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1.1 root 1: .TH SKY 7 bowell
2: .CT 1 inst_info
3: .SH NAME
4: sky \- astronomical ephemeris
5: .SH SYNOPSIS
6: .B sky
7: [
8: .B -l
9: ]
10: .SH DESCRIPTION
11: .I Sky
12: predicts the apparent locations of the sun, moon, visible planets,
13: and stars brighter than magnitude 2.5.
14: It reads one line from the standard input to obtain the desired time
15: expressed as five numbers: year, month, day, hour, and minute in GMT.
16: An empty line means now.
17: Each object is printed with astronomical coordinates, azimuth-elevation
18: coordinates relative to Murray Hill, NJ, and magnitude.
19: For variable stars the maximum magnitude is printed with
20: .LR * .
21: .PP
22: Option
23: .B -l
24: causes
25: .I sky
26: to prompt for another viewing location.
27: .PP
28: Standard astronomical effects are accounted for:
29: nutation and precession of the equinox, annual aberration, diurnal parallax,
30: and proper motion.
31: Atmospheric effects (extinction and refraction) are not calculated,
32: nor is perturbation of the earth by other bodies.
33: .PP
34: In ephemeris (slighly different from civil) time, the program
35: yields
36: positions of sun, moon, and stars good to a few tenths of an
37: arc-second.
38: Planets are good to a few seconds.
39: .SH FILES
40: .F /usr/lib/startab
41: .SH SEE ALSO
42: .IR scat (7)
43: .br
44: .I
45: American Ephemeris and Nautical Almanac
46: and
47: .I
48: Explanatory Supplement to the American Ephemeris and Nautical Almanac
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