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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
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+ by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds
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+<H2><A NAME="SECTION0004117000000000000000">SLA_MOON - Approx Moon Pos/Vel</A>
+<A NAME="xref_SLA_MOON">&#160;</A><A NAME="SLA_MOON">&#160;</A>
+</H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Approximate geocentric position and velocity of the Moon
+(single precision).
+<P> <DT><STRONG>CALL:</STRONG>
+<DD><TT>CALL sla_MOON (IY, ID, FD, PV)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>IY</EM></TD>
+<TH ALIGN="LEFT"><B>I</B></TH>
+<TD ALIGN="LEFT" NOWRAP>year</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>ID</EM></TD>
+<TD ALIGN="LEFT"><B>I</B></TD>
+<TD ALIGN="LEFT" NOWRAP>day in year (1 = Jan 1st)</TD>
+</TR>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>FD</EM></TD>
+<TD ALIGN="LEFT"><B>R </B></TD>
+<TD ALIGN="LEFT" NOWRAP>fraction of day</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>PV</EM></TD>
+<TH ALIGN="LEFT"><B>R(6)</B></TH>
+<TD ALIGN="LEFT" NOWRAP>Moon <IMG WIDTH="106" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img51.gif"
+ ALT="$[\,x,y,z,\dot{x},\dot{y},\dot{z}\,]$">, mean equator and equinox of
+date (AU, AU&nbsp;s<SUP>-1</SUP>)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>The date and time is TDB (loosely ET) in a Julian calendar
+which has been aligned to the ordinary Gregorian
+calendar for the interval 1900 March 1 to 2100 February 28.
+ The year and day can be obtained by calling sla_CALYD or
+ sla_CLYD.
+ <DT>2.
+<DD>The position is accurate to better than 0.5&nbsp;arcminute
+ in direction and 1000&nbsp;km in distance. The velocity
+ is accurate to better than
+ <IMG WIDTH="23" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
+ SRC="img83.gif"
+ ALT="$0\hspace{-0.05em}^{'\hspace{-0.1em}'}\hspace{-0.4em}.5$"> per hour in direction
+ and 4&nbsp;metres per socond in distance. (RMS figures with respect
+ to JPL DE200 for the interval 1960-2025 are <IMG WIDTH="25" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
+ SRC="img126.gif"
+ ALT="$14\hspace{-0.05em}^{'\hspace{-0.1em}'}$"> and
+<P> <IMG WIDTH="23" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
+ SRC="img76.gif"
+ ALT="$0\hspace{-0.05em}^{'\hspace{-0.1em}'}\hspace{-0.4em}.2$"> per hour in longitude, <IMG WIDTH="17" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
+ SRC="img127.gif"
+ ALT="$9\hspace{-0.05em}^{'\hspace{-0.1em}'}$"> and
+ <IMG WIDTH="23" HEIGHT="18" ALIGN="BOTTOM" BORDER="0"
+ SRC="img76.gif"
+ ALT="$0\hspace{-0.05em}^{'\hspace{-0.1em}'}\hspace{-0.4em}.2$"><P>
+per hour in latitude, 350&nbsp;km and 2&nbsp;metres per second in distance.)
+ Note that the distance accuracy is comparatively poor because this
+ routine is principally intended for computing topocentric direction.
+ <DT>3.
+<DD>This routine is only a partial implementation of the original
+ Meeus algorithm (reference below), which offers 4 times the
+ accuracy in direction and 20 times the accuracy in distance
+ when fully implemented (as it is in sla_DMOON).
+ </DL></DL>
+<P> <DL>
+<DT><STRONG>REFERENCE:</STRONG>
+<DD>Meeus, <I>l'Astronomie</I>, June 1984, p348.
+</DL>
+<BR> <HR>
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+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<ADDRESS>
+<I>SLALIB --- Positional Astronomy Library<BR>Starlink User Note 67<BR>P. T. Wallace<BR>12 October 1999<BR>E-mail:ptw@star.rl.ac.uk</I>
+</ADDRESS>
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