drm/linux: Add kasprintf and kvasprintf()
[dragonfly.git] / games / pom / pom.c
blob828d9bee0186fa5f218cb30572652fbbe52d369b
1 /*-
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
9 * are met:
10 * 1. Redistributions of source code must retain the above copyright
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. Neither the name of the University nor the names of its contributors
16 * may be used to endorse or promote products derived from this software
17 * without specific prior written permission.
19 * THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND
20 * ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
21 * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
22 * ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE
23 * FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
24 * DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS
25 * OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION)
26 * HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
27 * LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY
28 * OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
29 * SUCH DAMAGE.
31 * @(#) Copyright (c) 1989, 1993 The Regents of the University of California. All rights reserved.
32 * @(#)pom.c 8.1 (Berkeley) 5/31/93
33 * $FreeBSD: src/games/pom/pom.c,v 1.9 1999/11/30 03:49:09 billf Exp $
34 * $DragonFly: src/games/pom/pom.c,v 1.4 2006/08/08 17:08:49 pavalos Exp $
38 * Phase of the Moon. Calculates the current phase of the moon.
39 * Based on routines from `Practical Astronomy with Your Calculator',
40 * by Duffett-Smith. Comments give the section from the book that
41 * particular piece of code was adapted from.
43 * -- Keith E. Brandt VIII 1984
47 #include <time.h>
48 #include <stdio.h>
49 #include <math.h>
51 #define EPOCH 85
52 #define EPSILONg 279.611371 /* solar ecliptic long at EPOCH */
53 #define RHOg 282.680403 /* solar ecliptic long of perigee at EPOCH */
54 #define ECCEN 0.01671542 /* solar orbit eccentricity */
55 #define lzero 18.251907 /* lunar mean long at EPOCH */
56 #define Pzero 192.917585 /* lunar mean long of perigee at EPOCH */
57 #define Nzero 55.204723 /* lunar mean long of node at EPOCH */
58 #define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
60 static void adj360 (double *);
61 static double dtor (double);
62 static double potm (double);
64 int
65 main(void)
67 time_t tt;
68 struct tm *GMT;
69 double days, today, tomorrow;
70 int cnt;
72 (void) time(&tt);
73 GMT = gmtime(&tt);
74 days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
75 (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
76 for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
77 days += isleap(1900 + cnt) ? 366 : 365;
78 today = potm(days) + .5;
79 (void)printf("The Moon is ");
80 if ((int)today == 100)
81 (void)printf("Full\n");
82 else if (!(int)today)
83 (void)printf("New\n");
84 else {
85 tomorrow = potm(days + 1);
86 if ((int)today == 50)
87 (void)printf("%s\n", tomorrow > today ?
88 "at the First Quarter" : "at the Last Quarter");
89 else {
90 (void)printf("%s ", tomorrow > today ?
91 "Waxing" : "Waning");
92 if (today > 50)
93 (void)printf("Gibbous (%1.0f%% of Full)\n",
94 today);
95 else if (today < 50)
96 (void)printf("Crescent (%1.0f%% of Full)\n",
97 today);
101 return 0;
105 * potm --
106 * return phase of the moon
108 static double
109 potm(double days)
111 double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
112 double A4, lprime, V, ldprime, D, Nm;
114 N = 360 * days / 365.2422; /* sec 42 #3 */
115 adj360(&N);
116 Msol = N + EPSILONg - RHOg; /* sec 42 #4 */
117 adj360(&Msol);
118 Ec = 360 / M_PI * ECCEN * sin(dtor(Msol)); /* sec 42 #5 */
119 LambdaSol = N + Ec + EPSILONg; /* sec 42 #6 */
120 adj360(&LambdaSol);
121 l = 13.1763966 * days + lzero; /* sec 61 #4 */
122 adj360(&l);
123 Mm = l - (0.1114041 * days) - Pzero; /* sec 61 #5 */
124 adj360(&Mm);
125 Nm = Nzero - (0.0529539 * days); /* sec 61 #6 */
126 adj360(&Nm);
127 Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm)); /* sec 61 #7 */
128 Ac = 0.1858 * sin(dtor(Msol)); /* sec 61 #8 */
129 A3 = 0.37 * sin(dtor(Msol));
130 Mmprime = Mm + Ev - Ac - A3; /* sec 61 #9 */
131 Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 61 #10 */
132 A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 61 #11 */
133 lprime = l + Ev + Ec - Ac + A4; /* sec 61 #12 */
134 V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 61 #13 */
135 ldprime = lprime + V; /* sec 61 #14 */
136 D = ldprime - LambdaSol; /* sec 63 #2 */
137 return(50 * (1 - cos(dtor(D)))); /* sec 63 #3 */
141 * dtor --
142 * convert degrees to radians
144 static double
145 dtor(double deg)
147 return(deg * M_PI / 180);
151 * adj360 --
152 * adjust value so 0 <= deg <= 360
154 static void
155 adj360(double *deg)
157 for (;;)
158 if (*deg < 0)
159 *deg += 360;
160 else if (*deg > 360)
161 *deg -= 360;
162 else
163 break;