Total Lunar Eclipse of 1979 Sep 06
Fred Espenak
Key to Lunar Eclipse Figure (below)
Introduction
The Total Lunar Eclipse of 1979 Sep 06 is visible from the following geographic regions:
- Asia, Australia, Pacific, Americas
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 1979 Sep 06 at 10:55:02 TD (10:54:12 UT1). This is 0.2 days after the Moon reaches perigee. During the eclipse, the Moon is in the constellation Aquarius. The synodic month in which the eclipse takes place has a Brown Lunation Number of 701.
The eclipse belongs to Saros 137 and is number 24 of 78 eclipses in the series. All eclipses in this series occur at the Moons descending node. The Moon moves northward with respect to the node with each succeeding eclipse in the series and gamma increases.
This is a very shallow total eclipse. It has an umbral eclipse magnitude of only 1.0936 and a duration of totality lasting 44.4 minutes. Gamma has a value of -0.4305.
The total lunar eclipse of 1979 Sep 06 is preceded two weeks earlier by a annular solar eclipse on 1979 Aug 22.
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 50.2 seconds for this eclipse.
The following links provide maps and data for the eclipse.
- Detailed Lunar Eclipse Figure - eclipse geometry diagram and map of eclipse visibility (Key to Figure)
- Saros 137 Table - data for all eclipses in the Saros series
The tables below contain detailed predictions and additional information on the Total Lunar Eclipse of 1979 Sep 06 .