Penumbral Lunar Eclipse of 1969 Sep 25

Fred Espenak

Key to Lunar Eclipse Figure (below)

Introduction


The Penumbral Lunar Eclipse of 1969 Sep 25 is visible from the following geographic regions:

  • Europe, Africa, Asia, Austrlia

The diagram to the right depicts the Moon's path with respect to Earth's umbral and penumbral shadows. Below it is a map showing the geographic regions of eclipse visibility. Click on the figure to enlarge it. For an explanation of the features appearing in the figure, see Key to Lunar Eclipse Figures.

The instant of greatest eclipse takes place on 1969 Sep 25 at 20:10:18 TD (20:09:38 UT1). This is 3.4 days after the Moon reaches perigee. During the eclipse, the Moon is in the constellation Pisces. The synodic month in which the eclipse takes place has a Brown Lunation Number of 578.

The eclipse belongs to Saros 146 and is number 8 of 72 eclipses in the series. All eclipses in this series occur at the Moon’s ascending node. The Moon moves southward with respect to the node with each succeeding eclipse in the series and gamma decreases.

This is a very deep penumbral eclipse. It has a penumbral eclipse magnitude of 0.9008 and a penumbral eclipse duration of 245.2 minutes. Gamma has a value of 1.0656.

The penumbral lunar eclipse of 1969 Sep 25 is preceded two weeks earlier by a annular solar eclipse on 1969 Sep 11.

Another lunar eclipse occurs one synodic month before the 1969 Sep 25 eclipse. It is the penumbral lunar eclipse of 1969 Aug 27.

These eclipses all take place during a single eclipse season.

The eclipse predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., TD = UT1 + ΔT). ΔT has a value of 39.9 seconds for this eclipse.

The following links provide maps and data for the eclipse.

The tables below contain detailed predictions and additional information on the Penumbral Lunar Eclipse of 1969 Sep 25 .


Eclipse Data: Penumbral Lunar Eclipse of 1969 Sep 25

Eclipse Characteristics
Parameter Value
Penumbral Magnitude 0.90080
Umbral Magnitude-0.09519
Gamma 1.06558
Epsilon 1.0439°
Opposition Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 1969 Sep 25 at 20:10:18.2 TD (20:09:38.3 UT1) 2440490.340027
Ecliptic Opposition 1969 Sep 25 at 20:21:30.2 TD (20:20:50.3 UT1) 2440490.347804
Equatorial Opposition 1969 Sep 25 at 21:14:05.5 TD (21:13:25.5 UT1) 2440490.384323
Geocentric Coordinates of Sun and Moon
1969 Sep 25 at 20:10:18.2 TD (20:09:38.3 UT1)
Coordinate Sun Moon
Right Ascension12h09m26.5s00h07m25.1s
Declination-01°01'23.8"+01°56'11.3"
Semi-Diameter 15'57.2" 16'01.1"
Eq. Hor. Parallax 08.8" 0°58'47.2"
Geocentric Libration of Moon
Angle Value
l 4.7°
b -1.4°
c -21.9°
Earth's Shadows
Parameter Value
Penumbral Radius 1.2579°
Umbral Radius 0.7261°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE405
ΔT 39.9 s
Shadow Rule Danjon
Shadow Enlargement 1.010
Saros Series 146 ( 8/72)

Explanation of Lunar Eclipse Data Tables

Eclipse Contacts: Penumbral Lunar Eclipse of 1969 Sep 25

Lunar Eclipse Contacts
Eclipse Event Contact Time
TD
Time
UT1
Zenith Latitude Zenith Longitude Position Angle Axis Distance
Penumbral BeginsP118:07:38.418:06:58.501°21.8'N084°40.8'E 284.2° 1.5259°
Greatest EclipseGreatest20:10:18.220:09:38.301°56.2'N054°58.8'E 331.0° 1.0439°
Penumbral EndsP422:12:52.222:12:12.302°30.4'N025°18.2'E 17.8° 1.5238°
Eclipse Durations
Eclipse Phase Duration
Penumbral (P4 - P1)04h05m13.9s

Explanation of Lunar Eclipse Contacts Table

Polynomial Besselian Elements: Penumbral Lunar Eclipse of 1969 Sep 25

Polynomial Besselian Elements
1969 Sep 25 at 20:00:00.0 TD (=t0)
n x y d f1 f2 f3
0 -0.58750 0.86793 -0.0178 1.25797 0.72618 0.26698
1 0.47600 0.26365 -0.0003 -0.00041 -0.00042 -0.00011
2 -0.00018 -0.00017 0.0000 -0.00000 -0.00000 -0.00000
3 -0.00001 -0.00000 - - - -

At time t1 (decimal hours), each besselian element is evaluated by:

x = x0 + x1*t + x2*t2 + x3*t3 (or x = Σ [xn*tn]; n = 0 to 3)

where: t = t1 - t0 (decimal hours) and t0 = 20.000

Explanation of Besselian Elements

Eclipse Publications

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For more visit: AstroPixels Publishing


Links for the Penumbral Lunar Eclipse of 1969 Sep 25

Links to Additional Lunar Eclipse Information

Decade Tables of Lunar Eclipses:
| 1901 - 1910 | 1911 - 1919 | 1921 - 1930 | 1931 - 1940 | 1941 - 1950 |
| 1951 - 1960 | 1961 - 1970 | 1971 - 1980 | 1981 - 1990 | 1991 - 2000 |
| 2001 - 2010 | 2011 - 2020 | 2021 - 2030 | 2031 - 2040 | 2041 - 2050 |
| 2051 - 2060 | 2061 - 2070 | 2071 - 2080 | 2081 - 2090 | 2091 - 2100 |

Lunar Eclipse Publications

Eclipse Predictions

Predictions for the Penumbral Lunar Eclipse of 1969 Sep 25 were generated using the JPL DE405 solar and lunar ephemerides. The lunar coordinates were calculated with respect to the Moon's Center of Mass.

The Earth's umbral and penumbral shadows were calculated using the Danjon methodusing a mean mid-latitude ellipticity to compensate for the opacity of the terrestrial atmosphere.

The predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 39.9 seconds for this eclipse.

Acknowledgments

Some of the content on this web site is based on the book 21st Century Canon of Lunar Eclipses. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.

Permission is granted to reproduce eclipse data when accompanied by a link to this page and an acknowledgment:

"Eclipse Predictions by Fred Espenak, www.EclipseWise.com"

The use of diagrams and maps is permitted provided that they are NOT altered (except for re-sizing) and the embedded credit line is NOT removed or covered.