(1) Period: The three sliders allow the separation in astronomical units and the masses (in units of solar masses) to be input and the period in years is calculated.
(2) Separation: The three sliders allow the period in years and the masses in units of solar masses to be input and the separation in astronomical units is calculated.
(3) Sum of Masses:
The three sliders allow the period in years, the separation,
and the ratio of masses M(1)/M(2) to be input and the sum
of the masses M(1) + M(2) and the individual masses are calculated.
Note that Kepler's Laws alone allow only the sum of the masses
to be calculated. The ratio M(1)/M(2) used to apportion
masses between the two objects must be obtained independent of
Kepler's Laws (for example, by observing the orbits and locating
the center of mass).
Data Display: The upper left portion of the display area shows the quantity being calculated and the diagram for location of the masses and center of mass, and the orbits (assuming spherical orbits) as the parameters are varied with the sliders.
The lower left portion of the display area shows the algebraic equations that are being solved to construct the display in the upper left.