Spherical stellar mass and pressure structure
For a spherical quasistatic Newtonian star, enclosed mass increases with shell volume and density, while the pressure gradient balances gravity due to enclosed mass.
Key knowledge
For a spherical quasistatic Newtonian star, enclosed mass increases with shell volume and density, while the pressure gradient balances gravity due to enclosed mass. These coupled equations describe interior structure rather than a point mass held at one pressure.
Values and equations
dm/dr = 4πr²ρ; dP/dr = −Gmρ/r²
- m
- enclosed mass kg
- r
- radius m
- ρ
- density kg m⁻³
- P
- pressure Pa
- G
- Newtonian gravitational constant m³ kg⁻¹ s⁻²
Conditions and scope
- Rotation, magnetic stresses, rapid collapse and relativistic gravity require additional terms or a different model.
- An equation of state, energy/transport relations and boundary conditions are needed to close the structure problem.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Read shell-mass and hydrostatic equations; retained spherical/quasistatic assumptions and corrected the notes' malformed r-squared rendering in the flux expression.
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-stellar-hydrostatic
- Revision
- core.1
- Structured reference record
- University core expansion