2 * Copyright (c) 1989, 1993
3 * The Regents of the University of California. All rights reserved.
5 * This code is derived from software posted to USENET.
7 * Redistribution and use in source and binary forms, with or without
8 * modification, are permitted provided that the following conditions
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11 * notice, this list of conditions and the following disclaimer.
12 * 2. Redistributions in binary form must reproduce the above copyright
13 * notice, this list of conditions and the following disclaimer in the
14 * documentation and/or other materials provided with the distribution.
15 * 3. All advertising materials mentioning features or use of this software
16 * must display the following acknowledgement:
17 * This product includes software developed by the University of
18 * California, Berkeley and its contributors.
19 * 4. Neither the name of the University nor the names of its contributors
20 * may be used to endorse or promote products derived from this software
21 * without specific prior written permission.
23 * THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND
24 * ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
25 * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
26 * ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE
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29 * OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION)
30 * HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
31 * LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY
32 * OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
35 * @(#) Copyright (c) 1989, 1993 The Regents of the University of California. All rights reserved.
36 * @(#)pom.c 8.1 (Berkeley) 5/31/93
37 * $FreeBSD: src/games/pom/pom.c,v 1.9 1999/11/30 03:49:09 billf Exp $
38 * $DragonFly: src/games/pom/pom.c,v 1.4 2006/08/08 17:08:49 pavalos Exp $
42 * Phase of the Moon. Calculates the current phase of the moon.
43 * Based on routines from `Practical Astronomy with Your Calculator',
44 * by Duffett-Smith. Comments give the section from the book that
45 * particular piece of code was adapted from.
47 * -- Keith E. Brandt VIII 1984
56 #define EPSILONg 279.611371 /* solar ecliptic long at EPOCH */
57 #define RHOg 282.680403 /* solar ecliptic long of perigee at EPOCH */
58 #define ECCEN 0.01671542 /* solar orbit eccentricity */
59 #define lzero 18.251907 /* lunar mean long at EPOCH */
60 #define Pzero 192.917585 /* lunar mean long of perigee at EPOCH */
61 #define Nzero 55.204723 /* lunar mean long of node at EPOCH */
62 #define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
64 static void adj360 (double *);
65 static double dtor (double);
66 static double potm (double);
73 double days, today, tomorrow;
78 days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
79 (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
80 for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
81 days += isleap(1900 + cnt) ? 366 : 365;
82 today = potm(days) + .5;
83 (void)printf("The Moon is ");
84 if ((int)today == 100)
85 (void)printf("Full\n");
87 (void)printf("New\n");
89 tomorrow = potm(days + 1);
91 (void)printf("%s\n", tomorrow > today ?
92 "at the First Quarter" : "at the Last Quarter");
94 (void)printf("%s ", tomorrow > today ?
97 (void)printf("Gibbous (%1.0f%% of Full)\n",
100 (void)printf("Crescent (%1.0f%% of Full)\n",
110 * return phase of the moon
115 double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
116 double A4, lprime, V, ldprime, D, Nm;
118 N = 360 * days / 365.2422; /* sec 42 #3 */
120 Msol = N + EPSILONg - RHOg; /* sec 42 #4 */
122 Ec = 360 / M_PI * ECCEN * sin(dtor(Msol)); /* sec 42 #5 */
123 LambdaSol = N + Ec + EPSILONg; /* sec 42 #6 */
125 l = 13.1763966 * days + lzero; /* sec 61 #4 */
127 Mm = l - (0.1114041 * days) - Pzero; /* sec 61 #5 */
129 Nm = Nzero - (0.0529539 * days); /* sec 61 #6 */
131 Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm)); /* sec 61 #7 */
132 Ac = 0.1858 * sin(dtor(Msol)); /* sec 61 #8 */
133 A3 = 0.37 * sin(dtor(Msol));
134 Mmprime = Mm + Ev - Ac - A3; /* sec 61 #9 */
135 Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 61 #10 */
136 A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 61 #11 */
137 lprime = l + Ev + Ec - Ac + A4; /* sec 61 #12 */
138 V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 61 #13 */
139 ldprime = lprime + V; /* sec 61 #14 */
140 D = ldprime - LambdaSol; /* sec 63 #2 */
141 return(50 * (1 - cos(dtor(D)))); /* sec 63 #3 */
146 * convert degrees to radians
151 return(deg * M_PI / 180);
156 * adjust value so 0 <= deg <= 360