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REDUCE.C
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C/C++ Source or Header
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1990-09-13
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2KB
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64 lines
#include <math.h>
#include "astro.h"
/* convert those orbital elements that change from epoch mjd0 to epoch mjd.
*/
reduce_elements (mjd0, mjd, inc0, ap0, om0, inc, ap, om)
double mjd0; /* initial epoch */
double mjd; /* desired epoch */
double inc0; /* initial inclination, rads */
double ap0; /* initial argument of perihelion, as an mjd */
double om0; /* initial long of ascending node, rads */
double *inc; /* desired inclination, rads */
double *ap; /* desired epoch of perihelion, as an mjd */
double *om; /* desired long of ascending node, rads */
{
double t0, t1;
double tt, tt2, t02, tt3;
double eta, th, th0;
double a, b;
double dap;
double cinc, sinc;
double ot, sot, cot, ot1;
double seta, ceta;
t0 = mjd0/365250.0;
t1 = mjd/365250.0;
tt = t1-t0;
tt2 = tt*tt;
t02 = t0*t0;
tt3 = tt*tt2;
eta = (471.07-6.75*t0+.57*t02)*tt+(.57*t0-3.37)*tt2+.05*tt3;
th0 = 32869.0*t0+56*t02-(8694+55*t0)*tt+3*tt2;
eta = degrad(eta/3600.0);
th0 = degrad((th0/3600.0)+173.950833);
th = (50256.41+222.29*t0+.26*t02)*tt+(111.15+.26*t0)*tt2+.1*tt3;
th = th0+degrad(th/3600.0);
cinc = cos(inc0);
sinc = sin(inc0);
ot = om0-th0;
sot = sin(ot);
cot = cos(ot);
seta = sin(eta);
ceta = cos(eta);
a = sinc*sot;
b = ceta*sinc*cot-seta*cinc;
ot1 = atan(a/b);
if (b<0) ot1 += PI;
b = sinc*ceta-cinc*seta*cot;
a = -1*seta*sot;
dap = atan(a/b);
if (b<0) dap += PI;
*ap = ap0+dap;
range (ap, 2*PI);
*om = ot1+th;
range (om, 2*PI);
if (inc0<.175)
*inc = asin(a/sin(dap));
else
*inc = 1.570796327-asin((cinc*ceta)+(sinc*seta*cot));
}