May 1937 lunar eclipse

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, May 25, 1937,[1] with an umbral magnitude of −0.3033. 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 only about 18 hours after apogee (on May 24, 1937, at 13:30 UTC), the Moon's apparent diameter was smaller.[2]

May 1937 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateMay 25, 1937
Gamma−1.1582
Magnitude−0.3033
Saros cycle110 (67 of 72)
Penumbral254 minutes, 43 seconds
Contacts (UTC)
P15:43:50
Greatest7:51:10
P49:58:33

Visibility

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The eclipse was completely visible over much of North America, western and central South America, and Antarctica, seen rising over Australia and setting over northeastern North America, eastern South America, and west Africa.[3]

   

Eclipse details

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Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

May 25, 1937 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.76969
Umbral Magnitude −0.30327
Gamma −1.15820
Sun Right Ascension 04h06m39.7s
Sun Declination +20°53'38.5"
Sun Semi-Diameter 15'47.3"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 16h06m15.0s
Moon Declination -21°55'55.1"
Moon Semi-Diameter 14'42.9"
Moon Equatorial Horizontal Parallax 0°54'00.1"
ΔT 23.9 s

Eclipse season

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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.

Eclipse season of May–June 1937
May 25
Ascending node (full moon)
June 8
Descending node (new moon)
   
Penumbral lunar eclipse
Lunar Saros 110
Total solar eclipse
Solar Saros 136
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Eclipses in 1937

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 110

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Inex

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Triad

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Lunar eclipses of 1937–1940

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Lunar eclipse series sets from 1937–1940
Ascending node   Descending node
Saros Date
viewing
Type
chart
Saros Date
viewing
Type
chart
110 1937 May 25
 
Penumbral
 
115 1937 Nov 18
 
Partial
 
120 1938 May 14
 
Total
 
125 1938 Nov 07
 
Total
 
130 1939 May 03
 
Total
 
135 1939 Oct 28
 
Partial
 
140 1940 Apr 22
 
Penumbral
 
145 1940 Oct 16
 
Penumbral
 

Half-Saros cycle

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A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to one total and one partial = two solar eclipses of Solar Saros 117.

May 19, 1928 May 30, 1946
   

See also

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Notes

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  1. ^ "May 24–25, 1937 Penumbral Lunar Eclipse". timeanddate. Retrieved 18 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 18 December 2024.
  3. ^ "Penumbral Lunar Eclipse of 1937 May 25" (PDF). NASA. Retrieved 18 December 2024.
  4. ^ "Penumbral Lunar Eclipse of 1937 May 25". EclipseWise.com. Retrieved 18 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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  NODES
Note 3