By measuring the position angle of the companion star relative to the primary and the angler distance between the two stars over time, the [[ellipse]], called the apparent ellipse, which is the orbit of the secondary in respect to the primary, can be plotted out. From this measurement of the semi-major axis and orbital period of binary stars' orbit, the mass of the stars can be determined.<ref>http://csep10.phys.utk.edu/astr162/lect/binaries/visual.html</ref> | By measuring the position angle of the companion star relative to the primary and the angler distance between the two stars over time, the [[ellipse]], called the apparent ellipse, which is the orbit of the secondary in respect to the primary, can be plotted out. From this measurement of the semi-major axis and orbital period of binary stars' orbit, the mass of the stars can be determined.<ref>http://csep10.phys.utk.edu/astr162/lect/binaries/visual.html</ref> |