Jeans mass

E59371

The Jeans mass is the critical mass above which a cloud of gas becomes gravitationally unstable and begins to collapse, playing a key role in the formation of stars and galaxies.

AI illustration

How this image was made

AI-generated illustration of Jeans mass

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of the Jeans mass (The Jeans mass is the critical mass above which a cloud of gas becomes gravitationally unstable and begins to collapse, playing a key role in the formation of stars and galaxies.)

All labels observed (2)

Label Occurrences
Jeans mass canonical 4
Jeans length 1

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf astrophysical concept ⓘ
gravitational instability criterion ⓘ
physical quantity ⓘ
appliesTo interstellar molecular clouds ⓘ
primordial gas in the early universe ⓘ
protogalactic gas clouds ⓘ
approximateFormula M_J ∝ T^{3/2} ρ^{-1/2} ⓘ
M_J ≈ (5 k_B T / G μ m_H)^{3/2} (3 / 4πρ)^{1/2} ⓘ
assumes Newtonian gravity ⓘ
isothermal gas ⓘ
small perturbations in an infinite medium ⓘ
uniform density ⓘ
balances thermal pressure against gravitational attraction at the stability threshold ⓘ
characterizes onset of gravitational instability in a self-gravitating gas ⓘ
condition cloud remains stable when mass is below Jeans mass ⓘ
collapse occurs when cloud mass exceeds Jeans mass ⓘ
contrastedWith Bonnor–Ebert mass ⓘ
dependsOn gas density ⓘ
gas temperature ⓘ
mean molecular weight of the gas ⓘ
sound speed in the gas ⓘ
describes critical mass for gravitational collapse of a gas cloud ⓘ
dimension mass ⓘ
directlyProportionalTo 3/2 power of gas temperature ⓘ
field astrophysics ⓘ
cosmology ⓘ
star formation theory ⓘ
historicalContext introduced in early 20th century gravitational instability analyses ⓘ
influences fragmentation scale of collapsing clouds ⓘ
typical mass scale of forming stars ⓘ
inverselyProportionalTo square root of gas density ⓘ
namedAfter James Jeans ⓘ
relatedTo Jeans instability ⓘ
Jeans length ⓘ
linked to: Jeans mass

free-fall time ⓘ
self-gravity of gas clouds ⓘ
thermal pressure support ⓘ
virial theorem ⓘ
roleIn formation of galaxies ⓘ
formation of stars ⓘ
formation of stellar clusters ⓘ
symbol M_J ⓘ
usedIn initial mass function studies ⓘ
models of molecular cloud fragmentation ⓘ
numerical simulations of star formation ⓘ
structure formation in the early universe ⓘ

How these facts were elicited

Referenced by (5)

Full triples — surface form annotated when it differs from this entity's canonical label.

Jeans mass → relatedTo → Jeans length ⓘ
linked to: Jeans mass
James Jeans → knownFor → Jeans mass ⓘ
Bonnor–Ebert mass → relatedTo → Jeans mass ⓘ