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gptkbp:instanceOf
|
astronomical structure
|
|
gptkbp:age
|
about 30 to 50 million years
|
|
gptkbp:centeredIn
|
gptkb:constellation_Perseus
|
|
gptkbp:contains
|
gptkb:Orion_OB1_association
gptkb:Vela_OB2_association
gptkb:Cepheus_OB2_association
gptkb:Chamaeleon_molecular_cloud
gptkb:Lacerta_OB1_association
gptkb:Lupus_molecular_cloud
gptkb:Ophiuchus_molecular_cloud
gptkb:Orion_molecular_cloud_complex
gptkb:Perseus_OB2_association
gptkb:Scorpius–Centaurus_association
gptkb:Taurus_molecular_cloud
gptkb:OB_associations
young stars
molecular clouds
many of the nearest bright stars to the Sun
|
|
gptkbp:diameter
|
about 3000 light-years
|
|
gptkbp:discoveredBy
|
gptkb:Benjamin_Gould
|
|
gptkbp:discoveredIn
|
1879
|
|
gptkbp:distanceFromEarth
|
about 1000 light-years
|
|
gptkbp:hasViewOf
|
gptkb:Earth
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Gould Belt
|
|
gptkbp:inclinationAngle
|
about 16 to 20 degrees
|
|
gptkbp:inclinedTo
|
galactic plane
|
|
gptkbp:locatedIn
|
gptkb:Milky_Way
|
|
gptkbp:namedAfter
|
gptkb:Benjamin_Gould
|
|
gptkbp:notableFor
|
high rate of star formation
|
|
gptkbp:passesThrough
|
gptkb:Orion
gptkb:Ophiuchus
gptkb:Taurus
gptkb:Perseus
gptkb:Cepheus
gptkb:Centaurus
gptkb:Lupus
gptkb:Scorpius
Vela
|
|
gptkbp:relatedTo
|
gptkb:Local_Bubble
gptkb:Lindblad_Ring
gptkb:Radcliffe_Wave
|
|
gptkbp:type
|
partial ring of stars
|
|
gptkbp:bfsParent
|
gptkb:Hyades
gptkb:Benjamin_A._Gould
gptkb:Loop_I_Bubble
|
|
gptkbp:bfsLayer
|
6
|