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PLANETS.DOC
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1985-10-09
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Version 1.0
This Program computes information relating to the position, distance,
magnitude, etc for the major planets on a specified date and time.
Refer to PRACTICAL ASTRONOMY WITH YOUR CALCULATOR by Peter Duffett-Smith
for the calculation methods.
This program is placed in the public domain "as is".
Comments may be sent to the author:
Larry Puhl
6 Plum Court
Sleepy Hollow, Ill. 60118
Glossary of Terms
Azimuth : The angle from the North measured East to West. When
applied to set and rise times for a planet this
indicated where on the horizon, 180 deg. for South,
270 deg. for West, etc.
Daylight Savings : If Daylight savings time is enabed then the local time
is advanced one hour on the last Sunday in March and
set back on the last Sunday in October.
Ecliptic Coordinates : Are related to the earths orbit, Long is the
angle around from the first point of Aries
and Lat is angle Up or Down
Equatorial Coord. : Are related to the earths equator, DEC is how
far north or south of the equator and RA is
angle around the equator from the first point
of Aries
First Point of Aries : This direction remains fixed with respect to the
stars (except for Precession) and is used as a
reference for ecliptic and equatorial coordinates.
GMT : Greenwich Mean Time, time at longitude 0 deg.
GST : Greenwich mean sideral time, is related to the
position of of the stars rather than the Sun.
JD : Julian Day Number is the number of days since
January 1st 4713 B.C.
HA : Hour Angle is the time since the planet crossed
the meridian
helio ecliptic lat. : Angle north or south of the earths orbit
heliocentric long : Angle from the first point of Aries that planet
makes round the sun
Horizontal Coord. : Are related to the observers horizon, Alt is
angle above the horizon and Azim is angle from
the north going east.
Lat : Latitude of observing site
LCT : Local Civil Time (time locally used)
LST : Local Sideral Time, is related to the
position of of the stars rather than the Sun.
Long : Longitude of observing site
long of ascend node : The point where a planet rises out of the plane of
the ecliptic
Mag : Magnitude on a logrithmic scale which measures the
brightness of the planet ( the calculation here is
accurate to only 1 or 2
mean anomaly : Angle a fictitious planet, moving in a circle,
would make with a line from the sun to the
planets perihelion
Phase : Area of the disc which is illuminated
true anomaly : Corrects the mean anomaly to account for the
eccentricity of the orbit
radius vector : Distance from the Sun to the planet