83 Canum Venaticorum

GPTKB entity

Statements (55)
Predicate Object
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