gptkbp:instance_of
|
gptkb:star
|
gptkbp:age
|
5 billion years
nan
|
gptkbp:apparent_magnitude
|
5.5
5.57
|
gptkbp:average_temperature
|
around 5,200 K
around 5,300 K
|
gptkbp:constellation
|
gptkb:Canes_Venatici
|
gptkbp:contains_star
|
yes
nan
|
gptkbp:coordinates
|
+200.1 degrees
+60.2 degrees
|
gptkbp:country
|
nan
|
gptkbp:distance
|
5.5
|
gptkbp:exhibition
|
the Henry Draper Catalogue
|
gptkbp:has_henry_draper_designation
|
gptkb:HD_100453
|
gptkbp:has_luminosity
|
about 1.5 times that of the Sun
about 60 times that of the Sun
|
gptkbp:has_mechanic
|
-0.020 arcseconds/year
|
gptkbp:has_radius
|
about 10 times that of the Sun
about 1.2 solar radii
|
gptkbp:has_spectral_type
|
G8 III
G-type stars
G8 V
|
gptkbp:has_supernova
|
yes
|
gptkbp:head_of_state
|
nan
|
https://www.w3.org/2000/01/rdf-schema#label
|
93 Canum Venaticorum
|
gptkbp:is_a_candidate_for_a_supernova_progenitor
|
nan
|
gptkbp:is_a_member_of
|
local stellar population
|
gptkbp:is_a_part_of_the_milky_way's_stellar_population
|
nan
|
gptkbp:is_a_part_of_the_stellar_evolution_process
|
nan
|
gptkbp:is_a_part_of_the_stellar_kinematics_research
|
nan
|
gptkbp:is_a_part_of_the_stellar_lifecycle_studies
|
nan
|
gptkbp:is_a_part_of_the_stellar_population
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_atmospheres_in_giant_stars
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_chemical_evolution
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_clusters
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_dynamics_in_galaxies
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_binary_systems
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_different_stellar_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_galactic_dynamics
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_observational_studies_in_astronomy
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_observational_studies_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_classification_criteria
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_classification_criteria_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_dynamics_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_dynamics_in_galaxies
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_formation
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_formation_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_interactions
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_interactions_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_magnetic_fields
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_magnetic_fields_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_nucleosynthesis
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_photometry
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_photometry_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_populations_in_the_milky_way
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_in_the_context_of_stellar_populations_in_the_milky_way_in_different_environments
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_evolution_pathways
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_formation
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_interactions
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_interactions_in_binary_systems
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_magnetic_fields
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_mass_distribution
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_mass_loss
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_nucleosynthesis
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_populations
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_populations_in_galaxies
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_populations_in_the_milky_way
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_rotation
|
nan
|
gptkbp:is_a_part_of_the_study_of_stellar_variability
|
nan
|
gptkbp:is_a_reference_for_stellar_atmosphere_models
|
nan
|
gptkbp:is_a_reference_for_stellar_classification_criteria
|
nan
|
gptkbp:is_a_reference_for_stellar_classification_systems
|
nan
|
gptkbp:is_a_reference_for_stellar_distance_measurements
|
nan
|
gptkbp:is_a_reference_for_stellar_distances
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_dynamics
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_evolution_scenarios
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_evolution_scenarios_in_different_environments
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_interactions_in_binary_systems
