Besselian Elements for Hybrid Solar Eclipse of 1930 Apr 28 (original) (raw)

Fred Espenak

The following table contains the Besselian elements for the Hybrid Solar Eclipse of 1930 Apr 28 .

The geographic coordinates of the eclipse path are in the Path Table . The global visibility of the eclipse is shown on an Orthographic Map . The features of this map are described in the Key to Solar Eclipse Path Tables. The path of the eclipse is displayed in greater detail on a Google Map .

Besselian Elements for the Hybrid Solar Eclipse of 1930 Apr 28

        Equatorial Conjunction:     19:27:27.5 TDT     J.D. = 2426095.310735
          (Sun & Moon in R.A.)    (=19:27:03.4 UT)

         Ecliptic Conjunction:      19:08:43.9 TDT     J.D. = 2426095.297731
         (Sun & Moon in Ec. Lo.)  (=19:08:19.8 UT)

              Instant of            19:03:34.1 TDT     J.D. = 2426095.294144
           Greatest Eclipse:      (=19:03:10.0 UT)


        --------------------------------------------------------------------------- 
                    Gamma =  0.4730            Ephemerides = VSOP87/ELP2000-82
        Eclipse Magnitude =  1.0003           Lunation No. =    -862
                       ΔT =    24.1 s         Saros Series =  137 (31/70)

        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/ELP2000-82):

        Sun:       R.A. = 02h21m32.6s         Moon:      R.A. = 02h20m46.0s
                   Dec. =+14°06'03.1"                    Dec. =+14°30'42.8"
          Semi-Diameter =    15'52.8"           Semi-Diameter =    15'39.8"
            Eq.Hor.Par. =       08.7"             Eq.Hor.Par. =  0°57'29.0"

        --------------------------------------------------------------------------- 
        Polynomial Besselian Elements for:   1930 Apr 28   19:00:00.0 TDT  (=t0)

          n        x          y         d          l1         l2          μ

          0  -0.226122   0.416757   14.09906   0.550157   0.004000  105.63587
          1   0.4940888  0.2259773   0.012593 -0.0001219 -0.0001213  15.002804
          2   0.0000645 -0.0000944  -0.000003 -0.0000112 -0.0000111
          3  -0.0000067 -0.0000033

                         Tan ƒ1 = 0.0046428    Tan ƒ2 = 0.0046196

        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 = 19.000 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 16.00 ≤ t0 ≤ 22.00 TDT.

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

               Saros Series 137:  Member 31 of 70 eclipses in series.

Hybrid Solar Eclipse of 1930 Apr 28

Acknowledgments

Predictions for the Hybrid Solar Eclipse of 1930 Apr 28 were generated using the VSOP87/ELP2000-82 solar and lunar ephemerides and a value of ΔT = 24.1 seconds. The accuracy of the northern and southern edges of the eclipse path are limited to approximately 1-2 kilometers due to the lunar limb profile.

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