Penumbral Lunar Eclipse of 1944 Aug 04
The Penumbral Lunar Eclipse of 1944 Aug 04 is visible from the following geographic regions:
- eastern Asia, Australia, western 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 1944 Aug 04 at 12:26:52 TD (12:26:25 UT1). This is 1.4 days before the Moon reaches perigee. During the eclipse, the Moon is in the constellation Capricornus. The synodic month in which the eclipse takes place has a Brown Lunation Number of 267.
The eclipse belongs to Saros 147 and is number 4 of 70 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.
The penumbral lunar eclipse of 1944 Aug 04 is preceded two weeks earlier by a annular solar eclipse on 1944 Jul 20.
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 26.7 seconds for this eclipse.
The following links provide maps and data for the eclipse.
- Eclipse Figure - eclipse geometry diagram and map of eclipse visibility
- Saros 147 Table - data for all eclipses in the Saros series
The tables below contain detailed predictions and additional information on the Penumbral Lunar Eclipse of 1944 Aug 04 .