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1.1 root 1: .th SKY VI 9/22/73
2: .sh NAME
3: sky \*- obtain ephemerides
4: .sh SYNOPSIS
5: .bd sky
6: .sh DESCRIPTION
7: .it Sky
8: predicts the apparent locations
9: of the Sun, the Moon, the planets out to Saturn,
10: stars of magnitude at least 2.5,
11: and certain other celestial objects
12: including comet Kohoutek and M31.
13: .it Sky
14: reads the standard input to obtain
15: a GMT time typed
16: on one line with blanks separating
17: year, month number, day, hour, and minute;
18: if the year is missing the current year is used.
19: If a blank line is typed the current time is used.
20: The program prints the
21: azimuth, elevation, and magnitude
22: of objects which are above the horizon
23: at the ephemeris location of Murray Hill
24: at the indicated time.
25: .s3
26: Placing a ``1'' input after the minute entry
27: causes the program to print out the Greenwich Sidereal
28: Time at the indicated moment and
29: to print for each body
30: its right ascension and
31: declination as well as its azimuth and elevation.
32: Also, instead of the magnitude,
33: the geocentric distance of the body, in units the program
34: considers convenient, is printed.
35: (For planets the unit is essentially A. U.)
36: .s3
37: The magnitudes of Solar System bodies are not calculated
38: and are given as 0.
39: The effects of atmospheric extinction
40: are not included;
41: the mean magnitudes
42: of variable stars are marked with ``*''.
43: .s3
44: For all bodies, the program takes into account
45: precession and nutation of the equinox,
46: annual (but not diurnal) aberration, diurnal
47: parallax,
48: and the proper motion of stars (but not annual parallax).
49: In no case is refraction included.
50: .s3
51: The program takes into account perturbations
52: of the Earth due to the Moon, Venus, Mars, and Jupiter.
53: The expected accuracies
54: are:
55: for the Sun and other stellar bodies
56: a few tenths of seconds of arc;
57: for the Moon (on which particular care is lavished)
58: likewise a few tenths of seconds.
59: For the Sun, Moon and stars the accuracy is sufficient
60: to predict the circumstances of eclipses and occultations
61: to within a few seconds of time.
62: The planets may be off by several minutes of arc.
63: .s3
64: Information about the program
65: may be obtained from its author.
66: .sh FILES
67: /usr/lib/startab, /usr/lib/moontab
68: .sh "SEE ALSO"
69: azel (VI)
70: .br
71: .ft I
72: American Ephemeris and Nautical Almanac,
73: .ft R
74: for the appropriate years;
75: also, the
76: .ft I
77: Explanatory Supplement to the American Ephemeris
78: and Nautical Almanac.
79: .ft R
80: .sh AUTHOR
81: R. Morris
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