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physical object > natural object > celestial body > star > variable > periodic variable > beta Cephei star |
beta Cephei star (beta Canis Majoris star) | ||||
subject | fact |
beta Cephei star | has period P = 3.5 to 6 hr | |
has prototype beta Cephei | ||
has spectral type O9-B3 | ||
has synonym beta Canis Majoris star | ||
has definition A small group of short-period pulsating variables lying slightly above the upper main sequence. They have a doubly periodic light curve, and are confined within a narrow band of the H-R diagram which lies near the end of core hydrogen-burning stars of roughly 10-20 Msun. beta Cephei itself has at least three components. | ||
is a kind of periodic variable | ||
variable | has name designated with
| |
has observational problem some difficulty in distinguishing between various kinds | ||
has observable variation time scale within a period of decades | ||
has light curve | ||
has optical brightness variation 0.2 magnitudes or greater | ||
has amplitude | ||
star | has star surface temperature | |
has V magnitude | ||
has B magnitude | ||
has U magnitude | ||
has position on celestial sphere from the point of view of Earth | ||
has parallax from the point of view of Earth's orbit | ||
has proper motion | ||
has radiation at surface which is diffused out from the hotter core | ||
has energy source gravitational contraction and or fusion | ||
has energy production which takes place primarily within the core | ||
has surface density which depends on luminosity class | ||
has surface temperature greater than 1000 Kelvin | ||
has apparent magnitude | ||
has absolute magnitude | ||
has age | ||
has catalog star catalog | ||
has material hydrogen, helium | ||
has velocity determined from proper motion and radial velocity | ||
has mass greater than 0.08 the sun's mass | ||
celestial body | has spectra | |
physical object | has location or center of gravity | |
has angular momentum | ||
has momentum | ||
has temperature | ||
has volume | ||
has extent |
Kinds of beta Cephei star :
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