mars.c

Examples of how to use planetary functions.

/*
This program is free software; you can redistribute it and/or modify
it under the terms of the GNU Library General Public License as published by
the Free Software Foundation; either version 2 of the License, or
(at your option) any later version.
 
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
GNU General Public License for more details.
 
You should have received a copy of the GNU General Public License
along with this program; if not, write to the Free Software
Foundation, Inc., 59 Temple Place - Suite 330, Boston, MA 02111-1307, USA. 
 
Copyright (C) 2003 Liam Girdwood <lgirdwood@gmail.com>
 
 
A simple example showing some planetary calculations.
 
*/
 
#include <stdio.h>
#include <libnova/mars.h>
#include <libnova/julian_day.h>
#include <libnova/rise_set.h>
#include <libnova/transform.h>
#include <libnova/utility.h>
 
static void print_date(char *title, struct ln_zonedate *date)
{
    fprintf(stdout, "\n%s\n",title);
    fprintf(stdout, " Year    : %d\n", date->years);
    fprintf(stdout, " Month   : %d\n", date->months);
    fprintf(stdout, " Day     : %d\n", date->days);
    fprintf(stdout, " Hours   : %d\n", date->hours);
    fprintf(stdout, " Minutes : %d\n", date->minutes);
    fprintf(stdout, " Seconds : %f\n", date->seconds);
}
 
int main(int argc, const char *argv[])
{
    struct ln_helio_posn pos;
    struct lnh_equ_posn hequ;
    struct ln_equ_posn equ;
    struct ln_rst_time rst;
    struct ln_zonedate rise, set, transit;
    struct ln_lnlat_posn observer;
    double JD;
    double au;
    
    /* observers location (Edinburgh), used to calc rst */
    observer.lat = 55.92; /* 55.92 N */
    observer.lng = -3.18; /* 3.18 W */
    
    /* get Julian day from local time */
    JD = ln_get_julian_from_sys();  
    fprintf(stdout, "JD %f\n", JD);
    
    /* longitude, latitude and radius vector */
    ln_get_mars_helio_coords(JD, &pos); 
    fprintf(stdout, "Mars L %f B %f R %f\n", pos.L, pos.B, pos.R);
    
    /* RA, DEC */
    ln_get_mars_equ_coords(JD, &equ);
    ln_equ_to_hequ(&equ, &hequ);
    fprintf(stdout, "Mars RA %d:%d:%f Dec %d:%d:%f\n",
        hequ.ra.hours, hequ.ra.minutes, hequ.ra.seconds,
        hequ.dec.degrees, hequ.dec.minutes, hequ.dec.seconds);
    
    /* Earth - Mars dist AU */
    au = ln_get_mars_earth_dist(JD);
    fprintf(stdout, "mars -> Earth dist (AU) %f\n",au);
    
    /* Sun - Mars Dist AU */
    au = ln_get_mars_solar_dist(JD);
    fprintf(stdout, "mars -> Sun dist (AU) %f\n",au);
    
    /* Mars disk, magnitude and phase */
    au = ln_get_mars_disk(JD);
    fprintf(stdout, "mars -> illuminated disk %f\n",au);
    au = ln_get_mars_magnitude(JD);
    fprintf(stdout, "mars -> magnitude %f\n",au);
    au = ln_get_mars_phase(JD);
    fprintf(stdout, "mars -> phase %f\n",au);
    
        /* rise, set and transit time */
    if (ln_get_mars_rst(JD, &observer, &rst) != 0)
        fprintf(stdout, "Mars is circumpolar\n");
    else {
        ln_get_local_date(rst.rise, &rise);
        ln_get_local_date(rst.transit, &transit);
        ln_get_local_date(rst.set, &set);
        print_date("Rise", &rise);
        print_date("Transit", &transit);
        print_date("Set", &set);
    }
    
    return 0;
}