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Eta Persei (η Persei, abbreviated Eta Per, η Per), is a binary star and the 'A' component of a triple star system (the 'B' component is the star HD 237009) [8] in the constellation of Perseus. Parallax measurements by the Gaia spacecraft imply that it is 1,000 is light-years away from Earth. [1]
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Sirius, one of the brightest stars in the sky, is a binary system involving one dominant bluish component and a less dominant secondary component. A number of binaries have their component stars being of different colors which makes for very attractive photos (see below).
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5 sie 2012 · In this image, Algol is the bright blue star and Rho Persei is the bright red star. Algol (beta-Persei, SAO 38592) also known as the " Demon Star " is an eclipsing binary star , so an orbiting star eclipses Algol causing its magnitude to change from a relatively bright 2.1 to a much dimmer 3.4, every 2 days 20 hours and 49 minutes.
It is the fourth brightest star in Perseus. Gamma Persei is composed of a giant of the spectral type G9 III and a companion star which is usually classified either as A3V or A2III. The system is a wide eclipsing binary star, with the two stars orbiting each other every 14.6 years.
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