May 1939 lunar eclipse
{{Short description|Total lunar eclipse May 3, 1939}}
{{Infobox lunar eclipse
| type = total
| image = Lunar eclipse chart close-1939May03.png
| caption = The Moon's hourly motion shown right to left
| date = May 3, 1939
| gamma = 0.3693
| magnitude = 1.1765
| saros_ser = 130
| saros_no = 30 of 72
| totality = 62 minutes, 23 seconds
| partiality = 207 minutes, 3 seconds
| penumbral = 333 minutes, 31 seconds
| p1 = 12:24:35
| u1 = 13:27:45
| u2 = 14:40:06
| greatest = 15:11:18
| u3 = 15:42:28
| u4 = 16:54:48
| p4 = 17:58:06
| previous = November 1938
| next = October 1939
}}
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, May 3, 1939,{{cite web|title=May 3–4, 1939 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/1939-may-3|publisher=timeanddate|access-date=18 December 2024}} with an umbral magnitude of 1.1765. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 5.2 days after perigee (on April 28, 1939, at 11:05 UTC), the Moon's apparent diameter was larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1939&n=136|publisher=timeanddate|access-date=18 December 2024}}
This lunar eclipse was the third of an almost tetrad, with the others being on May 14, 1938 (total); November 7, 1938 (total); and October 28, 1939 (partial).
Visibility
The eclipse was completely visible over east Asia, Australia, and Antarctica, seen rising over central and east Africa, eastern Europe, and west, central, and south Asia and setting over western North America and the eastern Pacific Ocean.{{cite web|title=Total Lunar Eclipse of 1939 May 03|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1901/LE1939May03T.pdf|publisher=NASA|access-date=18 December 2024}}
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Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Total Lunar Eclipse of 1939 May 03|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1939May03Tprime.html|publisher=EclipseWise.com|access-date=18 December 2024}}
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|+May 3, 1939 Lunar Eclipse Parameters ! Parameter ! Value |
Penumbral Magnitude
| 2.18417 |
Umbral Magnitude
| 1.17649 |
Gamma
| 0.36934 |
Sun Right Ascension
| 02h39m22.9s |
Sun Declination
| +15°31'43.2" |
Sun Semi-Diameter
| 15'51.8" |
Sun Equatorial Horizontal Parallax
| 08.7" |
Moon Right Ascension
| 14h39m41.4s |
Moon Declination
| -15°10'51.4" |
Moon Semi-Diameter
| 15'44.6" |
Moon Equatorial Horizontal Parallax
| 0°57'46.6" |
ΔT
| 24.2 s |
{{clear}}
Eclipse season
{{See also|Eclipse cycle}}
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.
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|+ Eclipse season of April–May 1939 ! April 19 | |
200px | 200px |
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| Annular solar eclipse | Total lunar eclipse Lunar Saros 130 |
Related eclipses
= Eclipses in 1939 =
- An annular solar eclipse on April 19.
- A total lunar eclipse on May 3.
- A total solar eclipse on October 12.
- A partial lunar eclipse on October 28.
= Metonic =
- Preceded by: Lunar eclipse of July 16, 1935
- Followed by: Lunar eclipse of February 20, 1943
= Tzolkinex =
- Preceded by: Lunar eclipse of March 22, 1932
- Followed by: Lunar eclipse of June 14, 1946
= Half-Saros =
- Preceded by: Solar eclipse of April 28, 1930
- Followed by: Solar eclipse of May 9, 1948
= Tritos =
- Preceded by: Lunar eclipse of June 3, 1928
- Followed by: Lunar eclipse of April 2, 1950
= Lunar Saros 130 =
- Preceded by: Lunar eclipse of April 22, 1921
- Followed by: Lunar eclipse of May 13, 1957
= Inex =
- Preceded by: Lunar eclipse of May 24, 1910
- Followed by: Lunar eclipse of April 13, 1968
= Triad =
- Preceded by: Lunar eclipse of July 1, 1852
- Followed by: Lunar eclipse of March 3, 2026
= Lunar eclipses of 1937–1940 =
{{Lunar eclipse set 1937-1940}}
= Saros 130 =
{{Lunar Saros series 130}}
= Tritos series =
{{Lunar Tritos series October 2004}}
= Inex series =
{{Lunar Inex series March 2026}}
= 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 solar eclipses of Solar Saros 137.
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See also
Notes
{{reflist}}
External links
- {{LEplot1901 link|1939|May|03|T}}
{{Lunar eclipses}}
{{DEFAULTSORT:Lunar eclipse 1939-05}}
{{lunar-eclipse-stub}}