pom.c revision 15949 
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. 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.
22 *
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
27 * FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
28 * DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS
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
33 * SUCH DAMAGE.
34 */
35
36#ifndef lint
37static const char copyright[] =
38"@(#) Copyright (c) 1989, 1993\n\
39	The Regents of the University of California.  All rights reserved.\n";
40#endif /* not lint */
41
42#ifndef lint
43static const char sccsid[] = "@(#)pom.c       8.1 (Berkeley) 5/31/93";
44#endif /* not lint */
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 <time.h>
57#include <stdio.h>
58#include <math.h>
59
60#define	PI	  3.141592654
61#define	EPOCH	  85
62#define	EPSILONg  279.611371	/* solar ecliptic long at EPOCH */
63#define	RHOg	  282.680403	/* solar ecliptic long of perigee at EPOCH */
64#define	ECCEN	  0.01671542	/* solar orbit eccentricity */
65#define	lzero	  18.251907	/* lunar mean long at EPOCH */
66#define	Pzero	  192.917585	/* lunar mean long of perigee at EPOCH */
67#define	Nzero	  55.204723	/* lunar mean long of node at EPOCH */
68#define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
69
70double dtor(), potm();
71void adj360();
72
73void main()
74{
75	time_t tt;
76	struct tm *GMT;
77	double days, today, tomorrow;
78	int cnt;
79
80	(void) time(&tt);
81	GMT = gmtime(&tt);
82	days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
83	    (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
84	for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
85		days += isleap(cnt) ? 366 : 365;
86	today = potm(days) + .5;
87	(void)printf("The Moon is ");
88	if ((int)today == 100)
89		(void)printf("Full\n");
90	else if (!(int)today)
91		(void)printf("New\n");
92	else {
93		tomorrow = potm(days + 1);
94		if ((int)today == 50)
95			(void)printf("%s\n", tomorrow > today ?
96			    "at the First Quarter" : "at the Last Quarter");
97		else {
98			(void)printf("%s ", tomorrow > today ?
99			    "Waxing" : "Waning");
100			if (today > 50)
101				(void)printf("Gibbous (%1.0f%% of Full)\n",
102				    today);
103			else if (today < 50)
104				(void)printf("Crescent (%1.0f%% of Full)\n",
105				    today);
106		}
107	}
108}
109
110/*
111 * potm --
112 *	return phase of the moon
113 */
114double
115potm(days)
116	double days;
117{
118	double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
119	double A4, lprime, V, ldprime, D, Nm;
120
121	N = 360 * days / 365.2422;				/* sec 42 #3 */
122	adj360(&N);
123	Msol = N + EPSILONg - RHOg;				/* sec 42 #4 */
124	adj360(&Msol);
125	Ec = 360 / PI * ECCEN * sin(dtor(Msol));		/* sec 42 #5 */
126	LambdaSol = N + Ec + EPSILONg;				/* sec 42 #6 */
127	adj360(&LambdaSol);
128	l = 13.1763966 * days + lzero;				/* sec 61 #4 */
129	adj360(&l);
130	Mm = l - (0.1114041 * days) - Pzero;			/* sec 61 #5 */
131	adj360(&Mm);
132	Nm = Nzero - (0.0529539 * days);			/* sec 61 #6 */
133	adj360(&Nm);
134	Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm));	/* sec 61 #7 */
135	Ac = 0.1858 * sin(dtor(Msol));				/* sec 61 #8 */
136	A3 = 0.37 * sin(dtor(Msol));
137	Mmprime = Mm + Ev - Ac - A3;				/* sec 61 #9 */
138	Ec = 6.2886 * sin(dtor(Mmprime));			/* sec 61 #10 */
139	A4 = 0.214 * sin(dtor(2 * Mmprime));			/* sec 61 #11 */
140	lprime = l + Ev + Ec - Ac + A4;				/* sec 61 #12 */
141	V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol)));	/* sec 61 #13 */
142	ldprime = lprime + V;					/* sec 61 #14 */
143	D = ldprime - LambdaSol;				/* sec 63 #2 */
144	return(50 * (1 - cos(dtor(D))));			/* sec 63 #3 */
145}
146
147/*
148 * dtor --
149 *	convert degrees to radians
150 */
151double
152dtor(deg)
153	double deg;
154{
155	return(deg * PI / 180);
156}
157
158/*
159 * adj360 --
160 *	adjust value so 0 <= deg <= 360
161 */
162void
163adj360(deg)
164	double *deg;
165{
166	for (;;)
167		if (*deg < 0)
168			*deg += 360;
169		else if (*deg > 360)
170			*deg -= 360;
171		else
172			break;
173}
174