Local Volume

E450593

The Local Volume is the nearby region of the universe encompassing galaxies within roughly 10 megaparsecs of the Milky Way, used to study the structure, dynamics, and evolution of the local cosmos.

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Statements (48)

Predicate Object
instanceOf astronomical region
cosmological volume
boundaryDefinition often taken as radius of 8–11 megaparsecs in literature
centeredOn Milky Way NERFINISHED
characterizedBy detailed distance measurements to individual galaxies
relatively low redshift
significant peculiar velocities compared to Hubble flow
contains Andromeda Galaxy NERFINISHED
Local Group NERFINISHED
Milky Way NERFINISHED
Triangulum Galaxy NERFINISHED
dwarf galaxies
elliptical galaxies
field galaxies
irregular galaxies
nearby galaxy clusters
nearby galaxy groups
spiral galaxies
definedBy distance limit of roughly 10 megaparsecs from the Milky Way
distanceLimit ~10 megaparsecs
~30 million light-years
hasProperty allows high-resolution studies of galaxy structure
contains well-studied standard candles
provides benchmark for galaxy formation models
hasUncertainBoundary true
locatedIn observable universe NERFINISHED
observedBy optical telescopes
radio telescopes
space-based observatories
overlapsWith Local Group NERFINISHED
Local Sheet
Local Void boundary regions
relevantFor dark matter distribution studies
environmental effects on galaxies
near-field cosmology
star formation history of nearby universe
scale tens of millions of light-years
studiedIn extragalactic astronomy
galaxy evolution research
observational cosmology
usedFor calibration of distance indicators
mapping the local cosmic web
measurement of the Hubble constant on local scales
studies of peculiar velocities
study of galaxy dynamics
study of galaxy evolution
study of local large-scale structure
study of nearby galaxies

Referenced by (1)

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

M81 Group memberOfLargerStructure Local Volume