NGC 3293

GPTKB entity

Statements (137)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:bfsLayer 4
gptkbp:bfsParent gptkb:Carina
gptkb:Carina_Nebula
gptkbp:age approximately 10 million years
gptkbp:apparent_magnitude 8.0
gptkbp:associated_with gptkb:Carina_Nebula
gptkb:Carina-Sagittarius_Arm
gptkbp:contains gptkb:NGC_2516
gptkb:NGC_3532
gptkb:NGC_2244
young stars
several hundred stars
massive stars
gptkbp:coordinates RA 10h 36m, Dec -58° 24'
l = 284.5°, b = -0.5°
gptkbp:declination -58° 24' 00"
gptkbp:depicted_in best viewed in southern hemisphere
visible to the naked eye under dark skies
gptkbp:diameter approximately 10 light years
gptkbp:discovered_by gptkb:John_Frederick_William_Herschel
gptkbp:distance approximately 4,000 light years
approximately 8,000 light years
gptkbp:exhibition gptkb:New_General_Catalogue
gptkbp:features bright central region
gptkbp:has_color 0.75
B-V = 0.5
B-V = 0.3
gptkbp:has_spectral_type various types
O and B type stars
gptkbp:historical_significance important for studying stellar evolution
https://www.w3.org/2000/01/rdf-schema#label NGC 3293
gptkbp:image Hubble Space Telescope image available
Hubble image available
gptkbp:is_observed_in gptkb:Hubble_Space_Telescope
gptkbp:is_similar_to gptkb:NGC_3532
gptkbp:lighting moderately bright
gptkbp:located_in gptkb:Carina_constellation
gptkbp:mass main sequence stars
giant stars
approximately 1,000 solar masses
about 100 stars
supergiant stars
predominantly young stars
gptkbp:membership includes both main sequence and giant stars
gptkbp:metallicity solar metallicity
gptkbp:mission none known
gptkbp:notable_feature bright central region
gptkbp:notable_person gptkb:HD_91700
gptkb:HD_91701
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gptkb:HD_91748
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gptkb:HD_91750
several B-type stars
gptkbp:part_of Carina Nebula region
gptkbp:previous_name C 10-36
gptkbp:research gptkb:musician
photometry
observed by various astronomers
amateur telescopes
best observed in winter months
highly obscured by dust
requires dark skies for best view
light pollution affects visibility
gptkbp:research_focus studies of stellar evolution
important for studying star formation
gptkbp:research_interest analyzed for chemical composition
studied for star formation processes
analyzed for stellar rotation rates
compared with other open clusters
examined for mass segregation
examined for the effects of tidal forces
investigated for age determination
investigated for mass loss in stars
investigated for the presence of dark matter
mapped for spatial distribution of stars
monitored for supernova remnants
monitored for variable stars
observed for binary star systems
studied for stellar interactions
studied for the presence of exoplanets
used in simulations of cluster evolution
used in studies of cluster dynamics
gptkbp:right_ascension 10h 36m 00s
10h 38m 30s
10h 36m 30s
gptkbp:size approximately 10 arcminutes
gptkbp:type gptkb:star
young star cluster
young open cluster
gptkbp:year_created 1834