1/*
2 * Copyright (c) 1989, 1993
3 *	The Regents of the University of California.  All rights reserved.
4 *
5 * This code is derived from software posted to USENET.
6 *
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.
18 *
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.
30 */
31
32#if 0
33#ifndef lint
34static const char copyright[] =
35"@(#) Copyright (c) 1989, 1993\n\
36	The Regents of the University of California.  All rights reserved.\n";
37#endif /* not lint */
38
39#ifndef lint
40static const char sccsid[] = "@(#)pom.c       8.1 (Berkeley) 5/31/93";
41#endif /* not lint */
42#endif
43#include <sys/cdefs.h>
44__FBSDID("$FreeBSD$");
45
46/*
47 * Phase of the Moon.  Calculates the current phase of the moon.
48 * Based on routines from `Practical Astronomy with Your Calculator',
49 * by Duffett-Smith.  Comments give the section from the book that
50 * particular piece of code was adapted from.
51 *
52 * -- Keith E. Brandt  VIII 1984
53 *
54 */
55
56#include <sys/capsicum.h>
57#include <capsicum_helpers.h>
58
59#include <err.h>
60#include <errno.h>
61#include <stdio.h>
62#include <stdlib.h>
63#include <math.h>
64#include <string.h>
65#include <sysexits.h>
66#include <time.h>
67#include <unistd.h>
68
69#ifndef	PI
70#define	PI	  3.14159265358979323846
71#endif
72#define	EPOCH	  85
73#define	EPSILONg  279.611371	/* solar ecliptic long at EPOCH */
74#define	RHOg	  282.680403	/* solar ecliptic long of perigee at EPOCH */
75#define	ECCEN	  0.01671542	/* solar orbit eccentricity */
76#define	lzero	  18.251907	/* lunar mean long at EPOCH */
77#define	Pzero	  192.917585	/* lunar mean long of perigee at EPOCH */
78#define	Nzero	  55.204723	/* lunar mean long of node at EPOCH */
79#define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
80
81static void	adj360(double *);
82static double	dtor(double);
83static double	potm(double);
84static void	usage(char *progname);
85
86int
87main(int argc, char **argv)
88{
89	time_t tt;
90	struct tm GMT, tmd;
91	double days, today, tomorrow;
92	int ch, cnt, pflag = 0;
93	char *odate = NULL, *otime = NULL;
94	char *progname = argv[0];
95
96	if (caph_limit_stdio() < 0)
97		err(1, "unable to limit capabitilities for stdio");
98
99	caph_cache_catpages();
100	if (caph_enter() < 0)
101		err(1, "unable to enter capability mode");
102
103	while ((ch = getopt(argc, argv, "d:pt:")) != -1)
104		switch (ch) {
105		case 'd':
106			odate = optarg;
107			break;
108		case 'p':
109			pflag = 1;
110			break;
111		case 't':
112			otime = optarg;
113			break;
114		default:
115			usage(progname);
116		}
117
118        argc -= optind;
119	argv += optind;
120
121	if (argc)
122		usage(progname);
123
124	/* Adjust based on users preferences */
125	time(&tt);
126	if (otime != NULL || odate != NULL) {
127		/* Save today in case -d isn't specified */
128		localtime_r(&tt, &tmd);
129
130		if (odate != NULL) {
131			tmd.tm_year = strtol(odate, NULL, 10) - 1900;
132			tmd.tm_mon = strtol(odate + 5, NULL, 10) - 1;
133			tmd.tm_mday = strtol(odate + 8, NULL, 10);
134			/* Use midnight as the middle of the night */
135			tmd.tm_hour = 0;
136			tmd.tm_min = 0;
137			tmd.tm_sec = 0;
138			tmd.tm_isdst = -1;
139		}
140		if (otime != NULL) {
141			tmd.tm_hour = strtol(otime, NULL, 10);
142			tmd.tm_min = strtol(otime + 3, NULL, 10);
143			tmd.tm_sec = strtol(otime + 6, NULL, 10);
144			tmd.tm_isdst = -1;
145		}
146		tt = mktime(&tmd);
147	}
148
149	gmtime_r(&tt, &GMT);
150	days = (GMT.tm_yday + 1) + ((GMT.tm_hour +
151	    (GMT.tm_min / 60.0) + (GMT.tm_sec / 3600.0)) / 24.0);
152	for (cnt = EPOCH; cnt < GMT.tm_year; ++cnt)
153		days += isleap(1900 + cnt) ? 366 : 365;
154	today = potm(days);
155	if (pflag) {
156		(void)printf("%1.0f\n", today);
157		return (0);
158	}
159	(void)printf("The Moon is ");
160	if (today >= 99.5)
161		(void)printf("Full\n");
162	else if (today < 0.5)
163		(void)printf("New\n");
164	else {
165		tomorrow = potm(days + 1);
166		if (today >= 49.5 && today < 50.5)
167			(void)printf("%s\n", tomorrow > today ?
