gptkbp:instance_of
|
gptkb:star
|
gptkbp:apparent_magnitude
|
5.5
5.57
|
gptkbp:average_temperature
|
around 5,200 K
|
gptkbp:conducts_research_on
|
stellar evolution
|
gptkbp:constellation
|
gptkb:Canes_Venatici
|
gptkbp:contains_star
|
gptkb:none
gptkb:83_Canum_Venaticorum_B
|
gptkbp:distance
|
approximately 50 light years
|
gptkbp:eccentricity
|
0.3
|
gptkbp:has_bayer_designation
|
gptkb:none
|
gptkbp:has_color
|
0.67
|
gptkbp:has_henry_draper_designation
|
gptkb:HD_100453
|
gptkbp:has_historical_significance
|
noted in ancient star catalogs
|
gptkbp:has_luminosity
|
1.5 times that of the Sun
about 60 times that of the Sun
|
gptkbp:has_mechanic
|
-0.020 arcseconds/year
-0.045 arcseconds/year
|
gptkbp:has_radius
|
approximately 11 solar radii
|
gptkbp:has_spectral_type
|
G8 III
G5 V
|
gptkbp:has_title
|
gptkb:HIP_56334
|
https://www.w3.org/2000/01/rdf-schema#label
|
83 Canum Venaticorum
|
gptkbp:included
|
star catalogs
|
gptkbp:is_a
|
gptkb:Giant
|
gptkbp:is_analyzed_in
|
stellar atmospheres
|
gptkbp:is_approximately
|
50 light years away
|
gptkbp:is_associated_with
|
mythology of Canes Venatici
|
gptkbp:is_known_for
|
its brightness
|
gptkbp:is_located_in
|
gptkb:Canes_Venatici
|
gptkbp:is_mentioned_in
|
astronomical catalogs
|
gptkbp:is_noted_for
|
being a binary star system
|
gptkbp:is_observed_in
|
space telescopes
ground-based telescopes
stellar activity
|
gptkbp:is_part_of
|
gptkb:star
gptkb:Milky_Way
a binary star system
|
gptkbp:is_part_of_astrophysical_models
|
stellar evolution models
|
gptkbp:is_part_of_research_field
|
exoplanet studies
|
gptkbp:is_related_to
|
other G-type stars
|
gptkbp:is_studied_for
|
stellar dynamics
|
gptkbp:is_studied_in
|
astrophysics
|
gptkbp:is_used_for
|
navigational purposes
|
gptkbp:is_used_in
|
stellar classification studies
|
gptkbp:is_visible_from
|
yes
northern hemisphere
|
gptkbp:known_as
|
gptkb:HD_100453
|
gptkbp:mass
|
about 2.5 solar masses
1.1 times that of the Sun
|
gptkbp:number
|
Gl 1234
|
gptkbp:orbital_inclination
|
approximately 60 degrees
|
gptkbp:orbital_period
|
about 1000 days
|
gptkbp:scientific_classification
|
a main-sequence star
field star
|