The Algol star system is known as an eclipsing binary pair, As such, one star moves in front of the other, blocking it's light. Because the pair are in line with the Earth, it has the effect that one stars seems to disappear.
See related link for an animation of the effect.
Algol is a binary star system located approximately 93 light-years away from Earth. The primary star, Algol A, is a blue-white subgiant star with around 3 times the mass of the Sun, while the secondary star, Algol B, is a smaller main sequence star. The system has a combined apparent magnitude of about 2.1, making it one of the brightest stars in the night sky.
Algol (Demon Star) is a bright star in the constellation Perseus.Algol is actually a triple star system - Beta Persei A, B, and CBeta Persei A has a spectral type of B8 and is a blue-white giantBeta Persei B has a spectral type of K0 and is an orange subgiantSee related link for more information.
No, Algol and Mira are different astronomical objects. Algol is a binary star system located in the constellation Perseus, while Mira is a red giant star in the constellation Cetus. Both are variable stars, but they are not related astronomically.
There are no known planets located near the star Algol, which is a binary star system consisting of two stars. The distance between the two stars is relatively close, making it difficult for planets to stably orbit either of the stars.
Algol is a binary star system composed of two stars orbiting each other. The dimming and brightening of Algol occur when the dimmer star passes in front of the brighter star from our point of view, resulting in an eclipse. This regular change in brightness is known as an eclipsing binary system.
Algol is in the constellation Perseus.
Algol is a bright three-star system that is part of the constellation Perseus. Other names for Algol are Demon Star, Gorgona, and El Ghoul.
algol
Sirius is larger than Algol. Sirius is a binary star system with Sirius A being the larger star with about twice the mass of the Sun, while Algol is a triple star system with the main star being smaller than Sirius A.
Algol is a binary star system located approximately 93 light-years away from Earth. The primary star, Algol A, is a blue-white subgiant star with around 3 times the mass of the Sun, while the secondary star, Algol B, is a smaller main sequence star. The system has a combined apparent magnitude of about 2.1, making it one of the brightest stars in the night sky.
Algol (Demon Star) is a bright star in the constellation Perseus.Algol is actually a triple star system - Beta Persei A, B, and CBeta Persei A has a spectral type of B8 and is a blue-white giantBeta Persei B has a spectral type of K0 and is an orange subgiantSee related link for more information.
No, Algol and Mira are different astronomical objects. Algol is a binary star system located in the constellation Perseus, while Mira is a red giant star in the constellation Cetus. Both are variable stars, but they are not related astronomically.
Algol is a blue main-sequence star in the constellation Perseus
There are no known planets located near the star Algol, which is a binary star system consisting of two stars. The distance between the two stars is relatively close, making it difficult for planets to stably orbit either of the stars.
Algol is a binary star system composed of two stars orbiting each other. The dimming and brightening of Algol occur when the dimmer star passes in front of the brighter star from our point of view, resulting in an eclipse. This regular change in brightness is known as an eclipsing binary system.
Algol is best classified as a fixed star system in the constellation Perseus. It is actually a binary star system consisting of two stars that eclipse each other from the perspective of Earth. It is one of the best-known eclipsing binary stars and is a popular target for amateur astronomers.
In some binary systems, the less-massive star has become a giant, while the more-massive star is still on the main sequence. If higher-mass stars evolve faster than lower-mass stars, how do the lower-mass stars in such binaries manage to leave the main sequence first? This is called the Algol paradox, after the binary system Algol.