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sky2.doc
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1988-08-11
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The Time Variable
The program aims at providing the position of
celestial bodies for a certain point in time and as seen
from a certain location; therefore, information relative to
this particular instant and this location has to be provided
by the user.
Year, month and day are entered according to
normal practice. The calendar used is the Julian calendar
for dates until October 5, 1582, and the Gregorian calendar
afterwards.
The time of the day is entered as "hour min"
counted from midnight (hence 14h = 2 p. m.). The time scale
is either Ephemeris Time, Universal Time, Mean Local Time,
Standard Time (for wich you have to provide the Time Zone)
or Sundial Time.
Geographical longitude and latitude are entered as
decimal angles (DDD.dd). "M" can also be used; this was an
ancient way to determine latitude, by the ratio of the hours
of daylight to twelve hours at the summer solstice. If "M"
is not available, just enter two dashes "--". If "M" is
available and entered, it will override the geographical
latituded entered earlier.
Finally, you might want to enter a note of some
sort for future reference if a printout of the screen is
needed.
The program will display on a single screen the
information already entered, plus a number of time
conversions and other related information.
All input data provided by the user are kept into
memory for further runs of the program. If one wishes, one
can go over again the input data routine and change only
selected variables.