Ephemeris
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An ephemeris (plural: ephemerides) (from the Greek word ephemeros = daily) is a device giving the positions of astronomical objects in the sky. Different kinds are used for astronomy and astrology. Even today an ephemeris will often be a simple printed table; however this was also one of the first applications of mechanical computers.
The position is given to astronomers in a Cartesian coordinate system of right ascension and declination or to astrologer in longitude along the zodiacal ecliptic. Astrological positions may be given for either noon or midnight.
An ephemeris may also provide data on astronomical phenomena of interest to astrologers and astronomers such as eclipses, apparent retrogradation/planetary stations, planetary ingresses, sidereal time, positions for the Mean and True nodes of the moon, the phases of the Moon, and sometimes even the position(s) of Chiron, Lilith, and other minor or imaginary celestial bodies. Some ephemerides also contain a monthly aspectarian, while others often include the declination of the planets as well as their longitudes, right ascensions or Cartesian coordinates.
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[edit] History
In 1554, Johannes Stadius published a well-known work known as Ephemerides novae at auctae that attempted to give accurate planetary positions. The effort was not entirely successful, and there were, for example, periodic errors in Stadius’ Mercury positions of up to ten degrees.
[edit] Scientific ephemeris
For scientific uses, a modern planetary ephemeris comprises software that generates positions of the planets and often of their satellites, or of asteroids or comets at virtually any time desired by the user. Often there is an option to find the velocities of the bodies of interest, as well.
Typically, such ephemerides cover several centuries, past and future; the future ones can be covered because celestial mechanics is an accurate theory. Nevertheless, there are secular phenomena, factors that cannot adequately be considered by ephemerides. The biggest uncertainties on planetary positions are due to the perturbations of numerous asteroids, most of whose masses are poorly known, rendering their effect uncertain. Therefore, despite efforts to overcome these uncertainties, the JPL has to revise its published ephemerides at intervals of 20 years.
Solar system ephemerides are essential for the navigation of spacecraft and for all kinds of space observations of the planets, their natural satellites, stars and galaxies.
Scientific ephemerides for sky observers mostly contain the position of the mentioned celestial body in right ascension and declination, because these coordinates are the most often used on star maps and telescopes. The equinox of the coordinate system must be given. It is in nearly all cases either the actual equinox (the equinox valid for that moment, often referred to as "of date" or "current"), or that of the one of the "standard" equinoxes, typically J2000.0, B1950.0, or J1900. Star maps are almost always in one of the standard equinoxes.
Scientific ephemerides often contain further useful data about the moon, planet, asteroid, or comet beyond the pure coordinates in the sky, such as elongation to the sun, brightness, distance, velocity, apparent diameter in the sky, phase angle, times of rise, transit, and set, etc. Ephemerides of the planet Saturn also sometimes contain the apparent inclination of its ring.
An ephemeris is usually only correct for a particular location on the Earth. In many cases the differences are too small to matter, but for nearby asteroids or the Moon they can be quite important.
[edit] Astrological ephemeris
Astrologers pay attention to different data than scientists. In particular they are concerned with the motion of planets through constellations, and when planets appear to become stationary due to relative motion with the earth around the sun.
Though astrology is and always has been geocentric, heliocentric astrology is an emerging field; for this purpose a standard ephemeris cannot be utilized, and because of this specialized heliocentric ephemerides must be calculated and used instead of the default geocentric ephemerides that are used in standard Western astrology to construct the astrological chart/natal chart.
[edit] References
- Montenbruck, Oliver (1989). Practical Ephemeris Calculations. Springer-Verlag. ISBN 0-387-50704-3.
- Meeus, Jean (1991). Astronomical Algorithms. Willmann-Bell. ISBN 0-943396-35-2.
[edit] External links
- The JPL HORIZONS online ephemeris
- Introduction to the JPL ephemerides
- The effect of asteroidal perturbations on the long term accuracy of ephemerides.
- Kharin, A. S. and Kolesnik, Y. B.; On the Errors of the Ephemerides Derived from Optical Observations of Planets. (1990), IAU SYMP.141 P.189, 1989.
- Source code for computing ephemerides - by Steve Moshier
- A Free 3200 Year Ephemeris Provided by Astro.com -- Based out of Zürich, Switzerland (available in 8 languages)
- The Original 3,000 Year High-Precision Daily Astrological Online Ephemeris from Khaldea.com -- 600BC to 2400AD -- Calculated for Midnight GMT; also with an Aspectarian included for years 1900 to 2005
- Interactive orrery and ephemeris provided by Fourmilab in Switzerland.
- Online Ephemeris from 1891 to 2100 -- A simple ephemeris that is very easy to use and extremely accurate. All times are for Midnight (00:00 Hours) Greenwich Mean Time (UTC).
- Monthly Ephemeris
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