Upper Scorpius

E514325

Upper Scorpius is a nearby, young stellar subgroup rich in massive, hot stars and active star formation, located within the larger Scorpius–Centaurus OB association.

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Statements (47)

Predicate Object
instanceOf OB subgroup
star-forming region
stellar association subgroup
contains massive OB stars that ionize surrounding gas
numerous X-ray active young stars
hasAlternativeName USco NERFINISHED
Upper Sco subgroup NERFINISHED
hasApproximateAge 5–11 million years
~10 million years
hasDistanceFromSun ~140 parsecs
~450 light-years
hasEnvironment relatively low extinction compared to embedded regions
remnant of a past giant molecular cloud
hasKinematicProperty co-moving stellar group
common space motion of member stars
hasMemberCount hundreds of confirmed stellar members
many candidate members identified by Gaia
hasProperty active star formation
nearby to the Sun
rich in hot stars
young stellar population
hasRoleIn nearby star-formation history studies
studies of circumstellar disks
studies of early stellar evolution
studies of planet formation timescales
hasSignificance benchmark region for testing pre-main-sequence models
important for understanding recent local star formation
key region for studying disk dispersal
hasStellarPopulation Herbig Ae/Be stars
OB stars
T Tauri stars NERFINISHED
brown dwarfs
low-mass stars
massive stars
pre-main-sequence stars
isAssociatedWith Lower Centaurus–Crux subgroup NERFINISHED
Upper Centaurus–Lupus subgroup NERFINISHED
isLocatedIn Milky Way NERFINISHED
constellation Scorpius NERFINISHED
solar neighborhood
isObservedIn X-ray wavelengths
infrared wavelengths
optical wavelengths
isOneOf three main Sco–Cen subgroups
isSubgroupOf Scorpius–Centaurus OB association NERFINISHED
partOf Scorpius–Centaurus OB association NERFINISHED
Sco–Cen OB association NERFINISHED

Referenced by (1)

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