Statements (62)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:age |
a few million years
approximately 3 million years |
| gptkbp:analyzes |
its role in galactic evolution
|
| gptkbp:associated_with |
gptkb:supernova_remnants
star formation |
| gptkbp:contains |
young stars
massive stars |
| gptkbp:coordinates |
RA 05h 38m 42s, Dec -69° 45' 00"
|
| gptkbp:depicted_in |
gptkb:physicist
optical wavelengths |
| gptkbp:discovered_by |
gptkb:Henrietta_Leavitt
gptkb:observatory |
| gptkbp:distance |
approximately 163,000 light years
|
| gptkbp:emissions_standard |
hydrogen emission lines
|
| gptkbp:examines |
stellar population studies
its interaction with the Milky Way star cluster dynamics |
| https://www.w3.org/2000/01/rdf-schema#label |
LMC 21
|
| gptkbp:ingredients |
massive star clusters
|
| gptkbp:is_analyzed_in |
chemical composition
stellar evolution theories |
| gptkbp:is_associated_with |
stellar nurseries
the Tarantula Nebula |
| gptkbp:is_connected_to |
the cosmic web
the history of the LMC |
| gptkbp:is_considered |
a key site for astrophysical research
|
| gptkbp:is_documented_in |
gptkb:literary_work
astronomical catalogs |
| gptkbp:is_explored_in |
gptkb:musician
|
| gptkbp:is_home_to |
massive stars
various types of nebulae various stellar types |
| gptkbp:is_influenced_by |
supernova explosions
|
| gptkbp:is_influential_in |
the surrounding interstellar medium.
|
| gptkbp:is_known_for |
a region of active star formation
its bright emission nebulae its bright colors in images |
| gptkbp:is_located_near |
the 30 Doradus region
|
| gptkbp:is_noted_for |
its high star formation rate
|
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
radio wavelengths |
| gptkbp:is_part_of |
gptkb:star
the Local Group of galaxies the LMC star formation history the LMC's complex structure the LMC's star formation regions the interstellar medium of LMC the study of extragalactic astronomy |
| gptkbp:is_rich_in |
gas and dust
|
| gptkbp:is_studied_in |
infrared observations
stellar formation processes its impact on surrounding regions |
| gptkbp:length |
approximately 100 light-years across
|
| gptkbp:lighting |
apparent magnitude of 12.5
|
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
coordinates in the southern sky |
| gptkbp:significance |
understanding galaxy evolution
|
| gptkbp:type |
gptkb:region
gptkb:star |