|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:age
|
1 billion years
nan
|
|
gptkbp:apparent_magnitude
|
5.5
|
|
gptkbp:average_temperature
|
around 5000 K
|
|
gptkbp:composed_of
|
primarily hydrogen and helium
|
|
gptkbp:constellation
|
gptkb:Canes_Venatici
|
|
gptkbp:contains_star
|
gptkb:88_Canum_Venaticorum_B
no
|
|
gptkbp:distance
|
approximately 100 light years
|
|
gptkbp:has_bayer_designation
|
gptkb:Beta_Canum_Venaticorum
|
|
gptkbp:has_color
|
0.75
|
|
gptkbp:has_henry_draper_designation
|
gptkb:HD_100453
|
|
gptkbp:has_luminosity
|
about 50 times that of the Sun
|
|
gptkbp:has_mechanic
|
-0.01 arcseconds/year
-0.02 arcseconds/year
|
|
gptkbp:has_radius
|
about 10 times that of the Sun
approximately 11 solar radii
|
|
gptkbp:has_spectral_type
|
G8 III
|
|
gptkbp:has_title
|
gptkb:HIP_56307
|
|
gptkbp:has_variations
|
not variable
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
88 Canum Venaticorum
|
|
gptkbp:is_a
|
gptkb:Giant
|
|
gptkbp:is_approximately
|
60 light years away
|
|
gptkbp:is_associated_with
|
Canes Venatici constellation
|
|
gptkbp:is_displayed_in
|
gptkb:NASA_Exoplanet_Archive
|
|
gptkbp:is_in_catalog
|
gptkb:Bright_Star_Catalog
|
|
gptkbp:is_known_for
|
being a binary star system
|
|
gptkbp:is_located_in
|
gptkb:Canes_Venatici
|
|
gptkbp:is_moving_away_from_earth
|
gptkb:true
|
|
gptkbp:is_noted_for
|
its brightness
|
|
gptkbp:is_observed_in
|
amateur astronomers
|
|
gptkbp:is_part_of
|
gptkb:Milky_Way
|
|
gptkbp:is_part_of_sky_survey
|
gptkb:SDSS
|
|
gptkbp:is_studied_in
|
stellar astrophysics
|
|
gptkbp:is_used_in
|
stellar navigation
|
|
gptkbp:is_visible_from
|
gptkb:true
northern hemisphere
|
|
gptkbp:mass
|
about 2.5 solar masses
nan
about 2 times that of the Sun
|
|
gptkbp:number
|
gptkb:Gl_1233
|
|
gptkbp:orbital_period
|
about 1000 years
|
|
gptkbp:redshift
|
0.0001
|
|
gptkbp:scientific_classification
|
G-type star
|