76 Canum Venaticorum

GPTKB entity

Statements (48)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age gptkb:the_Sun
gptkbp:apparent_magnitude 5.5
5.56
gptkbp:average_temperature around 5,800 K
gptkbp:constellation gptkb:Canes_Venatici
gptkbp:contains_star gptkb:true
nan
gptkbp:coordinates +200.0 degrees
+50.0 degrees
gptkbp:distance about 5.5
gptkbp:has_a_proper_motion_in_dec -0.15 arcseconds/year
gptkbp:has_a_proper_motion_in_ra +0.12 arcseconds/year
gptkbp:has_color +0.65
gptkbp:has_luminosity about 1.5 times that of the Sun
gptkbp:has_radius 1.4 solar radii
about 1.2 solar radii
gptkbp:has_spectral_type F7 V
G5 V
https://www.w3.org/2000/01/rdf-schema#label 76 Canum Venaticorum
gptkbp:is_a_member_of gptkb:the_Milky_Way_galaxy
Galactic disk
gptkbp:is_a_relatively_stable_star nan
gptkbp:is_a_source_of stellar radiation
gptkbp:is_approximately 60 light years away from Earth
50 light years away
gptkbp:is_located_in gptkb:Canes_Venatici
the constellation Canes Venatici
gptkbp:is_not_known_to_have_any_planets nan
gptkbp:is_often_described_as gptkb:76_CVn
gptkbp:is_part_of gptkb:Hertzsprung-Russell_diagram
gptkb:Milky_Way_galaxy
solar neighborhood
Canes Venatici constellation group
local stellar population
gptkbp:is_studied_in stellar activity
gptkbp:is_used_in astrophysical research
gptkbp:is_visible_from northern hemisphere
under good conditions
gptkbp:mass about 1.1 solar masses
1.3 solar masses
gptkbp:metallicity similar to the Sun
gptkbp:rotation_period approximately 25 days
gptkbp:scientific_classification a yellow dwarf star
gptkbp:system nan
gptkbp:targets stellar evolution studies
gptkbp:type_of gptkb:main-sequence_star
gptkbp:was_first_cataloged_in the 19th century