Statements (40)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:age |
approximately 3 million years
|
| gptkbp:category |
a variable star
|
| gptkbp:climate |
approximately 7000 K
|
| gptkbp:component |
Epsilon_Aurigae_A
Epsilon_Aurigae_B |
| gptkbp:diameter |
approximately 20 solar radii
|
| gptkbp:hasDepartment |
yes
|
| gptkbp:hasFeature |
extensively studied spectroscopically
|
| gptkbp:hasHistoricalSignificance |
documented by various astronomers
important for understanding binary stars |
| gptkbp:hasRecognition |
3.7
|
| gptkbp:hasVariants |
yes
|
| gptkbp:historicalEvent |
studied since the 19th century
|
| https://www.w3.org/2000/01/rdf-schema#label |
Epsilon Aurigae
|
| gptkbp:isAccessibleBy |
yes
|
| gptkbp:isFiledIn |
+0.5
|
| gptkbp:isKnownFor |
its long period of eclipses
|
| gptkbp:isLocatedIn |
northern celestial hemisphere
|
| gptkbp:isNotableFor |
its unique light curve
|
| gptkbp:isPartOf |
Milky Way Galaxy
stellar dynamics the_Auriga_constellation |
| gptkbp:isServedBy |
amateur astronomers
|
| gptkbp:isStudiedIn |
astrophysics
|
| gptkbp:isUsedIn |
stellar modeling
|
| gptkbp:length |
2000 light years
|
| gptkbp:lighting |
approximately 1000 solar luminosities
complex due to multiple components due to eclipses |
| gptkbp:mission |
no known exoplanets
|
| gptkbp:notableFeature |
long orbital period
used to study stellar evolution by_John_Herschel |
| gptkbp:orbitalInclination |
27.1 years
|
| gptkbp:releaseYear |
1821
|
| gptkbp:type |
F0
eclipsing binary star |
| gptkbp:vision |
gptkb:Auriga
|
| gptkbp:weight |
approximately 10 solar masses
|