|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:bfsLayer
|
4
|
|
gptkbp:bfsParent
|
gptkb:Canis_Major
|
|
gptkbp:analyzes
|
stellar activity
|
|
gptkbp:apparent_magnitude
|
6.2
|
|
gptkbp:contains
|
gptkb:HD_89500_A
gptkb:HD_89500_B
|
|
gptkbp:controls
|
gptkb:theorem
|
|
gptkbp:depicted_in
|
gptkb:theorem
|
|
gptkbp:discovered_by
|
the 19th century
|
|
gptkbp:distance
|
approximately 100 light years from Earth
|
|
gptkbp:examines
|
stellar interactions
|
|
gptkbp:game_components
|
two stars
|
|
gptkbp:has_color
|
0.1
|
|
gptkbp:has_spectral_type
|
A0 V and B0 V
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
HD 89500
|
|
gptkbp:includes
|
star catalogs
|
|
gptkbp:is_analyzed_in
|
stellar composition
|
|
gptkbp:is_associated_with
|
stellar populations
|
|
gptkbp:is_considered
|
theories of star formation
|
|
gptkbp:is_discussed_in
|
astronomical catalogs
|
|
gptkbp:is_explored_in
|
gptkb:planet
|
|
gptkbp:is_known_for
|
its binary nature
|
|
gptkbp:is_noted_for
|
its brightness
|
|
gptkbp:is_observed_in
|
telescopes
various wavelengths
|
|
gptkbp:is_part_of
|
gptkb:Milky_Way_galaxy
multiple star system
astrophysical simulations
stellar surveys
|
|
gptkbp:is_referenced_in
|
astronomical literature
|
|
gptkbp:is_related_to
|
stellar dynamics
|
|
gptkbp:is_studied_in
|
astrophysics
|
|
gptkbp:is_used_for
|
distance measurement
|
|
gptkbp:is_used_in
|
stellar classification studies
|
|
gptkbp:is_utilized_in
|
stellar evolution models
|
|
gptkbp:located_in
|
constellation Centaurus
|
|
gptkbp:orbital_period
|
about 1000 years
|
|
gptkbp:research
|
stellar evolution
star formation
|
|
gptkbp:scientific_classification
|
gptkb:star
|
|
gptkbp:subject
|
gptkb:Research_Institute
|