Galactic rotation

E471606

Galactic rotation is the large-scale orbital motion of stars and gas around the center of a galaxy, revealing its mass distribution and the presence of dark matter.

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Statements (55)

Predicate Object
instanceOf astrophysical phenomenon
galactic dynamics phenomenon
appliesTo barred spiral galaxies
irregular galaxies
lenticular galaxies
spiral galaxies
the Milky Way NERFINISHED
characterizedBy approximately flat outer rotation curves
non-Keplerian velocity profiles
rotation velocity as a function of radius
dependsOn galactic halo properties
radial mass distribution
total galactic mass
describes large-scale motion around galactic centers
orbital motion of gas in galaxies
orbital motion of stars in galaxies
evidenceFor existence of dark matter
extended dark matter halos
field astrophysics
galactic astronomy
hasKeyConcept Keplerian decline
MOND NERFINISHED
Newtonian gravity NERFINISHED
baryonic matter
circular velocity
dark matter halo
differential rotation
flat rotation curve
mass-to-light ratio
modified gravity theories
orbital period
rotation curve
influences galactic disk stability
orbital resonances in disks
spiral arm structure
star formation patterns
modeledBy N-body simulations
hydrodynamical simulations
mass distribution models
relatedTo Oort constants NERFINISHED
Tully–Fisher relation NERFINISHED
dark matter
galactic gravitational potential
mass distribution in galaxies
rotation curves of galaxies
reveals distribution of dark matter in galaxies
distribution of visible matter in galaxies
total mass of galaxies
studiedUsing 21 cm hydrogen line observations
Doppler shift measurements
optical spectroscopy
radio astronomy
usedFor estimating galaxy masses
probing dark matter distribution
testing gravity theories

Referenced by (1)

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

Jan Oort knownFor Galactic rotation