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physical object > natural object > celestial body > collection of stars > star system > binary star > close binary > eclipsing binary > epsilon Aurigae
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epsilon Aurigae
subjectfact 
epsilon Aurigaehas primary A8 Ia2001-09-27 09:30:36.0
has distance 1 kpchas source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:30:36.0
is a part of Auriga2001-09-27 09:30:36.0
has orbital period 27 yearshas source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:30:36.0
has definition An eclipsing binary with an invisible supergiant companion. The primary is an extremely luminous A8 Ia supergiant of 30 Msun in a post-main-sequence stage of evolution; the secondary may be a collapsed star or black hole. It has at least six components.has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:30:36.0
is an instance of white supergiant2001-09-27 09:30:36.0
is an instance of eclipsing binary2001-09-27 09:30:36.0
eclipsing binaryhas eclipse duration2001-09-27 09:30:35.0
periodic variablehas period2001-09-27 09:30:34.0
A starhas color white2001-09-27 09:30:46.0
has surface temperature 10000 K2001-09-27 09:30:46.0
has absorption line H I2001-09-27 09:30:46.0
binary starhas number of stars 22001-09-27 09:30:54.0
variablehas name designated with
  1. R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
  2. RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
  3. AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
  4. V 335, V 336, etc., when the double letter designations are exhausted
2001-09-27 09:30:34.0
has observational problem some difficulty in distinguishing between various kinds2001-09-27 09:30:34.0
has observable variation time scale within a period of decadeshas URL: http://www.aavso.org, 2001-09-27 09:30:34.0
has light curve2001-09-27 09:30:34.0
has optical brightness variation 0.2 magnitudes or greater2001-09-27 09:30:34.0
has amplitude2001-09-27 09:30:34.0
early starhas spectral type O, B, A, and early F2001-09-27 09:30:44.0
star systemhas abundance half the stars in the solar neighborhood are members of star systems2001-09-27 09:30:54.0
starhas star surface temperature2001-09-27 09:30:25.0
has V magnitude2001-09-27 09:30:25.0
has B magnitude2001-09-27 09:30:25.0
has U magnitude2001-09-27 09:30:25.0
has position on celestial sphere from the point of view of Earth2001-09-27 09:30:25.0
has parallax from the point of view of Earth's orbit2001-09-27 09:30:25.0
has proper motion2001-09-27 09:30:24.0
has radiation at surface which is diffused out from the hotter core2001-09-27 09:30:24.0
has energy source gravitational contraction and or fusion2001-09-27 09:30:24.0
has energy production which takes place primarily within the core2001-09-27 09:30:24.0
has surface density which depends on luminosity class2001-09-27 09:30:24.0
has apparent magnitude2001-09-27 09:30:25.0
has absolute magnitude2001-09-27 09:30:25.0
has age2001-09-27 09:30:25.0
has catalog star catalog2001-09-27 09:30:25.0
has material hydrogen, helium2001-09-27 09:30:24.0
has velocity determined from proper motion and radial velocity2001-09-27 09:30:25.0
has mass greater than 0.08 the sun's mass2001-09-27 09:30:24.0
celestial bodyhas spectra2001-09-27 09:30:09.0
physical objecthas location or center of gravity2001-09-27 09:27:27.0
has angular momentum2001-09-27 09:27:27.0
has momentum2001-09-27 09:27:27.0
has temperature2001-09-27 09:27:27.0
has volume2001-09-27 09:27:27.0
has extent2001-09-27 09:27:27.0

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