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Eclipsing binary stars are a pair of stars that orbit each other in such a way that one star passes in front of the other as seen from Earth, causing periodic dimming of light observed from the system.
Astronomers and astrophysicists conducting research on binary star systems are required to file reports on eclipsing binary stars to share findings with the scientific community.
Filling out information on eclipsing binary stars typically involves gathering observational data, calculating light curves, and documenting the characteristics of the stars and their orbits in a standardized format.
The purpose of studying eclipsing binary stars is to understand their physical properties, such as mass, radius, and luminosity, and to gain insights into stellar evolution and dynamics.
Information that must be reported includes the periods of eclipses, brightness measurements, distances, spectral classifications, and any peculiar behaviors observed in the stars.
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