Topocentric Configuration of Major Solar System Bodies
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This data service provides tables of low precision topocentric position data for the Sun, Moon, and major planets at specified time(s). It is designed to provide "quick look" information that should be useful for tasks such as planning an observing session or pointing a telescope at one of the objects.

Data will be provided for a three year period from 1 January of the preceding year through 31 December of the following year. For dates outside of this range, see MICA and our other data services.

Use Form A for cities or towns in the U.S. or its territories. Use Form B for all other locations. Both forms are immediately below.

Be sure to read the Notes section (on this page beyond the two forms) for definitions and additional details on the data.

Form A - U.S. Cities or Towns


      Universal Time (UT1)

  (1 to 9999)



The place name you enter above must be a city or town in the U.S. The place's location will be retrieved from a file with over 22,000 places listed. Either upper- or lower-case letters or a combination can be used. Spell out place name prefixes, as in "East Orange", "Fort Lauderdale", "Mount Vernon", etc. The only exception is "St.", which is entered as an abbreviation with a period, as in "St. Louis". You need only enter as many characters as will unambiguously identify the place. The city or town name may be left blank if the State or Territory is District of Columbia.

  (-90 to 10999)  meters  

If the observer's height above sea level is known, you may enter it here. If unknown, sea level will be assumed.

Form B - Locations Worldwide


      Universal Time (UT1)

  (1 to 9999)


The place name you enter above is merely a label for the table header; you can enter any identifier, or none (avoid using punctuation characters). The data will be calculated for the longitude and latitude you enter below.

Note: With the exception of the seconds components, coordinate components should be entered as integers (no decimals).


  (-90 to 10999)  meters  

If the observer's height above sea level is known, you may enter it here. If unknown, sea level will be assumed.

Need coordinates?  Try NGA's GEOnet Names Server (GNS).
Need U.S. coordinates?  Try the USGS Geographic Names Information System (GNIS).


Output Table

The right ascension (R.A.) and declination (Dec.) columns provide the topocentric apparent equatorial coordinates of each object, rounded to the nearest tenth of a minute of time in right ascension and to the nearest arcminute in declination. The distance (Dist.) column gives the true distance from the observer to the object, rounded to the nearest 10-3 of an astronomical unit (A.U.) for the Sun and the major planets, and to the nearest kilometer (km) for the Moon. (Note that 10-3 AU is about 150,000 km, or 23.5 Earth radii.) Apparent horizon coordinates, referred to the observer's location, are tabulated in the zenith distance (Z.D.) and azimuth (Az.) columns. The horizon coordinates are tabulated to the nearest degree (atmospheric refraction is not taken into account). The elongation (Elong.) column gives the angular separation between the Sun and the object to the nearest degree. The direction of the object with respect to the Sun is given by the letters N, S, E, or W (north, south, east, or west) immediately preceding the angular measure. The diameter (Diam.) column lists the equatorial diameter of the object's apparent disk (fully illuminated), to the nearest tenth of an arcsecond.

The magnitude (Mag.) column provides the visual magnitude (not corrected for zenith angle) for of each major planet, rounded to the nearest tenth of a magnitude. The magnitudes of the Moon and Sun are not listed. When Mercury and Venus are near conjunction with the Sun, their computed magnitudes are not realistic and are not tabulated (i.e., dashes appear in the table in place of a numerical value). For Saturn, the magnitude includes the contribution due to the rings. For the Moon, the percentage of the disk that is illuminated is given in place of the magnitude.

Expressions for the apparent visual magnitudes of the major planets (except Mercury and Venus) are from Harris (1961) [1]. The expressions for the magnitudes of Mercury and Venus are based on the parameters given in Hilton (2005) [2]; these values may differ from those given in editions of The Astronomical Almanac published before 2007. Through its 2004 edition, The Astronomical Almanac used the work of Harris (1961) for Mercury and Venus as well. In 2005 and 2006, The Astronomical Almanac adopted values for Mercury and Venus from Hilton (2003) [3]. Since the 2007 edition, The Astronomical Almanac has followed Hilton (2005) for these two planets.

Eclipses and Transits

This data service also checks for the occurrence of eclipses of the Sun and Moon and transits of Mercury and Venus across the Sun. If one of these phenomena occurs, a message will appear directly below the main body of the table. The message will appear only if the phenomenon occurs when the objects involved are above the observer's horizon. It is important to understand that these messages describe the instantaneous status of the phenomenon at the time and location of interest. For example, a message such as "Sun in partial eclipse" means that at the time and location indicated, the Sun is partially obscured by the Moon, not that the eclipse necessarily is classified as a partial eclipse. A configuration table computed for the same date but some other time or location might indicate total or annular obscuration.


The user can specify the height of the observer, which can range from the surface of the Earth to a maximum of 10,999 m (the top of the troposphere). Although the observer's height is used in determining the positions, the effect is minimal and not usually apparent to the precision displayed here. However, due to the Moon's proximity, the effect on lunar distance is more noticeable.

How to Import the Table into a Spreadsheet

Open your favorite text editor, then copy the numerical part of the table (i.e., do not copy the table headings) from your browser and paste it into the text editor. Save the data as a text file.

In Excel for Windows, select Data on the menu bar, then From Text. Select your saved text file. Choose fixed width in the dialog box.

In Excel for Mac, select Data on the menu bar, then Get External Data, then Import from Text File. Select your saved text file. Choose fixed width in the dialog box.

  1. Harris, D. L. 1961, "Photometry and Colorimetry of Planets and Satellites," in Planets and Satellites, ed. G. P. Kuiper & B. A. Middlehurst (Chicago: University of Chicago Press) pp. 272-342.
  2. Hilton, J. 2005, "Improving the Visual Magnitudes of the Planets in The Astronomical Alamanac. I. Mercury and Venus," The Astronomical Journal, Vol. 129, pp. 2902-2906.
  3. Hilton, J. 2003, "Updating the Magnitudes of the Planets in The Astronomical Almanac," USNO/AA Tech Note 2003-04 (Washington: USNO)

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