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Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at...

Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top,
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Largest available format 2700 × 3375 px 3 MB
Dimension [pixels] Dimension in 300dpi [mm] File size [MB] Online Purchase
Large 2700 × 3375 px 229 × 286 mm 3.3 MB
Medium 819 × 1024 px 69 × 87 mm 1.6 MB

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IMAGE number
PIX4589805
Image title
Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top, the bright star is the polar star. Cepheus is a representation of King Cepheus of Ethiopia, who has stellar connections, being husband to Cassiopeia and the father of Andromeda. It is a large northern constellation of 588 square degrees, 27th out of 88 in size and is best seen in the early evening in November. It is distinguished by having two unusual stars that are easily seen. Delta Cephei is the prototype for an intrinsically bright class of regularly pulsating variable stars whose period of variability is closely related to their absolute magnitudes. The brightest stars have the longest period, so distance can be estimated by measuring the period and the apparent magnitude of a star. And these stars are bright, so the method can be extended to nearby galaxies. Mu (u) Cephei is an extremely red, irregular variable star easily seen in binoculars. This too is a prototype, of a class of stars known as semi - regular variables
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Cephee Constellation - Constellation of Cepheus - At the bottom left, the constellation Cassiopee; at the top, the bright star is the polar star. Cepheus is a representation of King Cepheus of Ethiopia, who has stellar connections, being husband to Cassiopeia and the father of Andromeda. It is a large northern constellation of 588 square degrees, 27th out of 88 in size and is best seen in the early evening in November. It is distinguished by having two unusual stars that are easily seen. Delta Cephei is the prototype for an intrinsically bright class of regularly pulsating variable stars whose period of variability is closely related to their absolute magnitudes. The brightest stars have the longest period, so distance can be estimated by measuring the period and the apparent magnitude of a star. And these stars are bright, so the method can be extended to nearby galaxies. Mu (u) Cephei is an extremely red, irregular variable star easily seen in binoculars. This too is a prototype, of a class of stars known as semi - regular variables

Photo credit
Photo © A.Fujii/David Malin Images/Novapix / Bridgeman Images
Image keywords
astronomy / card / star / constellation / astronomy / polaris / sky map / mark / mail / star / Novapix / astronomy / Laced Track / milky way / Cepheide / Fleece Star / cepheid / pole star / Star variable / nebula / nebula / cassiopee / cassiopeia / line / map / North Celestial Pole / cephee / cepheus / ic 1396

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