47 Canum Venaticorum A

GPTKB entity

Statements (51)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age approximately 3 billion years
gptkbp:apparent_magnitude 5.56
gptkbp:average_temperature 5800 K
gptkbp:composed_of hydrogen and helium
gptkbp:conducts_research_on stellar dynamics
stellar evolution studies
gptkbp:distance_from_earth 50.0 light years
gptkbp:eccentricity 0.3
gptkbp:exhibition Hipparcos catalog
gptkbp:has_color 0.5
gptkbp:has_companion 47 Canum Venaticorum B
gptkbp:has_luminosity 1.5 solar luminosities
gptkbp:has_mechanic -0.12 arcseconds/year
-0.15 arcseconds/year
gptkbp:has_radius 1.2 solar radii
gptkbp:has_spectral_type G0 V
https://www.w3.org/2000/01/rdf-schema#label 47 Canum Venaticorum A
gptkbp:impact binary star interactions
gptkbp:included star catalogs
gptkbp:investigates stellar population studies
gptkbp:is_analyzed_in stellar activity
gptkbp:is_associated_with Canes Venatici constellation
gptkbp:is_considered_as potential host for exoplanets
gptkbp:is_examined_in stellar astrophysics
habitable zone calculations
gptkbp:is_inhabited_by exoplanets (potentially)
gptkbp:is_known_for being a binary star system
gptkbp:is_located_in gptkb:Milky_Way_galaxy
gptkbp:is_located_near 50 light years from Earth
gptkbp:is_monitored_by gptkb:astronomy
gptkbp:is_observed_in telescopes
light curve analysis
gptkbp:is_part_of gptkb:star
Canes Venatici constellation
gptkbp:is_part_of_astrophysical_models stellar formation theories
gptkbp:is_related_to stellar classification
gptkbp:is_studied_for stellar mass determination
gptkbp:is_studied_in astrophysics
gptkbp:is_used_in stellar evolution models
gptkbp:is_visible_from gptkb:true
northern hemisphere
gptkbp:mass 1.1 solar masses
gptkbp:metallicity solar metallicity
gptkbp:orbital_period approximately 10 years
gptkbp:parallax 0.065 arcseconds
gptkbp:rotation_period approximately 25 days
gptkbp:surface 4.4 m/s²
gptkbp:system gptkb:true
47 Canum Venaticorum B
gptkbp:type_of gptkb:main-sequence_star