Geocentric Conjunction      10:11:46.79 TDT     J.D. = 2453646.924847
 of Sun & Moon in R.A.:   (=10:10:41.99 UT)

      Instant of            10:32:47.22 TDT     J.D. = 2453646.939435
   Greatest Eclipse:      (=10:31:42.42 UT)


Geocentric Coordinates of Sun & Moon at Greatest Eclipse (DE200/LE200):

Sun:       R.A. = 12h37m55.021s       Moon:      R.A. = 12h38m30.321s
           Dec. =-04°05´04.22"                   Dec. =-03°49´04.75"
  Semi-Diameter =    15´59.14"          Semi-Diameter =    15´05.26"
    Eq.Hor.Par. =       08.79"            Eq.Hor.Par. =  0°55´22.09"
         Δ R.A. =        9.082s/h              Δ R.A. =      109.997s/h
         Δ Dec. =      -57.97"/h               Δ Dec. =     -888.16"/h


Lunar Radius   k1 = 0.2725076 (Penumbra)        Shift in      Δb =  0.00"
 Constants:    k2 = 0.2722810 (Umbra)       Lunar Position:   Δl =  0.00"

Geocentric Libration:   l =  -4.0°       Brown Lun. No. = 1024
(Optical + Physical)    b =  -0.3°         Saros Series =  134 (43/71)
                        c =  21.5°            Ephemeris = (DE200/LE200)

Eclipse Magnitude = 0.95758        Gamma = 0.33058        ΔT =    64.8 s


Polynomial Besselian Elements for:   2005 Oct 03   11:00:00.0 TDT  (=t0)

  n        x          y         d          l1         l2          µ

  0   0.3660487  0.1758198 -4.0922399  0.5626813  0.0164416 347.754791
  1   0.4554799 -0.2508070 -0.0154901 -0.0001022 -0.0001017  15.004341
  2   0.0000099  0.0000075  0.0000007 -0.0000103 -0.0000103  -0.000001
  3  -0.0000054  0.0000032  0.0000000  0.0000000  0.0000000   0.000000

                 Tan f1 = 0.0046741    Tan f2 = 0.0046508

At time t1 (decimal hours), each Besselian element is evaluated by:

            a = a0 + a1*t + a2*t2 + a3*t3    (or a = Σ [an*tn]; n = 0 to 3)

    where:  a = x, y, d, l1, l2, or μ
            t = t1 - t0  (decimal hours) and t0 = 11.000


The Besselian elements were derived from a least-squares fit to elements
calculated at five uniformly spaced times over a six hour period centered at t0.
The Besselian elements are valid over the period  8.00  ≤ t0 ≤ 14.00 TDT.

Note that all times are expressed in Terrestrial Dynamical Time (TDT).

       Saros Series 134:  Member 43 of 71 eclipses in series.

All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy. Permission is freely granted to reproduce this data when accompanied by an acknowledgment:

Eclipse Predictions & WebMaster: Fred Espenak Planetary Systems Branch - Code 693 e-mail: espenak@gsfc.nasa.gov NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771 USA