The following table contains the Besselian elements for the Partial Solar Eclipse of 2040 Nov 04 .
The global visibility of the eclipse is shown on an Orthographic Map .
Besselian Elements for the Partial Solar Eclipse of 2040 Nov 04
Non-Central Eclipse
Equatorial Conjunction: 18:17:25.7 TDT J.D. = 2466463.262103
(Sun & Moon in R.A.) (=18:16:01.2 UT)
Ecliptic Conjunction: 18:57:11.8 TDT J.D. = 2466463.289719
(Sun & Moon in Ec. Lo.) (=18:55:47.3 UT)
Instant of 19:09:01.5 TDT J.D. = 2466463.297934
Greatest Eclipse: (=19:07:37.0 UT)
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Gamma = 1.0993 Ephemerides = VSOP87/ELP2000-85
Eclipse Magnitude = 0.8074 Lunation No. = 505
ΔT = 84.4 s Saros Series = 124 (56/73)
Lunar Radius k1 = 0.272488 (Penumbra) Shift in Δb = 0.00"
Constants: k2 = 0.272281 (Umbra) Lunar Position: Δl = 0.00"
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Geocentric Coordinates of Sun & Moon at Greatest Eclipse (VSOP87/ELP2000-85):
Sun: R.A. = 14h42m06.9s Moon: R.A. = 14h43m50.8s
Dec. =-15°43'53.9" Dec. =-14°45'19.7"
Semi-Diameter = 16'07.8" Semi-Diameter = 15'49.8"
Eq.Hor.Par. = 08.9" Eq.Hor.Par. = 0°58'05.6"
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Polynomial Besselian Elements for: 2040 Nov 04 19:00:00.0 TDT (=t0)
n x y d l1 l2 μ
0 0.357528 1.042811 -15.73231 0.551516 0.005352 109.10986
1 0.5039256 -0.2161531 -0.012099 -0.0001136 -0.0001130 15.000983
2 0.0000395 0.0000395 0.000004 -0.0000116 -0.0000115
3 -0.0000066 0.0000031
Tan ƒ1 = 0.0047155 Tan ƒ2 = 0.0046920
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 124: Member 56 of 73 eclipses in series.
Predictions for the Partial Solar Eclipse of 2040 Nov 04 were generated using the VSOP87/ELP2000-85 solar and lunar ephemerides and a value of ΔT = 84.4 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.
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
