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Hi George

You can find the low precision values of the Ecliptic Latitude and Longitude 
of the Moon in the Astronomical Almanac.  The published values are to two 
decimal places of degrees.

If you go to
http://asa.usno.navy.mil/SecD/LunarPoly.html
you will find the co-efficients to the Lunar Polynomials.

When you use them, you will derive the high precision RA, declination and HP.  
The results can be converted (as you point out) to Ecliptic Latitude and 
Longitude.

One issue I found, however, is that I had to add 180 degrees the ATAN function 
provided to obtain correlation.  That is, the equation reads

Ecliptic Long = 180 + atan(((sin(RA)cos(ObliquityEcliptic) + tan(dec)sin(ObliquityEcliptic))/cos(RA))

EXAMPLE
7June09

Polynomial Coefficients
RA
245.4302085
 13.3954668
  0.0795003
 -0.0392653
 -0.0030594
  0.0007151

Dec
-25.6866823
 -1.3663138
  0.6207190
  0.0099947
 -0.0035461
 -0.0000342

HP
 0.91121504
-0.00532634
 0.00057368
 0.00001426
 0.00000293

YIELDS (at midnight, we can easily shift the time)
RA 245.4302085
Dec -25.6866823
HP 0.91121504

CONVERTING TO ECLIPTIC LAT LONG
Elip Lat -4.110005927
Elip Long 247.9338333


The Astronomical Almanac 2009 publishes the 0h TT data as

RA 16h 21m 43.25s
Dec -25d 41m 12.1s
HP 54m 40.37s

Ecliptic Lat -4.11
Ecliptic Long 247.93

It seems to be worth while to go through the polynomial expansion, 
particularly if we intend to include the Limb Effects (mountains) like Frank 
suggests.

Best Regards
Brad



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