A time series of a binary star system's apparent brightness, collected by NASA's Kepler mission. These "eclipsing binary" stars orbit one other with a period of ~1.56 Earth days and eclipse one another from the perspective of Earthly observers. The Kepler identification number for this eclipsing binary system is KIC 6048106.

eclipsing_binary

Format

A tibble with column set c("phase", "flux", "std_err").

Source

http://keplerebs.villanova.edu/