Luminosity and received flux
For an isotropic source in transparent Euclidean space, bolometric flux decreases as luminosity divided by the area of a sphere.
Key knowledge
For an isotropic source in transparent Euclidean space, bolometric flux decreases as luminosity divided by the area of a sphere. Intrinsic luminosity and received flux are different quantities; anisotropy, absorption and cosmological geometry require a different observation model.
Values and equations
F = L / (4πd²)
- F
- received bolometric flux W m⁻²
- L
- isotropic bolometric luminosity W
- d
- geometric distance m
Conditions and scope
- The distance is the ordinary geometric distance in the stated nearby-space model.
- Cosmological luminosity distance is defined to preserve this flux relation; it is not generally an angular-diameter distance.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Read the standard-candle flux equation; excluded dated distances and the notes' oversimplified description of a nearly constant expansion rate.
2026-10-10 · Independent AI editorial review: All26 Life-authored Cosmos compact statements, conditions, displayed equations and all56 origin semantic links read. Entire26-entry author statement/source matrix and explicit exclusions assessed. Targeted independent primary sections are listed below; this does not claim every referenced source body or proof was independently re-read. This is scoped AI reference-content review, not human disciplinary certification or whole-field completion. Receipt: cosmos-life-independent-content-review.1.
Entry details
Permanent link to this entry ↗- Record identity
- uni-cosmos-flux-luminosity
- Revision
- core.1
- Structured reference record
- University core expansion