Geocentric Conjunction 07:39:48.73 TDT J.D. = 2452612.819314 of Sun & Moon in R.A.: (=07:38:44.03 UT) Instant of 07:32:15.65 TDT J.D. = 2452612.814070 Greatest Eclipse: (=07:31:10.95 UT) Geocentric Coordinates of Sun & Moon at Greatest Eclipse (DE200/LE200): Sun: R.A. = 16h41m50.939s Moon: R.A. = 16h41m32.881s Dec. =-22°13´29.20" Dec. =-22°31´05.17" Semi-Diameter = 16´13.60" Semi-Diameter = 16´21.60" Eq.Hor.Par. = 08.92" Eq.Hor.Par. = 1°00´02.27" Æ R.A. = 10.867s/h Æ R.A. = 154.401s/h Æ Dec. = -20.23"/h Æ Dec. = -487.39"/h Lunar Radius k1 = 0.2725076 (Penumbra) Shift in delta b = 0.00" Constants: k2 = 0.2722810 (Umbra) Lunar Position: delta l = 0.00" Geocentric Libration: l = 3.8° Brown Lun. No. = 989 (Optical + Physical) b = 0.5° Saros Series = 142 (22/72) c = 5.7° Ephemeris = (DE200/LE200) Eclipse Magnitude = 1.02437 Gamma =-0.30204 delta T = 64.7 s Polynomial Besselian Elements for: 2002 Dec 04 08:00:00.0 TDT (=t0) n x y d l1 l2 µ 0 0.1861473 -0.3544635 -22.2264977 0.5441862 -0.0019615 302.485046 1 0.5532511 -0.1309133 -0.0052963 0.0000834 0.0000830 14.997272 2 0.0000155 0.0001807 0.0000058 -0.0000125 -0.0000124 -0.000002 3 -0.0000087 0.0000022 0.0000000 0.0000000 0.0000000 0.000000 Tan f1 = 0.0047437 Tan f2 = 0.0047201 At time t1 (decimal hours), each Besselian element is evaluated by: a = a0 + a1*t + a2*t2 + a3*t3 (or a = · [an*tn]; n = 0 to 3) where: a = x, y, d, l1, l2, or µ t = t1 - t0 (decimal hours) and t0 = 8.000 TDT 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. Thus the elements are valid over the period 5.00 < t0 < 11.00 TDT. Note that all times are expressed in Terrestrial Dynamical Time (TDT). Saros Series 142: Member 22 of 72 eclipses in series.
Table adapted from NASA TP 1999-209484 "Total Solar Eclipse of 2002 December 04".
WebMaster: Fred Espenak Planetary Systems Branch - Code 693 e-mail: espenak@gsfc.nasa.gov NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771 USA
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