Now supports control for Meade LX200 and compatable telescopes
The primary goals of PSC are to:
Other handy features include:
Theory of Operation
PSC performs all computations to full precision, always opting for accuracy over speed. Nevertheless, times are not unacceptable even on small PDAs with no hardware floating point due to extensive look-ahead and field-culling techniques. Fixed objects are first sorted into roughly 1 degree sky patches based on their J2000 coordinates. These patches are indexed for fast random access and each is also sorted by decreasing brightness within each patch. So large areas are fast because each patch is quickly abandoned (assuming reasonable limiting magnitude) and small areas are fast because only the required patches are searched. No further computation is required unless Topo or EOD options are turned on.
Things are not quite so easy for asteroids because they move. They are sorted according their brightest possible magnitude which can be computed for all time from their orbital elements alone. An asteroid's ephemeris is recomputed if 1) it can ever be as bright as the current limiting magnitude setting and 2) it could conceivable enter the field of view based on their last known location and velocity (which implies they must all be computed at least once, which you can witness as you look at dimmer magnitudes).
The small progress bar in the lower left will help you get a feel for these algorithms in practice. In general, load only the catalogs of interest and either don't look deep or use a small field of view. The limiting magnitude PSC chooses automatically for any given field size is a good compromise, but can be changed if desired using the light bulbs in the toolbar.