Geocentric Conjunction 17:20:50.88 TDT J.D. = 2449483.222811 of Sun & Moon in R.A.: (=17:19:51.38 UT) Instant of 17:12:26.49 TDT J.D. = 2449483.216973 Greatest Eclipse: (=17:11:26.99 UT) Geocentric Coordinates of Sun & Moon at Greatest Eclipse (DE200/LE200): Sun: R.A. = 3h 9m 27.149s Moon: R.A. = 3h 9m 11.285s Dec. = 17¡ 41« 21.51" Dec. = 18¡ 3« 1.10" Semi-Diameter = 15« 50.22" Semi-Diameter = 14« 44.08" Eq.Hor.Par. = 8.71" Eq.Hor.Par. = 0¡ 54« 4.35" Æ R.A. = 9.772s/h Æ R.A. = 122.984s/h Æ Dec. = 39.06"/h Æ Dec. = 320.89"/h Lunar Radius k1 = 0.2725076 (Penumbra) Shift in Æb = 0.0" Constants: k2 = 0.2722810 (Umbra) Lunar Position: Æl = 0.0" Geocentric Libration: l = -1.6¡ Brown Lun. Nbr. = 1167 (Optical + Physical) b = -0.5¡ Saros Series = 128 (57/73) c = -17.2¡ Ephemeris = (DE200/LE200) Eclipse Magnitude = 0.94314 Gamma = 0.40772 ÆT = 59.5 s Polynomial Besselian Elements for: 10 May 1994 17:00:00.0 TDT (=t0) n x y d l1 l2 µ 0 -0.1734118 0.3836521 17.6861305 0.5669329 0.0206722 75.905975 1 0.4990638 0.0869394 0.0106418 -0.0000318 -0.0000317 15.001621 2 0.0000296 -0.0001183 -0.0000040 -0.0000098 -0.0000097 -0.000002 3 -0.0000056 -0.0000009 Tan Ä1 = 0.0046308 Tan Ä2 = 0.0046077 At time 't1' (decimal hours), each besselian element is evaluated by: x = x0 + x1*t + x2*t2 + x3*t3 (or x = · [xn*tn]; n = 0 to 3) where: t = t1 - t0 (decimal hours) and t0 = 17.000 Note that all times are expressed in Terrestrial Dynamical Time (TDT). Saros Series 128: Member 57 of 73 eclipses in series.