Statements (91)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:astronomy
|
gptkbp:contains |
gptkb:the_Pleiades_star_cluster
gptkb:the_Hyades_star_cluster star-forming regions star formation regions the Orion Nebula the Rho Ophiuchi cloud complex the Sco-Cen association the Carina Nebula |
gptkbp:feature |
the Milky Way's structure
the galactic structure the Galactic plane |
gptkbp:has_a_focus_on |
stellar evolution studies
stellar research |
gptkbp:has_produced |
from a past supernova event
|
https://www.w3.org/2000/01/rdf-schema#label |
Gould's Belt
|
gptkbp:includes |
the constellation Sagittarius
the Orion Arm the constellation Orion the Scorpius-Centaurus Association the constellation Scorpius |
gptkbp:is_a_region_that_has_been_identified_as |
a key area for research
a star-forming region |
gptkbp:is_a_region_that_has_been_mapped_by |
gptkb:astronomy
|
gptkbp:is_a_region_that_has_been_observed_by |
space telescopes
|
gptkbp:is_a_region_that_has_been_studied_for |
stellar dynamics
|
gptkbp:is_a_region_that_is_associated_with |
the formation of stars
the Galactic Center |
gptkbp:is_a_region_that_is_characterized_by |
young stellar objects
young stellar populations |
gptkbp:is_a_region_that_is_crucial_for |
understanding the Milky Way's structure.
|
gptkbp:is_a_region_that_is_important_for |
understanding galactic evolution
understanding the Milky Way |
gptkbp:is_a_region_that_is_often_analyzed_for |
stellar population studies
|
gptkbp:is_a_region_that_is_often_included_in |
galactic surveys
astronomical surveys |
gptkbp:is_a_region_that_is_often_observed_in |
radio wavelengths
|
gptkbp:is_a_region_that_is_often_referenced_in |
gptkb:literature
astronomical literature |
gptkbp:is_a_region_that_is_often_studied_in |
galactic astronomy
|
gptkbp:is_a_region_that_is_rich_in |
interstellar matter
|
gptkbp:is_a_region_that_is_significant_for |
cosmological studies
the study of stellar evolution |
gptkbp:is_a_structure_that_spans |
multiple constellations
|
gptkbp:is_a_subject_of |
galactic studies
|
gptkbp:is_approximately |
3,000 light-years in diameter
3,000 light-years long |
gptkbp:is_associated_with |
molecular clouds
the Gould Belt system the Orion Arm OB associations |
gptkbp:is_characterized_by |
young stars
high rates of star formation a high concentration of molecular clouds |
gptkbp:is_essential_for |
understanding star formation
|
gptkbp:is_explored_in |
stellar formation theories
|
gptkbp:is_home_to |
multiple open clusters
many young stars the Rho Ophiuchi cloud complex |
gptkbp:is_linked_to |
the solar neighborhood
|
gptkbp:is_located_in |
gptkb:the_Milky_Way_galaxy
|
gptkbp:is_often_studied_using |
infrared observations
|
gptkbp:is_part_of |
the local bubble
the local spiral arm structure |
gptkbp:is_said_to_be |
a result of galactic dynamics
|
gptkbp:is_significant_for |
observational astronomy
galactic archaeology |
gptkbp:is_studied_in |
astrophysics
|
gptkbp:is_surrounded_by |
older stellar populations
|
gptkbp:is_tilted_at_an_angle_of |
about 20 degrees to the plane of the Milky Way
about 20 degrees |
gptkbp:is_visible_from |
gptkb:Earth
|
gptkbp:named_after |
gptkb:B._A._Gould
|
gptkbp:region |
gptkb:exoplanet
gptkb:the_Lagoon_Nebula gptkb:the_Trifid_Nebula galactic dynamics various types of stars high stellar density its bright nebulae the larger structure of the Milky Way its star clusters multiple stellar associations numerous open clusters massive stars are born stellar nurseries are found the Southern Cross constellation a rich history of study new stars are born |
gptkbp:bfsParent |
gptkb:Ben_Gould
|
gptkbp:bfsLayer |
6
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