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Eclipsing binary stars become dimmer when one star passes in front of the other, blocking its light from reaching an observer. This periodic obscuration reduces the overall brightness of the system as seen from Earth. The dimming occurs when the stars are aligned such that the foreground star partially or completely obscures the background star, leading to a characteristic light curve that reveals the stars' sizes and orbital dynamics.

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Does Taurus have any Binary stars?

Yes. Zeta Tauri, Kappa Tauri, and Lambda Tauri are eclipsing binary stars.


What role do binary stars play in eclipsing binaries?

Binary stars in eclipsing binaries orbit each other in such a way that from our viewpoint on Earth, they regularly pass in front of each other, causing eclipses. By studying the light curves during these eclipses, astronomers can infer information about the stars' sizes, masses, and orbital dynamics. This makes eclipsing binaries important for understanding stellar properties and evolution.


Eclipsing binary stars can sometimes be identified because?

they exhibit periodic variations in brightness as one star passes in front of the other, causing an eclipse-like event. By monitoring these changes in brightness over time, astronomers can determine the properties of the stars within the binary system, such as their sizes, masses, and orbital parameters. This information can provide valuable insights into stellar evolution and the dynamics of binary star systems.


Why are some binary stars called eclipsing?

Because in eclipsing binaries, the two stars orbit each other regularly passing in front of the other, blocking out some or all of light of the hidden star.


A star system in which on star blocks the light from another is called?

"Occulting binary". The word "occult" means hidden or in shadows; if a binary star's orbital plane happens to be exactly through the Earth's path, we might see two stars when they're separate and then see one of the stars disappear behind (or in front of) the other.


What is double stars in which one star moves directly in front of the other?

Each of those is an eclipsing binary.


Why Algol regularly change its brightness?

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.


Are eclipsing binary stars better for determining masses than non-eclipsing binaries?

Yes, because it is easier to determine the precise times of their mutual orbits, which allows us to calculate their masses.


Eclipsing binary star in Perseus?

An eclipsing binary star in Perseus is a system where two stars orbit each other in such a way that they periodically pass in front of each other, causing eclipses and variations in brightness as viewed from Earth. By studying these changes in brightness, astronomers can determine important properties of the stars, such as their masses and radii.


How can you tell if a star system is an eclipsing binary system?

Precisely by the eclipse - that's what an "eclipsing binary system" is all about. The idea is that one of the stars partially (or completely, in some cases) covers the other star; with the result that the combined brightness (as seen from Earth) gets less for some time.


What information can be gained from the light curves of eclipsing binaries?

By studying the variation of the light from an eclipsing binary's light curve, astronomers can derive detailed information not only about the stars' orbits and masses, but also about their radii.(McMillian)


What does a eclipsing binary look like?

An eclipsing binary system consists of two stars orbiting each other in such a way that they periodically pass in front of each other as seen from Earth. The light curve of an eclipsing binary system will show regular dips in brightness when one star crosses in front of the other, creating a characteristic pattern of alternating minima and maxima. These dips in brightness are caused by eclipses and can be used to determine various properties of the stars, such as their sizes and masses.