83 Canum Venaticorum A

GPTKB entity

Statements (47)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age approximately 4.5 billion years
gptkbp:apparent_magnitude 5.57
gptkbp:average_temperature approximately 5800 K
gptkbp:composed_of solar metallicity
gptkbp:contains_star gptkb:83_Canum_Venaticorum_B
gptkbp:coordinates approximately -30 degrees
approximately 200 degrees
l = 150°, b = -30°
gptkbp:discovery_year discovered in 1830
gptkbp:distance approximately 50 light years
gptkbp:element determined through astrometry
gptkbp:exhibition gptkb:Henry_Draper_catalog
Hipparcos catalog
Gliese catalog
gptkbp:has_color 0.6
gptkbp:has_historical_significance notable for binary star studies
gptkbp:has_luminosity 1.3 solar luminosities
gptkbp:has_magnitude_difference 1.5 between A and B
gptkbp:has_mechanic -0.020 arcseconds/year
-0.045 arcseconds/year
gptkbp:has_radius 1.1 solar radii
gptkbp:has_spectral_type G5 V
gptkbp:has_title gptkb:83_Canum_Venaticorum_A
https://www.w3.org/2000/01/rdf-schema#label 83 Canum Venaticorum A
gptkbp:is_associated_with gptkb:exoplanet
gptkbp:is_located_in gptkb:Milky_Way_galaxy
the northern celestial hemisphere
gptkbp:is_noted_for its binary nature
gptkbp:is_observed_in space telescopes
various wavelengths
ground-based telescopes
gptkbp:is_part_of gptkb:star
multiple star system
Canes Venatici constellation
gptkbp:is_related_to stellar dynamics
gptkbp:is_studied_in astrophysics
gptkbp:is_used_in stellar evolution models
gptkbp:is_visible_from gptkb:true
visible to the naked eye
gptkbp:mass 1.1 solar masses
gptkbp:orbital_inclination approximately 45 degrees
gptkbp:orbital_period approximately 1000 days
gptkbp:parallax 0.065 arcseconds
gptkbp:speed -10 km/s
gptkbp:system gptkb:true
gptkbp:type_of gptkb:main-sequence_star