Besselian Elements for the Annular Solar Eclipse of 2003 May 31

Fred Espenak

The following table contains the Besselian elements for the Annular Solar Eclipse of 2003 May 31 .

The geographic coordinates of the eclipse path are listed in the Path Table . The global visibility of the eclipse is shown on an Orthographic Map . The path of the eclipse is displayed in greater detail on an Google Map .


            

Besselian Elements for the Annular Solar Eclipse of 2003 May 31

Central Eclipse With One Limit

Equatorial Conjunction: 04:39:20.6 TDT J.D. = 2452790.693988 (Sun & Moon in R.A.) (=04:38:16.1 UT) Ecliptic Conjunction: 04:20:57.1 TDT J.D. = 2452790.681217 (Sun & Moon in Ec. Lo.) (=04:19:52.7 UT) Instant of 04:09:22.5 TDT J.D. = 2452790.673177 Greatest Eclipse: (=04:08:18.0 UT) --------------------------------------------------------------------------- Gamma = 0.9960 Ephemerides = VSOP87/ELP2000-85 Eclipse Magnitude = 0.9384 Lunation No. = 42 ΔT = 64.5 s Saros Series = 147 (22/80) Lunar Radius k1 = 0.272488 (Penumbra) Shift in Δb = 0.00" Constants: k2 = 0.272281 (Umbra) Lunar Position: Δl = 0.00" --------------------------------------------------------------------------- Geocentric Coordinates of Sun & Moon at Greatest Eclipse (VSOP87/ELP2000-85): Sun: R.A. = 04h30m33.5s Moon: R.A. = 04h29m35.5s Dec. =+21°50'57.2" Dec. =+22°43'13.2" Semi-Diameter = 15'46.5" Semi-Diameter = 14'48.1" Eq.Hor.Par. = 08.7" Eq.Hor.Par. = 0°54'19.3" --------------------------------------------------------------------------- Polynomial Besselian Elements for: 2003 May 31 04:00:00.0 TDT (=t0) n x y d l1 l2 μ 0 -0.323877 0.945216 21.84598 0.564384 0.018156 240.61102 1 0.4938982 0.1263284 0.005746 -0.0000530 -0.0000527 14.999792 2 0.0000546 -0.0001692 -0.000004 -0.0000098 -0.0000098 3 -0.0000054 -0.0000015 Tan ƒ1 = 0.0046126 Tan ƒ2 = 0.0045896 At time t1 (decimal hours), each Besselian element is evaluated by: a = a0 + a1*t + a2*t^2 + a3*t^3 (or a = Σ [an*t^n]; n = 0 to 3) where: a = x, y, d, l1, l2, or μ t = t1 - t0 (decimal hours) and t0 = 4.000 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. The Besselian elements are valid over the period 1.00 ≤ t0 ≤ 7.00 TDT. Note that all times are expressed in Terrestrial Dynamical Time (TDT). Saros Series 147: Member 22 of 80 eclipses in series.

Greatest Eclipse and Greatest Duration


   Instant of 
Greatest Eclipse:       Time =  04:08:18.0 UT       Lat = 66°32.7'N      Long = 024°30.7'W
      (GE)               Sun Altitude =   2.9°          Path Width =4663.1 km
                          Sun Azimuth =  35.1°    Central Duration =   03m36.8s


   Instant of 
Greatest Duration:      Time =    04:07:54 UT       Lat =   66°26'N      Long =   024°01'W
      (GD)               Sun Altitude =   2.9°          Path Width =4684.2 km
                          Sun Azimuth =  35.4°    Central Duration =   03m36.8s


Links for the Annular Solar Eclipse of 2003 May 31


Eclipse Predictions

Predictions for the Annular Solar Eclipse of 2003 May 31 were generated using the VSOP87/ELP2000-85 solar and lunar ephemerides and a value of ΔT = 64.5 seconds. The luanr coordinates have been calculated with respect to the Moon's Center of Mass. They DO NOT include a correction to the Center of Figure, or the effects of mountains and valleys along the edge of the Moon.

Acknowledgments

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 by Fred Espenak, NASA's GSFC"

For more information, see: NASA Copyright Information


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