September 1932 lunar eclipse

{{Short description|Partial lunar eclipse September 14, 1932}}

{{Infobox lunar eclipse

| type = partial

| image = Lunar eclipse chart close-1932Sep14.png

| caption = The Moon's hourly motion shown right to left

| date = September 14, 1932

| gamma = 0.4664

| magnitude = 0.9752

| saros_ser = 136

| saros_no = 15 of 72

| partiality = 203 minutes, 58 seconds

| penumbral = 347 minutes, 12 seconds

| p1 = 18:07:03

| u1 = 19:18:35

| greatest = 21:00:36

| u4 = 22:42:33

| p4 = 23:54:15

| previous = March 1932

| next = February 1933

}}

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, September 14, 1932,{{cite web|title=September 14–15, 1932 Partial Lunar Eclipse|url=https://www.timeanddate.com/eclipse/lunar/1932-september-14|publisher=timeanddate|access-date=16 December 2024}} with an umbral magnitude of 0.9752. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 4.8 days before apogee (on September 19, 1932, at 17:00 UTC), the Moon's apparent diameter was smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1932&n=136|publisher=timeanddate|access-date=16 December 2024}}

This was the last of the first set of partial lunar eclipses in Lunar Saros 136, preceding the first total eclipse on September 26, 1950.

Visibility

The eclipse was completely visible over much of Africa, Europe, and west, central, and south Asia, seen rising over west Africa, South America, and eastern North America and setting over east and northeast Asia and Australia.{{cite web|title=Partial Lunar Eclipse of 1932 Sep 14|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1901/LE1932Sep14P.pdf|publisher=NASA|access-date=16 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=Partial Lunar Eclipse of 1932 Sep 14|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1932Sep14Pprime.html|publisher=EclipseWise.com|access-date=16 December 2024}}

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|+September 14, 1932 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.02964

Umbral Magnitude

| 0.97519

Gamma

| 0.46642

Sun Right Ascension

| 11h29m54.4s

Sun Declination

| +03°15'02.3"

Sun Semi-Diameter

| 15'54.5"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 23h29m04.4s

Moon Declination

| -02°52'26.5"

Moon Semi-Diameter

| 15'05.2"

Moon Equatorial Horizontal Parallax

| 0°55'22.0"

ΔT

| 23.9 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 August–September 1932

! August 31
Descending node (new moon)

September 14
Ascending node (full moon)
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| Total solar eclipse
Solar Saros 124

Partial lunar eclipse
Lunar Saros 136

Related eclipses

= Eclipses in 1932 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 136 =

= Inex =

= Triad =

= Lunar eclipses of 1930–1933 =

{{Lunar eclipse set 1930-1933}}

= Saros 136 =

{{Lunar Saros series 136}}

= Tritos series =

{{Lunar Tritos series February 2009}}

= Inex series =

{{Lunar Inex series July 2019}}

= 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 143.

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!September 10, 1923

!September 21, 1941

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See also

References

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