HD 93250

GPTKB entity

Statements (35)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age approximately 2 million years
gptkbp:average_temperature approximately 40,000 K
gptkbp:constellation gptkb:Carina
gptkbp:contains_star gptkb:HD_93250_A
gptkb:HD_93250_B
gptkb:Milky_Way
O3 V: (n)
gptkbp:discovery discovered in the 19th century
gptkbp:distance approximately 5,500 light years
gptkbp:distance_from_earth 5,000 light years
gptkbp:has_companion gptkb:HD_93250_B
gptkbp:has_luminosity approximately 100,000 times that of the Sun
gptkbp:has_spectral_type O3 V
https://www.w3.org/2000/01/rdf-schema#label HD 93250
gptkbp:is_associated_with gptkb:Carina_Nebula
gptkbp:is_located_in gptkb:Carina_constellation
gptkbp:is_notable_for massive stars
gptkbp:is_part_of gptkb:open_cluster
gptkb:Milky_Way_galaxy
gptkbp:is_studied_in astrophysics
gptkbp:is_visible_from yes
gptkbp:lighting magnitude 8.5
gptkbp:location near the Carina Nebula
gptkbp:losses high mass loss rate due to stellar winds
gptkbp:mass approximately 50 times that of the Sun
gptkbp:massive_star one of the most massive stars known
gptkbp:notable_feature part of the Trumpler 14 cluster
gptkbp:originated_in gptkb:main-sequence_star
gptkbp:research observed through photometry and spectroscopy
gptkbp:role contributes to the ionization of surrounding nebulae
gptkbp:type O-type star
gptkbp:variable_star not classified as a variable star
gptkbp:bfsParent gptkb:Trumpler_16
gptkbp:bfsLayer 5