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+/*
+ * 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. 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.
+ */
+
+#if 0
+#ifndef lint
+static const char copyright[] =
+"@(#) Copyright (c) 1989, 1993\n\
+ The Regents of the University of California. All rights reserved.\n";
+#endif /* not lint */
+
+#ifndef lint
+static const char sccsid[] = "@(#)pom.c 8.1 (Berkeley) 5/31/93";
+#endif /* not lint */
+#endif
+#include <sys/cdefs.h>
+__FBSDID("$FreeBSD$");
+
+/*
+ * 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 <stdio.h>
+#include <stdlib.h>
+#include <math.h>
+#include <string.h>
+#include <sysexits.h>
+#include <time.h>
+#include <unistd.h>
+
+#ifndef PI
+#define PI 3.14159265358979323846
+#endif
+#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 */
+#define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
+
+static void adj360(double *);
+static double dtor(double);
+static double potm(double);
+static void usage(char *progname);
+
+int
+main(int argc, char **argv)
+{
+ time_t tt;
+ struct tm GMT, tmd;
+ double days, today, tomorrow;
+ int ch, cnt, pflag = 0;
+ char *odate = NULL, *otime = NULL;
+ char *progname = argv[0];
+
+ while ((ch = getopt(argc, argv, "d:pt:")) != -1)
+ switch (ch) {
+ case 'd':
+ odate = optarg;
+ break;
+ case 'p':
+ pflag = 1;
+ break;
+ case 't':
+ otime = optarg;
+ break;
+ default:
+ usage(progname);
+ }
+
+ argc -= optind;
+ argv += optind;
+
+ if (argc)
+ usage(progname);
+
+ /* Adjust based on users preferences */
+ time(&tt);
+ if (otime != NULL || odate != NULL) {
+ /* Save today in case -d isn't specified */
+ localtime_r(&tt, &tmd);
+
+ if (odate != NULL) {
+ tmd.tm_year = strtol(odate, NULL, 10) - 1900;
+ tmd.tm_mon = strtol(odate + 5, NULL, 10) - 1;
+ tmd.tm_mday = strtol(odate + 8, NULL, 10);
+ /* Use midnight as the middle of the night */
+ tmd.tm_hour = 0;
+ tmd.tm_min = 0;
+ tmd.tm_sec = 0;
+ }
+ if (otime != NULL) {
+ tmd.tm_hour = strtol(otime, NULL, 10);
+ tmd.tm_min = strtol(otime + 3, NULL, 10);
+ tmd.tm_sec = strtol(otime + 6, NULL, 10);
+ }
+ tt = mktime(&tmd);
+ }
+
+ gmtime_r(&tt, &GMT);
+ 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(1900 + cnt) ? 366 : 365;
+ today = potm(days) + .5;
+ if (pflag) {
+ (void)printf("%1.0f\n", today);
+ return (0);
+ }
+ (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);
+ }
+ }
+
+ return 0;
+}
+
+/*
+ * potm --
+ * return phase of the moon
+ */
+static double
+potm(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
+ */
+static double
+dtor(double deg)
+{
+
+ return(deg * PI / 180);
+}
+
+/*
+ * adj360 --
+ * adjust value so 0 <= deg <= 360
+ */
+static void
+adj360(double *deg)
+{
+
+ for (;;)
+ if (*deg < 0)
+ *deg += 360;
+ else if (*deg > 360)
+ *deg -= 360;
+ else
+ break;
+}
+
+static void
+usage(char *progname)
+{
+
+ fprintf(stderr, "Usage: %s [-p] [-d yyyy.mm.dd] [-t hh:mm:ss]\n",
+ progname);
+ exit(EX_USAGE);
+}
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