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pom.c revision 1.11
      1 /*	$NetBSD: pom.c,v 1.11 1998/09/11 14:07:04 hubertf 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 1.11 1998/09/11 14:07:04 hubertf 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  */
     61 
     62 #include <sys/time.h>
     63 #include <err.h>
     64 #include <errno.h>
     65 #include <math.h>
     66 #include <stdio.h>
     67 #include <string.h>
     68 #include <stdlib.h>
     69 #include <tzfile.h>
     70 
     71 #ifndef PI
     72 #define	PI	  3.14159265358979323846
     73 #endif
     74 #define	EPOCH	  85		/* really 1985 */
     75 #define	EPSILONg  279.611371	/* solar ecliptic long at EPOCH */
     76 #define	RHOg	  282.680403	/* solar ecliptic long of perigee at EPOCH */
     77 #define	ECCEN	  0.01671542	/* solar orbit eccentricity */
     78 #define	lzero	  18.251907	/* lunar mean long at EPOCH */
     79 #define	Pzero	  192.917585	/* lunar mean long of perigee at EPOCH */
     80 #define	Nzero	  55.204723	/* lunar mean long of node at EPOCH */
     81 
     82 void	adj360 __P((double *));
     83 double	dtor __P((double));
     84 int	main __P((int, char *[]));
     85 double	potm __P((double));
     86 
     87 int
     88 main(argc, argv)
     89 	int argc;
     90 	char *argv[];
     91 {
     92 	struct timeval tp;
     93 	struct timezone tzp;
     94 	struct tm *GMT;
     95 	time_t tmpt;
     96 	double days, today, tomorrow;
     97 	int cnt;
     98 
     99 	if (argc > 1) {
    100 		tp.tv_sec = atoi(argv[1]);
    101 		tp.tv_usec = 0;
    102 	} else {
    103 		if (gettimeofday(&tp,&tzp))
    104 			err(1, "gettimeofday");
    105 	}
    106 	tmpt = tp.tv_sec;
    107 	GMT = gmtime(&tmpt);
    108 	days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
    109 	    (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
    110 	for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
    111 		days += isleap(cnt + 1900) ? 366 : 365;
    112 	today = potm(days) + .5;
    113 	(void)printf("The Moon is ");
    114 	if ((int)today == 100)
    115 		(void)printf("Full\n");
    116 	else if (!(int)today)
    117 		(void)printf("New\n");
    118 	else {
    119 		tomorrow = potm(days + 1);
    120 		if ((int)today == 50)
    121 			(void)printf("%s\n", tomorrow > today ?
    122 			    "at the First Quarter" : "at the Last Quarter");
    123 		else {
    124 			(void)printf("%s ", tomorrow > today ?
    125 			    "Waxing" : "Waning");
    126 			if (today > 50)
    127 				(void)printf("Gibbous (%1.0f%% of Full)\n",
    128 				    today);
    129 			else if (today < 50)
    130 				(void)printf("Crescent (%1.0f%% of Full)\n",
    131 				    today);
    132 		}
    133 	}
    134 	exit(0);
    135 }
    136 
    137 /*
    138  * potm --
    139  *	return phase of the moon
    140  */
    141 double
    142 potm(days)
    143 	double days;
    144 {
    145 	double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
    146 	double A4, lprime, V, ldprime, D, Nm;
    147 
    148 	N = 360 * days / 365.2422;				/* sec 42 #3 */
    149 	adj360(&N);
    150 	Msol = N + EPSILONg - RHOg;				/* sec 42 #4 */
    151 	adj360(&Msol);
    152 	Ec = 360 / PI * ECCEN * sin(dtor(Msol));		/* sec 42 #5 */
    153 	LambdaSol = N + Ec + EPSILONg;				/* sec 42 #6 */
    154 	adj360(&LambdaSol);
    155 	l = 13.1763966 * days + lzero;				/* sec 61 #4 */
    156 	adj360(&l);
    157 	Mm = l - (0.1114041 * days) - Pzero;			/* sec 61 #5 */
    158 	adj360(&Mm);
    159 	Nm = Nzero - (0.0529539 * days);			/* sec 61 #6 */
    160 	adj360(&Nm);
    161 	Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm));	/* sec 61 #7 */
    162 	Ac = 0.1858 * sin(dtor(Msol));				/* sec 61 #8 */
    163 	A3 = 0.37 * sin(dtor(Msol));
    164 	Mmprime = Mm + Ev - Ac - A3;				/* sec 61 #9 */
    165 	Ec = 6.2886 * sin(dtor(Mmprime));			/* sec 61 #10 */
    166 	A4 = 0.214 * sin(dtor(2 * Mmprime));			/* sec 61 #11 */
    167 	lprime = l + Ev + Ec - Ac + A4;				/* sec 61 #12 */
    168 	V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol)));	/* sec 61 #13 */
    169 	ldprime = lprime + V;					/* sec 61 #14 */
    170 	D = ldprime - LambdaSol;				/* sec 63 #2 */
    171 	return(50 * (1 - cos(dtor(D))));			/* sec 63 #3 */
    172 }
    173 
    174 /*
    175  * dtor --
    176  *	convert degrees to radians
    177  */
    178 double
    179 dtor(deg)
    180 	double deg;
    181 {
    182 	return(deg * PI / 180);
    183 }
    184 
    185 /*
    186  * adj360 --
    187  *	adjust value so 0 <= deg <= 360
    188  */
    189 void
    190 adj360(deg)
    191 	double *deg;
    192 {
    193 	for (;;)
    194 		if (*deg < 0)
    195 			*deg += 360;
    196 		else if (*deg > 360)
    197 			*deg -= 360;
    198 		else
    199 			break;
    200 }
    201