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Update pom to the third edition of Duffett-Smith's book, and clean it
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1 /* $NetBSD: pom.c,v 1.12 1999/09/14 20:00:07 jsm Exp $ */
2
3 /*
4 * Copyright (c) 1989, 1993
5 * The Regents of the University of California. All rights reserved.
6 *
7 * This code is derived from software posted to USENET.
8 *
9 * Redistribution and use in source and binary forms, with or without
10 * modification, are permitted provided that the following conditions
11 * are met:
12 * 1. Redistributions of source code must retain the above copyright
13 * notice, this list of conditions and the following disclaimer.
14 * 2. Redistributions in binary form must reproduce the above copyright
15 * notice, this list of conditions and the following disclaimer in the
16 * documentation and/or other materials provided with the distribution.
17 * 3. All advertising materials mentioning features or use of this software
18 * must display the following acknowledgement:
19 * This product includes software developed by the University of
20 * California, Berkeley and its contributors.
21 * 4. Neither the name of the University nor the names of its contributors
22 * may be used to endorse or promote products derived from this software
23 * without specific prior written permission.
24 *
25 * THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND
26 * ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
27 * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
28 * ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE
29 * FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
30 * DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS
31 * OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION)
32 * HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
33 * LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY
34 * OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
35 * SUCH DAMAGE.
36 */
37
38 #include <sys/cdefs.h>
39 #ifndef lint
40 __COPYRIGHT("@(#) Copyright (c) 1989, 1993\n\
41 The Regents of the University of California. All rights reserved.\n");
42 #endif /* not lint */
43
44 #ifndef lint
45 #if 0
46 static char sccsid[] = "@(#)pom.c 8.1 (Berkeley) 5/31/93";
47 #else
48 __RCSID("$NetBSD: pom.c,v 1.12 1999/09/14 20:00:07 jsm Exp $");
49 #endif
50 #endif /* not lint */
51
52 /*
53 * Phase of the Moon. Calculates the current phase of the moon.
54 * Based on routines from `Practical Astronomy with Your Calculator',
55 * by Duffett-Smith. Comments give the section from the book that
56 * particular piece of code was adapted from.
57 *
58 * -- Keith E. Brandt VIII 1984
59 *
60 * Updated to the Third Edition of Duffett-Smith's book, Paul Janzen, IX 1998
61 *
62 */
63
64 #include <ctype.h>
65 #include <err.h>
66 #include <math.h>
67 #include <stdio.h>
68 #include <string.h>
69 #include <stdlib.h>
70 #include <time.h>
71 #include <unistd.h>
72
73 #ifndef PI
74 #define PI 3.14159265358979323846
75 #endif
76
77 /*
78 * The EPOCH in the third edition of the book is 1990 Jan 0.0 TDT.
79 * In this program, we do not bother to correct for the differences
80 * between UTC (as shown by the UNIX clock) and TDT. (TDT = TAI + 32.184s;
81 * TAI-UTC = 32s in Jan 1999.)
82 */
83 #define EPOCH_MINUS_1970 (20 * 365 + 5 - 1) /* 20 years, 5 leaps, back 1 day to Jan 0 */
84 #define EPSILONg 279.403303 /* solar ecliptic long at EPOCH */
85 #define RHOg 282.768422 /* solar ecliptic long of perigee at EPOCH */
86 #define ECCEN 0.016713 /* solar orbit eccentricity */
87 #define lzero 318.351648 /* lunar mean long at EPOCH */
88 #define Pzero 36.340410 /* lunar mean long of perigee at EPOCH */
89 #define Nzero 318.510107 /* lunar mean long of node at EPOCH */
90
91 void adj360 __P((double *));
92 double dtor __P((double));
93 int main __P((int, char *[]));
94 double potm __P((double));
95 time_t parsetime __P((char *));
96 void badformat __P((void)) __attribute__((__noreturn__));
97
98 int
99 main(argc, argv)
100 int argc;
101 char *argv[];
102 {
103 time_t tmpt, now;
104 double days, today, tomorrow;
105 char buf[1024];
106
107 if (time(&now) == (time_t)-1)
108 err(1, "time");
109 if (argc > 1) {
110 tmpt = parsetime(argv[1]);
111 strftime(buf, sizeof(buf), "%a %Y %b %e %H:%M:%S (%Z)",
112 localtime(&tmpt));
113 printf("%s: ", buf);
114 } else {
115 tmpt = now;
116 }
117 days = (tmpt - EPOCH_MINUS_1970 * 86400) / 86400.0;
118 today = potm(days) + .5;
119 if (tmpt < now)
120 (void)printf("The Moon was ");
121 else if (tmpt == now)
122 (void)printf("The Moon is ");
123 else
124 (void)printf("The Moon will be ");
125 if ((int)today == 100)
126 (void)printf("Full\n");
127 else if (!(int)today)
128 (void)printf("New\n");
129 else {
130 tomorrow = potm(days + 1);
131 if ((int)today == 50)
132 (void)printf("%s\n", tomorrow > today ?
