ratio is called the Eddington ratio.
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Further reading
About this page
| Tag | RH17N68SJP |
|---|---|
| URI | m2://RH17N68SJP |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A15, 85A25 |
| Defines | Eddington luminosity |
| Uses | Newton's law of universal gravitation, Hydrostatic equilibrium |
| Changed | 3 November 2026 |
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