/* $OpenBSD: pom.c,v 1.5 1998/07/26 06:27:39 pjanzen Exp $ */ /* $NetBSD: pom.c,v 1.6 1996/02/06 22:47:29 jtc Exp $ */ /* * Copyright (c) 1989, 1993 * The Regents of the University of California. All rights reserved. * * This code is derived from software posted to USENET. * * Redistribution and use in source and binary forms, with or without * modification, are permitted provided that the following conditions * are met: * 1. Redistributions of source code must retain the above copyright * notice, this list of conditions and the following disclaimer. * 2. Redistributions in binary form must reproduce the above copyright * notice, this list of conditions and the following disclaimer in the * documentation and/or other materials provided with the distribution. * 3. All advertising materials mentioning features or use of this software * must display the following acknowledgement: * This product includes software developed by the University of * California, Berkeley and its contributors. * 4. Neither the name of the University nor the names of its contributors * may be used to endorse or promote products derived from this software * without specific prior written permission. * * THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND * ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE * ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE * FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL * DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS * OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) * HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT * LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY * OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF * SUCH DAMAGE. */ #ifndef lint static char copyright[] = "@(#) Copyright (c) 1989, 1993\n\ The Regents of the University of California. All rights reserved.\n"; #endif /* not lint */ #ifndef lint #if 0 static char sccsid[] = "@(#)pom.c 8.1 (Berkeley) 5/31/93"; #else static char rcsid[] = "$NetBSD: pom.c,v 1.6 1996/02/06 22:47:29 jtc Exp $"; #endif #endif /* not lint */ /* * Phase of the Moon. Calculates the current phase of the moon. * Based on routines from `Practical Astronomy with Your Calculator', * by Duffett-Smith. Comments give the section from the book that * particular piece of code was adapted from. * * -- Keith E. Brandt VIII 1984 * */ #include #include #include #include #include #include #define PI 3.141592654 #define EPOCH 85 #define EPSILONg 279.611371 /* solar ecliptic long at EPOCH */ #define RHOg 282.680403 /* solar ecliptic long of perigee at EPOCH */ #define ECCEN 0.01671542 /* solar orbit eccentricity */ #define lzero 18.251907 /* lunar mean long at EPOCH */ #define Pzero 192.917585 /* lunar mean long of perigee at EPOCH */ #define Nzero 55.204723 /* lunar mean long of node at EPOCH */ double dtor(), potm(), adj360(); main() { struct timeval tp; struct timezone tzp; struct tm *GMT, *gmtime(); time_t tmpt; double days, today, tomorrow; int cnt; /* revoke */ setegid(getgid()); setgid(getgid()); if (gettimeofday(&tp,&tzp)) { (void)fprintf(stderr, "pom: %s\n", strerror(errno)); exit(1); } tmpt = tp.tv_sec; GMT = gmtime(&tmpt); days = (GMT->tm_yday + 1) + ((GMT->tm_hour + (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0); for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt) days += isleap(cnt + 1900) ? 366 : 365; today = potm(days) + .5; (void)printf("The Moon is "); if ((int)today == 100) (void)printf("Full\n"); else if (!(int)today) (void)printf("New\n"); else { tomorrow = potm(days + 1); if ((int)today == 50) (void)printf("%s\n", tomorrow > today ? "at the First Quarter" : "at the Last Quarter"); else { (void)printf("%s ", tomorrow > today ? "Waxing" : "Waning"); if (today > 50) (void)printf("Gibbous (%1.0f%% of Full)\n", today); else if (today < 50) (void)printf("Crescent (%1.0f%% of Full)\n", today); } } exit(0); } /* * potm -- * return phase of the moon */ double potm(days) double days; { double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime; double A4, lprime, V, ldprime, D, Nm; N = 360 * days / 365.2422; /* sec 42 #3 */ adj360(&N); Msol = N + EPSILONg - RHOg; /* sec 42 #4 */ adj360(&Msol); Ec = 360 / PI * ECCEN * sin(dtor(Msol)); /* sec 42 #5 */ LambdaSol = N + Ec + EPSILONg; /* sec 42 #6 */ adj360(&LambdaSol); l = 13.1763966 * days + lzero; /* sec 61 #4 */ adj360(&l); Mm = l - (0.1114041 * days) - Pzero; /* sec 61 #5 */ adj360(&Mm); Nm = Nzero - (0.0529539 * days); /* sec 61 #6 */ adj360(&Nm); Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm)); /* sec 61 #7 */ Ac = 0.1858 * sin(dtor(Msol)); /* sec 61 #8 */ A3 = 0.37 * sin(dtor(Msol)); Mmprime = Mm + Ev - Ac - A3; /* sec 61 #9 */ Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 61 #10 */ A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 61 #11 */ lprime = l + Ev + Ec - Ac + A4; /* sec 61 #12 */ V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 61 #13 */ ldprime = lprime + V; /* sec 61 #14 */ D = ldprime - LambdaSol; /* sec 63 #2 */ return(50 * (1 - cos(dtor(D)))); /* sec 63 #3 */ } /* * dtor -- * convert degrees to radians */ double dtor(deg) double deg; { return(deg * PI / 180); } /* * adj360 -- * adjust value so 0 <= deg <= 360 */ double adj360(deg) double *deg; { for (;;) if (*deg < 0) *deg += 360; else if (*deg > 360) *deg -= 360; else break; }