Statements (99)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Nebula_Award
|
| gptkbp:age |
2 million years
|
| gptkbp:associated_with |
gptkb:30_Doradus
gptkb:supernova_remnants |
| gptkbp:contains |
gptkb:Wolf-Rayet_stars
star-forming regions massive stars HII regions young stellar clusters |
| gptkbp:diameter |
1,000 light years
|
| gptkbp:discovered_by |
gptkb:John_Herschel
|
| gptkbp:discovery_year |
1834
|
| gptkbp:distance_from_earth |
161,000 light years
approximately 161,000 light-years |
| gptkbp:features |
gptkb:Wolf-Rayet_stars
gptkb:supernova_remnants |
| gptkbp:has |
complex structure
high stellar density |
| https://www.w3.org/2000/01/rdf-schema#label |
Tarantula Nebula
|
| gptkbp:image |
gptkb:Hubble_Space_Telescope
|
| gptkbp:is_a |
gptkb:region
|
| gptkbp:is_associated_with |
gptkb:LMC_2
cosmic rays star clusters stellar populations stellar winds supernova explosions |
| gptkbp:is_characterized_by |
high luminosity
high-energy processes |
| gptkbp:is_examined_in |
chemical composition
|
| gptkbp:is_explored_in |
space telescopes
stellar populations |
| gptkbp:is_home_to |
massive star formation
young stellar objects massive star clusters young stellar clusters massive stellar populations young massive stars supergiant stars nebular emissions |
| gptkbp:is_influential_in |
astrophysics research
|
| gptkbp:is_known_for |
stellar winds
stellar nurseries extensive research bright emission lines spectacular images high-energy phenomena bright nebular emission |
| gptkbp:is_located_in |
southern hemisphere
Doradus region |
| gptkbp:is_located_near |
gptkb:NGC_2070
gptkb:30_Doradus |
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:is_part_of |
gptkb:galaxy
gptkb:LMC_star_formation_region gptkb:Local_Group gptkb:Doradus_constellation gptkb:interstellar_medium gptkb:LMC intergalactic medium star-forming complex starburst region LMC star formation history LMC star formation regions |
| gptkbp:is_significant_for |
galactic studies
|
| gptkbp:is_studied_for |
galactic dynamics
chemical composition stellar evolution stellar lifecycle stellar feedback |
| gptkbp:is_studied_in |
gptkb:astronomy
gptkb:cosmology astrophysics |
| gptkbp:is_surrounded_by |
gptkb:interstellar_medium
dark nebulae |
| gptkbp:is_visible_from |
gptkb:Earth
infrared spectrum optical wavelengths radio wavelengths infrared wavelengths southern sky radio spectrum small telescopes optical spectrum |
| gptkbp:known_as |
gptkb:30_Doradus
|
| gptkbp:lighting |
magnitude 8.0
very bright in infrared |
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:mass |
10 million solar masses
|
| gptkbp:notable_for |
high rate of star formation
|
| gptkbp:part_of |
gptkb:NGC_2070
LMC-3 region |
| gptkbp:size |
approximately 1,000 light-years across
|
| gptkbp:bfsParent |
gptkb:NGC_2070
gptkb:The_LMC_(Large_Magellanic_Cloud) gptkb:LMC_(Large_Magellanic_Cloud) gptkb:30_Doradus gptkb:Large_Magellanic_Cloud |
| gptkbp:bfsLayer |
6
|