Topocentric Positions of Major Solar System Objects and Bright Stars
This data service provides topocentric position data for the major Solar System bodies and selected bright stars. The output includes either right ascension and declination in reference to the true equator and equinox of date, or the zenith distance and azimuth . The distance to the object is included for Solar System bodies.
Data will be provided for the years 1800 through 2050.
Use the buttons under Location to find coordinates of cities or towns in the U.S. or its territories, or to convert between Degrees-Minutes-Seconds (DMS) and Decimal Degrees.
Be sure to read the Notes section for definitions and additional details on the data.
Notes
UT1
UT1 is a form of Universal Time affected by irregularities in the Earth's rotation, and is the modern version of mean solar time on the Greenwich meridian.
Ephemeris
The positions of the Solar System bodies are based on the Jet Propulsion Laboratory's DE405 ephemeris (Standish, E.M. 1998, "JPL Planetary and Lunar Ephemerides, DE405/LE405", JPL IOM 312.F-98-048)
Definitions
Distance: The distance from the observers position on the surface of the Earth to the Solar System object, given in Astronomical Units (Kilometers for the Moon). Distance is not calculated for stars.