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.