[BASIC OPTIONS AND TERMINOLOGY] In Nightfall, the is the star passing in front of the other one first, and the thus is the star first eclipsed. The is mass(Secondary)/mass(Primary), thus it is higher than one if the Secondary is more massive. The is the angle, under which the plane, in which the two stars orbit each other, is seen from earth. Only for inclinations near 90 deg (near edge-on view) an eclipse is possible. The is the maximum size a star can have in a binary system. It depends on the mass ratio - the more massive star has the larger Roche lobe. If the stars overfill their Roche lobes, they form a or system. To define the sizes of the two stars, you have to specify the , which are defined in units of the maximum polar radii (i.e. the polar radii of the Roche lobes). The is the surface temperature of the star. The luminosity of a star depends on its surface area (i.e. size) and the temperature. [Limiting values] To avoid numerical problems, parameters are limited to reasonable values. These are: { mass ratio: 0.0001 - 10000 inclination: 0 - 90 Roche lobe fill factor: 0.001 - 1.3 temperature: 350 - 350000 (blackbody) 2000 - 31000 (model atmosphere, log g 3.5) 2000 - 39000 (model atmosphere, log g 4.0) 2000 - 49000 (model atmosphere, log g 4.5) 2000 - 49000 (model atmosphere, log g 5.0) } If a value is out of range, it will be reset to the lowest/highest allowed value. For Roche lobe fill factors above one, the mass ratio is restricted to 0.003 - 50. [Terminal Output] will cause Nightfall to print out warnings (like parameter out of range). Usually, this refers to problems Nightfall can cope with by itself. In case Nightfall refuses to do what you want, it might be of some help to use this option. will print out some verbose output on what Nightfall is currently doing. will print out some status information (just enought to keep your screen busy) in case you are doing something rather lengthy, like, e.g., automatic fitting of parameters to observational data.