The Planet Visibility Calculator answers one question every stargazer asks: which planets can I actually see tonight, and when? Give it a date and your location and it computes the rise, transit and set times, the altitude and the brightness of Mercury, Venus, Mars, Jupiter and Saturn, then rates how well each is placed. This article explains how those numbers are produced, what each input changes, and where the simple model reaches its limits.
How the Planet Visibility Calculator works
The calculator uses NASA/JPL low-precision Keplerian orbital elements (the Standish formulae, accurate to a few arcminutes from 1800 to 2050) to find each planet's heliocentric position, then subtracts Earth's position to get the geocentric direction and converts it to right ascension and declination. Combining those coordinates with your latitude, longitude and the local sidereal time gives the planet's altitude, from which the rise, transit and set times follow. Brightness comes from standard magnitude formulae using the Sun-planet and Earth-planet distances and the phase angle. Sources: JPL Approximate Positions of the Planets and Jean Meeus, Astronomical Algorithms.
Inputs and what they mean
Date sets the evening you want to observe; results cover that night from dusk to the following dawn. Latitude and longitude fix your spot on Earth — latitude controls how high each planet climbs, while longitude shifts the clock times. Use positive numbers for north and east, negative for south and west. Planet lets you focus on one world or show all five at once. Times are displayed in your browser's local time zone, shown beneath the inputs, so a location far from you will read in your clock rather than the site's local time.
Limits and edge cases
The positions are accurate to roughly a few arcminutes — far finer than the naked eye can resolve — but this is a planning tool, not an ephemeris for telescope pointing. It ignores atmospheric extinction, so a planet listed at 3° altitude will be dimmer and redder than its magnitude suggests, and light pollution can hide a faint Mercury entirely. Near the poles the Sun may never set, which collapses the dark window. Saturn's ring tilt is not modelled, so its magnitude can be off by up to half a magnitude. For exact rise times to the second or occultation work, consult a dedicated ephemeris such as JPL HORIZONS or planetarium software like Stellarium.