Astro with some minor changes to placate Unix.

src/cmd/astro/jup.c

@@ -0,0 +1,68 @@
+#include "astro.h"
+
+void
+jup(void)
+{
+	double pturbl, pturbb, pturbr;
+	double lograd;
+	double dele, enom, vnom, nd, sl;
+
+
+	ecc = .0483376 + 163.e-6*capt;
+	incl = 1.308660 - .0055*capt;
+	node = 99.43785 + 1.011*capt;
+	argp = 12.71165 + 1.611*capt;
+	mrad = 5.202803;
+	anom = 225.22165 + .0830912*eday - .0484*capt;
+	motion = 299.1284/3600.;
+
+
+	anom = anom;
+	incl *= radian;
+	node *= radian;
+	argp *= radian;
+	anom = fmod(anom,360.)*radian;
+
+	enom = anom + ecc*sin(anom);
+	do {
+		dele = (anom - enom + ecc * sin(enom)) /
+			(1. - ecc*cos(enom));
+		enom += dele;
+	} while(fabs(dele) > converge);
+	vnom = 2.*atan2(sqrt((1.+ecc)/(1.-ecc))*sin(enom/2.),
+		cos(enom/2.));
+	rad = mrad*(1. - ecc*cos(enom));
+
+	lambda = vnom + argp;
+
+	pturbl = 0.;
+
+	lambda += pturbl*radsec;
+
+	pturbb = 0.;
+
+	pturbr = 0.;
+
+/*
+ *	reduce to the ecliptic
+ */
+
+	nd = lambda - node;
+	lambda = node + atan2(sin(nd)*cos(incl),cos(nd));
+
+	sl = sin(incl)*sin(nd) + pturbb*radsec;
+	beta = atan2(sl, pyth(sl));
+
+	lograd = pturbr*2.30258509;
+	rad *= 1. + lograd;
+
+
+	lambda += 555.*radsec;
+	beta -= 51.*radsec;
+	motion *= radian*mrad*mrad/(rad*rad);
+	semi = 98.47;
+
+	mag = -8.93;
+	helio();
+	geo();
+}