/* 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 <liam@gnova.org> A simple example showing the asteroid Pallas. */ #include <stdio.h> #include <libnova/asteroid.h> #include <libnova/julian_day.h> #include <libnova/rise_set.h> #include <libnova/transform.h> #include <libnova/elliptic_motion.h> /* just prints the date */ void print_date (char * title, struct ln_zonedate* date) { printf ("\n%s\n",title); printf (" Year : %d\n", date->years); printf (" Month : %d\n", date->months); printf (" Day : %d\n", date->days); printf (" Hours : %d\n", date->hours); printf (" Minutes : %d\n", date->minutes); printf (" Seconds : %f\n", date->seconds); } int main (int argc, char * argv[]) { struct ln_rst_time rst; struct ln_zonedate rise, set, transit; struct ln_lnlat_posn observer; struct ln_hrz_posn hrz; struct ln_ell_orbit orbit; struct ln_rect_posn posn; double JD, M_JD; double l,V,dist; struct ln_equ_posn equ_posn; double H, G; double mag, elong, ph; char* M_epoch = "K036A"; /* 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(); printf ("JD (sys) %f\n", JD); /* Pallas orbital parameters * Taken from MPCORB.DAT * 00002 4.13 0.11 K036A 260.69458 310.45917 173.16479 * 34.84989 0.2299839 0.21343771 2.7730346 MPC 24084 * 5482 63 1839-1993 0.55 M-c 28 Bowell 0000 (2) Pallas */ orbit.a = 2.7730346; orbit.e = 0.2299839; orbit.i = 34.84989; orbit.omega = 173.16479; orbit.w = 310.45917; orbit.n =0.21343771; H = 4.13; G = 0.11; /* calc last passage in Perihelion, in julian day */ M_JD = ln_get_julian_from_mpc(M_epoch); orbit.JD = ln_get_ell_last_perihelion (M_JD, 260.69458, orbit.n); printf ("JD (Perihelion) %f\n", orbit.JD); /* calc the earth centered position */ ln_get_ell_geo_rect_posn (&orbit, JD, &posn); printf ("(Geocentric Rect Coords X) for Pallas %f\n", posn.X); printf ("(Geocentric Rect Coords Y) for Pallas %f\n", posn.Y); printf ("(Geocentric Rect Coords Z) for Pallas %f\n", posn.Z); /* calc the sun centered position */ ln_get_ell_helio_rect_posn (&orbit, JD, &posn); printf ("(Heliocentric Rect Coords X) for Pallas %f\n", posn.X); printf ("(Heliocentric Rect Coords Y) for Pallas %f\n", posn.Y); printf ("(Heliocentric Rect Coords Z) for Pallas %f\n", posn.Z); /* get the RA and Dec */ ln_get_ell_body_equ_coords (JD, &orbit, &equ_posn); printf ("(RA) for Pallas %f\n", equ_posn.ra); printf ("(Dec) for Pallas %f\n", equ_posn.dec); /* get Alt, Az */ ln_get_hrz_from_equ (&equ_posn, &observer, JD, &hrz); printf ("Az %f\n",hrz.az); printf ("Alt %f\n", hrz.alt); /* orbit length */ l = ln_get_ell_orbit_len (&orbit); printf ("(Orbit Length) for Pallas in AU %f\n", l); /* orbit velocities */ V = ln_get_ell_orbit_pvel (&orbit); printf ("(Orbit Perihelion Vel) for Pallas in kms %f\n", V); V = ln_get_ell_orbit_avel (&orbit); printf ("(Orbit Aphelion Vel) for Pallas in kms %f\n", V); V = ln_get_ell_orbit_vel (JD, &orbit); printf ("(Orbit Vel JD) for Pallas in kms %f\n", V); /* earth and solar distance */ dist = ln_get_ell_body_solar_dist (JD, &orbit); printf ("Solar Dist (AU) : %f\n", dist); dist = ln_get_ell_body_earth_dist (JD, &orbit); printf ("Earth Dist (AU) : %f\n", dist); /* phase angle, elongation */ ph = ln_get_ell_body_phase_angle(JD, &orbit); printf ("Phase angle : %f\n",ph); elong = ln_get_ell_body_elong(JD, &orbit); printf ("Elongation : %f\n",elong); /* magnitude */ mag = ln_get_asteroid_mag (JD, &orbit, H, G); printf ("Magnitude : %f\n", mag); /* rise, set and transit time */ if (ln_get_ell_body_rst (JD, &observer, &orbit, &rst) == 1) printf ("Pallas 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; }