the time between eclipses and the average distance between the stars
[object Object]
Figuring out what mass a star has is tricky. We have to calculate things like temperature, mass, and distance, and each calculation depends on the others. When two bodies orbit each other, we can calculate their masses based on the orbital time and the distance between them. When the binaries are eclipsing each other, that helps a LOT to figure out the distance between them and their masses.
Stellar masses can be determined by observing binary star-systems. The calculations of the orbits of the binary stars allow the masses of their component stars to be directly determined, which in turn allows other stellar parameters, such as radius and density, to be indirectly estimated.
somewhere between the stars
According to the book Earth Science: Geology, the Environment, and the Universe, astronomers can identify binary stars by measuring the position of the visible star in the pair and noting shifts as it orbits the center of mass between it and the unseen companion star.
Kilometers, kilograms or Earth masses and Earth radii.
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)
It is easy (with the right equipment ) to measure the periodicity of the eclipsing system and thereby the rotational speeds and thereby the relative masses and thereby (with the brightness) the distance and all sorts of other things.
Yes, because it is easier to determine the precise times of their mutual orbits, which allows us to calculate their masses.
Figuring out what mass a star has is tricky. We have to calculate things like temperature, mass, and distance, and each calculation depends on the others. When two bodies orbit each other, we can calculate their masses based on the orbital time and the distance between them. When the binaries are eclipsing each other, that helps a LOT to figure out the distance between them and their masses.
Stellar masses can be determined by observing binary star-systems. The calculations of the orbits of the binary stars allow the masses of their component stars to be directly determined, which in turn allows other stellar parameters, such as radius and density, to be indirectly estimated.
The masses of the two stars.
A balance.See the Related Questions to the left for more information.
somewhere between the stars
you
is an objects density the measure of the amount of matter in the object compared to known masses
According to the book Earth Science: Geology, the Environment, and the Universe, astronomers can identify binary stars by measuring the position of the visible star in the pair and noting shifts as it orbits the center of mass between it and the unseen companion star.
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