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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-07-08 20:46:52 -0400
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-07-08 20:46:52 -0400
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+.help rdplan Jun99 "Slalib Package"
+.nf
+
+ SUBROUTINE slRDPL (DATE, NP, ELONG, PHI, RA, DEC, DIAM)
+
+ - - - - - - -
+ R D P L
+ - - - - - - -
+
+ Approximate topocentric apparent RA,Dec of a planet, and its
+ angular diameter.
+
+ Given:
+ DATE d MJD of observation (JD - 2400000.5)
+ NP i planet: 1 = Mercury
+ 2 = Venus
+ 3 = Moon
+ 4 = Mars
+ 5 = Jupiter
+ 6 = Saturn
+ 7 = Uranus
+ 8 = Neptune
+ 9 = Pluto
+ else = Sun
+ ELONG,PHI d observer's east longitude and geodetic
+ latitude (radians)
+
+ Returned:
+ RA,DEC d RA, Dec (topocentric apparent, radians)
+ DIAM d angular diameter (equatorial, radians)
+
+ Notes:
+
+ 1 The date is in a dynamical timescale (TDB, formerly ET) and is
+ in the form of a Modified Julian Date (JD-2400000.5). For all
+ practical purposes, TT can be used instead of TDB, and for many
+ applications UT will do (except for the Moon).
+
+ 2 The longitude and latitude allow correction for geocentric
+ parallax. This is a major effect for the Moon, but in the
+ context of the limited accuracy of the present routine its
+ effect on planetary positions is small (negligible for the
+ outer planets). Geocentric positions can be generated by
+ appropriate use of the routines slDMON and slPLNT.
+
+ 3 The direction accuracy (arcsec, 1000-3000AD) is of order:
+
+ Sun 5
+ Mercury 2
+ Venus 10
+ Moon 30
+ Mars 50
+ Jupiter 90
+ Saturn 90
+ Uranus 90
+ Neptune 10
+ Pluto 1 (1885-2099AD only)
+
+ The angular diameter accuracy is about 0.4% for the Moon,
+ and 0.01% or better for the Sun and planets.
+
+ See the slPLNT routine for references.
+
+ Called: slGMST, slDT, slEPJ, slDMON, slPVOB, slPRNU,
+ slPLNT, slDMXV, slDC2S, slDA2P
+
+ P.T.Wallace Starlink 26 May 1997
+
+ Copyright (C) 1997 Rutherford Appleton Laboratory
+ Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+
+.fi
+.endhelp