Epsilon Aurigae

GPTKB entity

Statements (48)
Predicate Object
gptkbp:instance_of gptkb:star
gptkbp:age approximately 3 million years
gptkbp:apparent_magnitude 3.7
gptkbp:average_temperature approximately 7000 K
gptkbp:catalog_designation HR 2028
gptkbp:collection data collected over centuries
gptkbp:companion_type B-type star
gptkbp:constellation gptkb:Auriga
gptkbp:contains_star classified as a binary star system
similar to other eclipsing binaries
gptkbp:discovery_year 1821
gptkbp:distance 2000 light years
gptkbp:eclipse_frequency every 27.1 years
gptkbp:eclipsing_nature characterized by periodic eclipses
gptkbp:field_of_study astrophysics
gptkbp:first_appearance by John Herschel
gptkbp:has_bayer_designation gptkb:ε_Aurigae
gptkbp:has_luminosity approximately 1000 solar luminosities
gptkbp:has_radius approximately 20 solar radii
gptkbp:has_spectral_type F0
gptkbp:has_title gptkb:HIP_23312
gptkbp:historical_significance one of the first binary stars discovered
https://www.w3.org/2000/01/rdf-schema#label Epsilon Aurigae
gptkbp:is_observed_in various telescopes
gptkbp:lighting 0.5 magnitudes
analyzed for periodicity
complex light curve due to eclipses
periodic variability due to eclipses
gptkbp:mass approximately 10 solar masses
gptkbp:metallicity solar metallicity
gptkbp:module approximately 2 years
gptkbp:notable_feature long-duration eclipses
gptkbp:notable_work studied for its unique eclipsing nature
gptkbp:number gptkb:HD_31964
gptkbp:orbital_period 27.1 years
gptkbp:parallax 0.0016 arcseconds
gptkbp:primary_component gptkb:Epsilon_Aurigae_A
gptkbp:research observed in various wavelengths
subject of numerous studies
difficult to observe during eclipses
utilizes photometry and spectroscopy
gptkbp:research_importance helps study stellar evolution
gptkbp:rotation_period approximately 10 days
gptkbp:secondary_component gptkb:Epsilon_Aurigae_B
gptkbp:system gptkb:star
gptkbp:type eclipsing binary star
gptkbp:bfsParent gptkb:Auriga
gptkbp:bfsLayer 6