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pom.c revision 1.2
      1 /*
      2  * Copyright (c) 1989 The Regents of the University of California.
      3  * 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
     37 char copyright[] =
     38 "@(#) Copyright (c) 1989 The Regents of the University of California.\n\
     39  All rights reserved.\n";
     40 #endif /* not lint */
     41 
     42 #ifndef lint
     43 /*static char sccsid[] = "from: @(#)pom.c	5.3 (Berkeley) 2/28/91";*/
     44 static char rcsid[] = "$Id: pom.c,v 1.2 1993/08/01 18:53:16 mycroft Exp $";
     45 #endif /* not lint */
     46 
     47 /*
     48  * Phase of the Moon.  Calculates the current phase of the moon.
     49  * Based on routines from `Practical Astronomy with Your Calculator',
     50  * by Duffett-Smith.  Comments give the section from the book that
     51  * particular piece of code was adapted from.
     52  *
     53  * -- Keith E. Brandt  VIII 1984
     54  *
     55  */
     56 
     57 #include <sys/time.h>
     58 #include <stdio.h>
     59 #include <tzfile.h>
     60 #include <math.h>
     61 
     62 #define	PI	  3.141592654
     63 #define	EPOCH	  85
     64 #define	EPSILONg  279.611371	/* solar ecliptic long at EPOCH */
     65 #define	RHOg	  282.680403	/* solar ecliptic long of perigee at EPOCH */
     66 #define	ECCEN	  0.01671542	/* solar orbit eccentricity */
     67 #define	lzero	  18.251907	/* lunar mean long at EPOCH */
     68 #define	Pzero	  192.917585	/* lunar mean long of perigee at EPOCH */
     69 #define	Nzero	  55.204723	/* lunar mean long of node at EPOCH */
     70 
     71 double dtor(), potm(), adj360();
     72 
     73 main()
     74 {
     75 	extern int errno;
     76 	struct timeval tp;
     77 	struct timezone tzp;
     78 	struct tm *GMT, *gmtime();
     79 	double days, today, tomorrow;
     80 	int cnt;
     81 	char *strerror();
     82 
     83 	if (gettimeofday(&tp,&tzp)) {
     84 		(void)fprintf(stderr, "pom: %s\n", strerror(errno));
     85 		exit(1);
     86 	}
     87 	GMT = gmtime(&tp.tv_sec);
     88 	days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
     89 	    (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
     90 	for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
     91 		days += isleap(cnt) ? 366 : 365;
     92 	today = potm(days) + .5;
     93 	(void)printf("The Moon is ");
     94 	if ((int)today == 100)
     95 		(void)printf("Full\n");
     96 	else if (!(int)today)
     97 		(void)printf("New\n");
     98 	else {
     99 		tomorrow = potm(days + 1);
    100 		if ((int)today == 50)
    101 			(void)printf("%s\n", tomorrow > today ?
    102 			    "at the First Quarter" : "at the Last Quarter");
    103 		else {
    104 			(void)printf("%s ", tomorrow > today ?
    105 			    "Waxing" : "Waning");
    106 			if (today > 50)
    107 				(void)printf("Gibbous (%1.0f%% of Full)\n",
    108 				    today);
    109 			else if (today < 50)
    110 				(void)printf("Crescent (%1.0f%% of Full)\n",
    111 				    today);
    112 		}
    113 	}
    114 }
    115 
    116 /*
    117  * potm --
    118  *	return phase of the moon
    119  */
    120 double
    121 potm(days)
    122 	double days;
    123 {
    124 	double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
    125 	double A4, lprime, V, ldprime, D, Nm;
    126 
    127 	N = 360 * days / 365.2422;				/* sec 42 #3 */
    128 	adj360(&N);
    129 	Msol = N + EPSILONg - RHOg;				/* sec 42 #4 */
    130 	adj360(&Msol);
    131 	Ec = 360 / PI * ECCEN * sin(dtor(Msol));		/* sec 42 #5 */
    132 	LambdaSol = N + Ec + EPSILONg;				/* sec 42 #6 */
    133 	adj360(&LambdaSol);
    134 	l = 13.1763966 * days + lzero;				/* sec 61 #4 */
    135 	adj360(&l);
    136 	Mm = l - (0.1114041 * days) - Pzero;			/* sec 61 #5 */
    137 	adj360(&Mm);
    138 	Nm = Nzero - (0.0529539 * days);			/* sec 61 #6 */
    139 	adj360(&Nm);
    140 	Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm));	/* sec 61 #7 */
    141 	Ac = 0.1858 * sin(dtor(Msol));				/* sec 61 #8 */
    142 	A3 = 0.37 * sin(dtor(Msol));
    143 	Mmprime = Mm + Ev - Ac - A3;				/* sec 61 #9 */
    144 	Ec = 6.2886 * sin(dtor(Mmprime));			/* sec 61 #10 */
    145 	A4 = 0.214 * sin(dtor(2 * Mmprime));			/* sec 61 #11 */
    146 	lprime = l + Ev + Ec - Ac + A4;				/* sec 61 #12 */
    147 	V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol)));	/* sec 61 #13 */
    148 	ldprime = lprime + V;					/* sec 61 #14 */
    149 	D = ldprime - LambdaSol;				/* sec 63 #2 */
    150 	return(50 * (1 - cos(dtor(D))));			/* sec 63 #3 */
    151 }
    152 
    153 /*
    154  * dtor --
    155  *	convert degrees to radians
    156  */
    157 double
    158 dtor(deg)
    159 	double deg;
    160 {
    161 	return(deg * PI / 180);
    162 }
    163 
    164 /*
    165  * adj360 --
    166  *	adjust value so 0 <= deg <= 360
    167  */
    168 double
    169 adj360(deg)
    170 	double *deg;
    171 {
    172 	for (;;)
    173 		if (*deg < 0)
    174 			*deg += 360;
    175 		else if (*deg > 360)
    176 			*deg -= 360;
    177 		else
    178 			break;
    179 }
    180