Preface | |
Using your personal computer for astronomy | |
Default value input routine | |
'Y' or 'N' input routine MINSEC converts between decimal hours/degrees and min/sec form | |
JULDAY calendar date to Julian day number since 1900 Jan. 0.5 | |
CALDAY Julian day number since 1900 Jan. 0.5 to calendar date | |
TIME converts between local civil and sidereal times | |
EQHOR converts between equatorial and horizon coordinates | |
HRANG converts between right ascension and hour-angle | |
OBLIQ calculates the value of the obliquity of the ecliptic | |
NUTAT finds corrections for nutation in longitude and obliquity | |
EQECL converts between equatorial and ecliptic coordinates | |
EQGAL converts between equatorial and galactic coordinates | |
GENCON converts between any of the coordinate systems | |
PRCESS1 approximate precession of equatorial coordinates | |
PRCESS2 rigorous precession of equatorial coordinates | |
PARALLX converts between geocentric and apparent position | |
REFRACT calculates the effect of atmospheric refraction | |
RISET finds the circumstances of rising and setting | |
ANOMALY solves Kepler's equation for elliptical motion | |
SUN finds the ecliptic coordinates of the Sun | |
SUNRS finds the circumstances of sunrise and sunset | |
PELMENT returns the orbital elements of the major planets | |
PLANS finds the position of a planet | |
MOON finds the position and parallax of the Moon | |
MOONRS finds the circumstances of moonrise and moonset | |
MOONNF finds the times of new and full moon | |
ECLIPSE finds the circumstances of lunar and solar eclipses | |
Displays an eclipse in graphical form | |
ELOSC finds positions from osculating elliptical elements | |
RELEM converts ecliptic orbital elements from one epoch to another | |
PCOMET finds the position of a comet from parabolic elements | |
PFIT finds parabolic elements from observations | |
EFIT finds elliptical elements from observations | |
List of variables | |
Bibliography | |
Index. |
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