A penumbral lunar eclipse occurred at the Moon's descending node of orbit on Friday, August 4, 1944, with an umbral magnitude of −0.4758. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 1.5 days before perigee (on August 5, 1944, at 23:45 UTC), the Moon's apparent diameter was larger.
This eclipse was the third of four penumbral lunar eclipses in 1944, with the others occurring on February 9, July 6, and December 29.
Visibility The eclipse was completely visible over Australia and Antarctica, seen rising over east and south Asia and setting over western North and South America.
Eclipse details Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.
+August 4, 1944 Lunar Eclipse Parameters Parameter Value Penumbral Magnitude 0.47847 Umbral Magnitude −0.47577 Gamma −1.28428 Sun Right Ascension 08h57m44.4s Sun Declination +17°12'21.5" Sun Semi-Diameter 15'46.0" Sun Equatorial Horizontal Parallax 08.7" Moon Right Ascension 20h58m45.5s Moon Declination -18°28'52.1" Moon Semi-Diameter 16'31.4" Moon Equatorial Horizontal Parallax 1°00'38.5" ΔT 26.7 s
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.
+ Eclipse season of July–August 1944 July 6Descending node (full moon) July 20Ascending node (new moon) August 4Descending node (full moon) Penumbral lunar eclipseLunar Saros 109 Annular solar eclipseSolar Saros 135 Penumbral lunar eclipseLunar Saros 147
Related lunar eclipses Eclipses in 1944 A total solar eclipse on January 25. A penumbral lunar eclipse on February 9. A penumbral lunar eclipse on July 6. An annular solar eclipse on July 20. A penumbral lunar eclipse on August 4. A penumbral lunar eclipse on December 29.
Metonic Preceded by: Lunar eclipse of October 16, 1940
Tzolkinex Followed by: Lunar eclipse of September 15, 1951
Half-Saros Preceded by: Solar eclipse of July 30, 1935 Followed by: Solar eclipse of August 9, 1953
Tritos Preceded by: Lunar eclipse of September 4, 1933
Lunar Saros 147 Preceded by: Lunar eclipse of July 25, 1926 Followed by: Lunar eclipse of August 15, 1962
Inex Preceded by: Lunar eclipse of August 24, 1915 Followed by: Lunar eclipse of July 15, 1973
Triad Preceded by: Lunar eclipse of October 3, 1857 Followed by: Lunar eclipse of June 5, 2031
Lunar eclipses of 1940–1944
Saros 147
Tritos series
Series members between 1801 and 2042 1802 Sep 11(Saros 134) 1813 Aug 12(Saros 135) 1824 Jul 11(Saros 136) 1835 Jun 10(Saros 137) 1846 May 11(Saros 138) 1857 Apr 09(Saros 139) 1868 Mar 08(Saros 140) 1879 Feb 07(Saros 141) 1890 Jan 06(Saros 142) 1900 Dec 06(Saros 143) 1911 Nov 06(Saros 144) 1922 Oct 06(Saros 145) 1933 Sep 04(Saros 146) 1944 Aug 04(Saros 147) 2042 Oct 28(Saros 156)
Inex series
Half-Saros cycle A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two total solar eclipses of Solar Saros 154. July 30, 1935August 9, 1953
See also List of lunar eclipses and List of 21st-century lunar eclipses
References
External links Saros series 147