Eta Carinae Nebula

GPTKB entity

Statements (106)
Predicate Object
gptkbp:instance_of gptkb:Nebula_Award
gptkbp:age about 2 million years
gptkbp:associated_with star formation
gptkbp:average_temperature around 10,000 K
gptkbp:composed_of hydrogen, helium, and heavier elements
gptkbp:contains gptkb:NGC_3372
dense gas and dust
Eta Carinae star system
gptkbp:contains_gas_and_dust yes
gptkbp:discovered_by gptkb:John_Herschel
gptkbp:distance_from_earth approximately 7,500 light-years
approximately 7,500 light years
gptkbp:emissions_standard yes
gptkbp:exhibition 1837
gptkbp:features the Homunculus Nebula
gptkbp:has_color blue and red hues
gptkbp:has_high_energy X-ray emissions
gptkbp:has_spectacular_images_from space telescopes
gptkbp:has_spectral_type O-type stars
https://www.w3.org/2000/01/rdf-schema#label Eta Carinae Nebula
gptkbp:is_a gptkb:star
gptkbp:is_associated_with gptkb:supernova_remnants
massive star formation
stellar winds
the star formation process
the Carina Nebula complex
gptkbp:is_home_to gptkb:Wolf-Rayet_stars
young stellar objects
multiple stellar populations
massive star clusters
multiple star clusters
various types of nebulae
young massive stars
massive star Eta Carinae
the star Eta Carinae
massive stars like Eta Carinae A and B
the Homunculus Nebula structure
gptkbp:is_known_for its variability
massive stars
its complex structure
its historical significance in astronomy
its role in the life cycle of stars
its bright and colorful appearance
its outflows and jets
gptkbp:is_located_near the Southern Cross constellation
gptkbp:is_observed_in gptkb:Hubble_Space_Telescope
observed since the 19th century
gptkbp:is_part_of gptkb:interstellar_medium
gptkb:the_Milky_Way_galaxy
gptkb:Carina-Sagittarius_Arm
gptkb:star
gptkb:Milky_Way_galaxy
Giant Molecular Cloud
the interstellar medium
stellar nursery
galactic structure
the local group of galaxies
the Carina constellation
the Carina-Sagittarius Arm
starburst region
the Galactic plane
the larger Carina Nebula region
gptkbp:is_studied_for stellar dynamics
stellar evolution
its chemical composition
mass loss in stars
its stellar populations
its interaction with surrounding space
massive star interactions
its dynamics and kinematics
gptkbp:is_studied_in gptkb:Hubble_Space_Telescope
gptkb:astronomy
astrophysics
gptkbp:is_visible_from gptkb:Earth
gptkb:Seimas
yes
optical wavelengths
southern hemisphere
radio wavelengths
infrared wavelengths
infrared observations
amateur telescopes
ultraviolet wavelengths
gptkbp:length about 7 light-years across
gptkbp:lighting magnitude -4.0
very bright in infrared
gptkbp:located_in gptkb:Carina_constellation
gptkbp:mass approximately 100,000 solar masses
gptkbp:notable_feature gptkb:Homunculus_Nebula
gptkb:Great_Eruption_of_Eta_Carinae
complex structure
massive stars
dark lanes of dust
bright central region
nebular filaments
gptkbp:notable_for first observed in 1837
gptkbp:notable_person gptkb:Eta_Carinae_B
gptkb:Eta_Carinae_A
gptkbp:research_interest yes
gptkbp:size about 7 light years across
gptkbp:type gptkb:Nebula_Award
gptkbp:bfsParent gptkb:Carina
gptkb:Eta_Carinae
gptkb:Trumpler_16
gptkb:NGC_3372
gptkbp:bfsLayer 5