168			    "at the First Quarter" : "at the Last Quarter");
169		else {
170			(void)printf("%s ", tomorrow > today ?
171			    "Waxing" : "Waning");
172			if (today > 50)
173				(void)printf("Gibbous (%1.0f%% of Full)\n",
174				    today);
175			else if (today < 50)
176				(void)printf("Crescent (%1.0f%% of Full)\n",
177				    today);
178		}
179	}
180
181	return 0;
182}
183
184/*
185 * potm --
186 *	return phase of the moon
187 */
188static double
189potm(double days)
190{
191	double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
192	double A4, lprime, V, ldprime, D, Nm;
193
194	N = 360 * days / 365.2422;				/* sec 42 #3 */
195	adj360(&N);
196	Msol = N + EPSILONg - RHOg;				/* sec 42 #4 */
197	adj360(&Msol);
198	Ec = 360 / PI * ECCEN * sin(dtor(Msol));		/* sec 42 #5 */
199	LambdaSol = N + Ec + EPSILONg;				/* sec 42 #6 */
200	adj360(&LambdaSol);
201	l = 13.1763966 * days + lzero;				/* sec 61 #4 */
202	adj360(&l);
203	Mm = l - (0.1114041 * days) - Pzero;			/* sec 61 #5 */
204	adj360(&Mm);
205	Nm = Nzero - (0.0529539 * days);			/* sec 61 #6 */
206	adj360(&Nm);
207	Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm));	/* sec 61 #7 */
208	Ac = 0.1858 * sin(dtor(Msol));				/* sec 61 #8 */
209	A3 = 0.37 * sin(dtor(Msol));
210	Mmprime = Mm + Ev - Ac - A3;				/* sec 61 #9 */
211	Ec = 6.2886 * sin(dtor(Mmprime));			/* sec 61 #10 */
212	A4 = 0.214 * sin(dtor(2 * Mmprime));			/* sec 61 #11 */
213	lprime = l + Ev + Ec - Ac + A4;				/* sec 61 #12 */
214	V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol)));	/* sec 61 #13 */
215	ldprime = lprime + V;					/* sec 61 #14 */
216	D = ldprime - LambdaSol;				/* sec 63 #2 */
217	return(50 * (1 - cos(dtor(D))));			/* sec 63 #3 */
218}
219
220/*
221 * dtor --
222 *	convert degrees to radians
223 */
224static double
225dtor(double deg)
226{
227
228	return(deg * PI / 180);
229}
230
231/*
232 * adj360 --
233 *	adjust value so 0 <= deg <= 360
234 */
235static void
236adj360(double *deg)
237{
238
239	for (;;)
240		if (*deg < 0)
241			*deg += 360;
242		else if (*deg > 360)
243			*deg -= 360;
244		else
245			break;
246}
247
248static void
249usage(char *progname)
250{
251
252	fprintf(stderr, "Usage: %s [-p] [-d yyyy.mm.dd] [-t hh:mm:ss]\n",
253	    progname);
254	exit(EX_USAGE);
255}
256