133 "at the First Quarter" : "at the Last Quarter");
134 /* today is 0.5 too big, but it doesn't matter here
135 * since the phase is changing fast enough
136 */
137 else {
138 today -= 0.5; /* Now it might matter */
139 (void)printf("%s ", tomorrow > today ?
140 "Waxing" : "Waning");
141 if (today > 50)
142 (void)printf("Gibbous (%1.0f%% of Full)\n",
143 today);
144 else if (today < 50)
145 (void)printf("Crescent (%1.0f%% of Full)\n",
146 today);
147 }
148 }
149 exit(0);
150 }
151
152 /*
153 * potm --
154 * return phase of the moon
155 */
156 double
157 potm(days)
158 double days;
159 {
160 double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
161 double A4, lprime, V, ldprime, D, Nm;
162
163 N = 360 * days / 365.242191; /* sec 46 #3 */
164 adj360(&N);
165 Msol = N + EPSILONg - RHOg; /* sec 46 #4 */
166 adj360(&Msol);
167 Ec = 360 / PI * ECCEN * sin(dtor(Msol)); /* sec 46 #5 */
168 LambdaSol = N + Ec + EPSILONg; /* sec 46 #6 */
169 adj360(&LambdaSol);
170 l = 13.1763966 * days + lzero; /* sec 65 #4 */
171 adj360(&l);
172 Mm = l - (0.1114041 * days) - Pzero; /* sec 65 #5 */
173 adj360(&Mm);
174 Nm = Nzero - (0.0529539 * days); /* sec 65 #6 */
175 adj360(&Nm);
176 Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm)); /* sec 65 #7 */
177 Ac = 0.1858 * sin(dtor(Msol)); /* sec 65 #8 */
178 A3 = 0.37 * sin(dtor(Msol));
179 Mmprime = Mm + Ev - Ac - A3; /* sec 65 #9 */
180 Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 65 #10 */
181 A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 65 #11 */
182 lprime = l + Ev + Ec - Ac + A4; /* sec 65 #12 */
183 V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 65 #13 */
184 ldprime = lprime + V; /* sec 65 #14 */
185 D = ldprime - LambdaSol; /* sec 67 #2 */
186 return(50.0 * (1 - cos(dtor(D)))); /* sec 67 #3 */
187 }
188
189 /*
190 * dtor --
191 * convert degrees to radians
192 */
193 double
194 dtor(deg)
195 double deg;
196 {
197 return(deg * PI / 180);
198 }
199
200 /*
201 * adj360 --
202 * adjust value so 0 <= deg <= 360
203 */
204 void
205 adj360(deg)
206 double *deg;
207 {
208 for (;;)
209 if (*deg < 0)
210 *deg += 360;
211 else if (*deg > 360)
212 *deg -= 360;
213 else
214 break;
215 }
216
217 #define ATOI2(ar) ((ar)[0] - '0') * 10 + ((ar)[1] - '0'); (ar) += 2;
218 time_t
219 parsetime(p)
220 char *p;
221 {
222 struct tm *lt;
223 int bigyear;
224 int yearset = 0;
225 time_t tval;
226 unsigned char *t;
227
228 for (t = p; *t; ++t) {
229 if (isdigit(*t))
230 continue;
231 badformat();
232 }
233
234 tval = time(NULL);
235 lt = localtime(&tval);
236 lt->tm_sec = 0;
237 lt->tm_min = 0;
238
239 switch (strlen(p)) {
240 case 10: /* yyyy */
241 bigyear = ATOI2(p);
242 lt->tm_year = bigyear * 100 - 1900;
243 yearset = 1;
244 /* FALLTHROUGH */
245 case 8: /* yy */
246 if (yearset) {
247 lt->tm_year += ATOI2(p);
248 } else {
249 lt->tm_year = ATOI2(p);
250 if (lt->tm_year < 69) /* hack for 2000 */
251 lt->tm_year += 100;
252 }
253 /* FALLTHROUGH */
254 case 6: /* mm */
255 lt->tm_mon = ATOI2(p);
256 if ((lt->tm_mon > 12) || !lt->tm_mon)
257 badformat();
258 --lt->tm_mon; /* time struct is 0 - 11 */
259 /* FALLTHROUGH */
260 case 4: /* dd */
261 lt->tm_mday = ATOI2(p);
262 if ((lt->tm_mday > 31) || !lt->tm_mday)
263 badformat();
264 /* FALLTHROUGH */
265 case 2: /* HH */
266 lt->tm_hour = ATOI2(p);
267 if (lt->tm_hour > 23)
268 badformat();
269 break;
270 default:
271 badformat();
272 }
273 /* The calling code needs a valid tm_ydays and this is the easiest
274 * way to get one */
275 if ((tval = mktime(lt)) == -1)
276 errx(1, "specified date is outside allowed range");
277 return (tval);
278 }
279
280 void
281 badformat()
282 {
283 warnx("illegal time format");
284 (void)fprintf(stderr, "usage: pom [[[[[cc]yy]mm]dd]HH]\n");
285 exit(1);
286 }