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_interactions_in_different_environments
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_mass_loss
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_populations
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_rotation
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_stellar_rotation_in_different_environments
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_in_the_context_of_the_milky_way
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_models
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_models_in_g-type_stars
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_scenarios
|
nan
|
gptkbp:is_a_reference_for_stellar_evolution_theories
|
nan
|
gptkbp:is_a_reference_for_stellar_models
|
nan
|
gptkbp:is_a_reference_point_for_stellar_classification
|
nan
|
gptkbp:is_a_source_of_stellar_wind
|
nan
|
gptkbp:is_a_subject_of_astrobiology_research
|
nan
|
gptkbp:is_a_subject_of_astrophysical_research
|
nan
|
gptkbp:is_a_subject_of_galactic_dynamics_studies
|
nan
|
gptkbp:is_a_subject_of_galactic_structure_research
|
nan
|
gptkbp:is_a_subject_of_observational_astronomy
|
nan
|
gptkbp:is_a_subject_of_observational_studies_in_astronomy
|
nan
|
gptkbp:is_a_subject_of_photometric_studies
|
nan
|
gptkbp:is_a_subject_of_research_in_galactic_astronomy
|
nan
|
gptkbp:is_a_subject_of_research_in_stellar_astrophysics
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_astrophysics
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_chemical_evolution
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_dynamics
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_evolution_in_different_environments
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_evolution_in_different_environments_in_different_environments
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_evolution_in_the_context_of_stellar_nucleosynthesis
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_mass_distribution
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_mass_distribution_in_different_environments
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_population_synthesis
|
nan
|
gptkbp:is_a_subject_of_research_in_the_field_of_stellar_population_synthesis_in_different_environments
|
nan
|
gptkbp:is_a_subject_of_stellar_dynamics_research
|
nan
|
gptkbp:is_a_subject_of_stellar_photometry
|
nan
|
gptkbp:is_a_subject_of_stellar_population_synthesis
|
nan
|
gptkbp:is_a_subject_of_theoretical_astrophysics
|
nan
|
gptkbp:is_a_target_for_spectroscopy
|
nan
|
gptkbp:is_approximately
|
50 light years away from Earth
50 light years away
|
gptkbp:is_associated_with_the_galactic_halo
|
nan
|
gptkbp:is_classified_as_a_yellow_giant
|
nan
|
gptkbp:is_involved_in_stellar_evolution_studies
|
nan
|
gptkbp:is_involved_in_the_study_of_stellar_atmospheres
|
nan
|
gptkbp:is_listed_in_the
|
gptkb:Hipparcos_Catalogue
|
gptkbp:is_located_in
|
gptkb:Canes_Venatici
Canes Venatici constellation
|
gptkbp:is_not_a_brown_dwarf
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_a
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_b
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_f
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_k
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_m
|
yes
|
gptkbp:is_not_a_main-sequence_star_of_type_o
|
yes
|
gptkbp:is_not_a_pulsar
|
yes
|
gptkbp:is_not_a_red_dwarf
|
yes
|
gptkbp:is_not_a_supernova_remnant
|
yes
|
gptkbp:is_not_known_to_have_any_planets
|
yes
|
gptkbp:is_observed_in
|
gptkb:Hubble_Space_Telescope
|
gptkbp:is_often_described_as
|
HR 4703
|
gptkbp:is_part_of
|
gptkb:Milky_Way_galaxy
Galactic disk
solar neighborhood
Canes Venatici constellation group
|
gptkbp:is_part_of_the_galactic_disk
|
nan
|
gptkbp:is_part_of_the_hipparcos_catalogue
|
gptkb:HIP_56334
|
gptkbp:is_studied_for_its_chemical_composition
|
nan
|
gptkbp:is_used_in_astronomical_studies
|
nan
|
gptkbp:is_used_in_distance_measurement_techniques
|
nan
|
gptkbp:is_visible_from
|
yes
northern hemisphere
nan
|
gptkbp:isotopes
|
yes
|
gptkbp:mass
|
yes
nan
about 2 times that of the Sun
about 1.1 solar masses
|
gptkbp:metallicity
|
approximately solar
around solar metallicity
|
gptkbp:notable_galaxies
|
nan
|
gptkbp:notable_person
|
yes
|
gptkbp:right_ascension
|
-0.045 arcseconds/year
|
gptkbp:rotation_period
|
about 25 days
about 30 days
|
gptkbp:scientific_classification
|
a yellow dwarf star
|
gptkbp:system
|
yes
nan
|
gptkbp:targets
|
stellar evolution studies
|
gptkbp:type_of
|
gptkb:main-sequence_star
|