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SUBROUTINE slPVUE (PV, DATE, PMASS, U, JSTAT)
*+
* - - - - - -
* P V U E
* - - - - - -
*
* Construct a universal element set based on an instantaneous position
* and velocity.
*
* Given:
* PV d(6) heliocentric x,y,z,xdot,ydot,zdot of date,
* (AU,AU/s; Note 1)
* DATE d date (TT Modified Julian Date = JD-2400000.5)
* PMASS d mass of the planet (Sun=1; Note 2)
*
* Returned:
* U d(13) universal orbital elements (Note 3)
*
* (1) combined mass (M+m)
* (2) total energy of the orbit (alpha)
* (3) reference (osculating) epoch (t0)
* (4-6) position at reference epoch (r0)
* (7-9) velocity at reference epoch (v0)
* (10) heliocentric distance at reference epoch
* (11) r0.v0
* (12) date (t)
* (13) universal eccentric anomaly (psi) of date, approx
*
* JSTAT i status: 0 = OK
* -1 = illegal PMASS
* -2 = too close to Sun
* -3 = too slow
*
* Notes
*
* 1 The PV 6-vector can be with respect to any chosen inertial frame,
* and the resulting universal-element set will be with respect to
* the same frame. A common choice will be mean equator and ecliptic
* of epoch J2000.
*
* 2 The mass, PMASS, is important only for the larger planets. For
* most purposes (e.g. asteroids) use 0D0. Values less than zero
* are illegal.
*
* 3 The "universal" elements are those which define the orbit for the
* purposes of the method of universal variables (see reference).
* They consist of the combined mass of the two bodies, an epoch,
* and the position and velocity vectors (arbitrary reference frame)
* at that epoch. The parameter set used here includes also various
* quantities that can, in fact, be derived from the other
* information. This approach is taken to avoiding unnecessary
* computation and loss of accuracy. The supplementary quantities
* are (i) alpha, which is proportional to the total energy of the
* orbit, (ii) the heliocentric distance at epoch, (iii) the
* outwards component of the velocity at the given epoch, (iv) an
* estimate of psi, the "universal eccentric anomaly" at a given
* date and (v) that date.
*
* Reference: Everhart, E. & Pitkin, E.T., Am.J.Phys. 51, 712, 1983.
*
* P.T.Wallace Starlink 18 March 1999
*
* Copyright (C) 1999 Rutherford Appleton Laboratory
*
* License:
* This program is free software; you can redistribute it and/or modify
* it under the terms of the GNU 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 (see SLA_CONDITIONS); if not, write to the
* Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor,
* Boston, MA 02110-1301 USA
*
* Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
*-
IMPLICIT NONE
DOUBLE PRECISION PV(6),DATE,PMASS,U(13)
INTEGER JSTAT
* Gaussian gravitational constant (exact)
DOUBLE PRECISION GCON
PARAMETER (GCON=0.01720209895D0)
* Canonical days to seconds
DOUBLE PRECISION CD2S
PARAMETER (CD2S=GCON/86400D0)
* Minimum allowed distance (AU) and speed (AU per canonical day)
DOUBLE PRECISION RMIN,VMIN
PARAMETER (RMIN=1D-3,VMIN=1D-3)
DOUBLE PRECISION T0,CM,X,Y,Z,XD,YD,ZD,R,V2,V,ALPHA,RDV
* Reference epoch.
T0 = DATE
* Combined mass (mu=M+m).
IF (PMASS.LT.0D0) GO TO 9010
CM = 1D0+PMASS
* Unpack the state vector, expressing velocity in AU per canonical day.
X = PV(1)
Y = PV(2)
Z = PV(3)
XD = PV(4)/CD2S
YD = PV(5)/CD2S
ZD = PV(6)/CD2S
* Heliocentric distance, and speed.
R = SQRT(X*X+Y*Y+Z*Z)
V2 = XD*XD+YD*YD+ZD*ZD
V = SQRT(V2)
* Reject unreasonably small values.
IF (R.LT.RMIN) GO TO 9020
IF (V.LT.VMIN) GO TO 9030
* Total energy of the orbit.
ALPHA = V2-2D0*CM/R
* Outward component of velocity.
RDV = X*XD+Y*YD+Z*ZD
* Construct the universal-element set.
U(1) = CM
U(2) = ALPHA
U(3) = T0
U(4) = X
U(5) = Y
U(6) = Z
U(7) = XD
U(8) = YD
U(9) = ZD
U(10) = R
U(11) = RDV
U(12) = T0
U(13) = 0D0
* Exit.
JSTAT = 0
GO TO 9999
* Negative PMASS.
9010 CONTINUE
JSTAT = -1
GO TO 9999
* Too close.
9020 CONTINUE
JSTAT = -2
GO TO 9999
* Too slow.
9030 CONTINUE
JSTAT = -3
9999 CONTINUE
END
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