May 1957 lunar eclipse

{{Short description|Total lunar eclipse May 13, 1957}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-1957May13.png

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

| date = May 13, 1957

| gamma = 0.3046

| magnitude = 1.2982

| saros_ser = 130

| saros_no = 31 of 72

| totality = 77 minutes, 39 seconds

| partiality = 211 minutes, 36 seconds

| penumbral = 334 minutes, 57 seconds

| p1 = 19:43:30

| u1 = 20:45:06

| u2 = 21:52:05

| greatest = 22:30:56

| u3 = 23:09:44

| u4 = 0:16:42

| p4 = 1:18:27

| previous = November 1956

| next = November 1957

}}

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, May 13, 1957,{{cite web|title=May 13–14, 1957 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/1957-may-13|publisher=timeanddate|access-date=25 December 2024}} with an umbral magnitude of 1.2982. 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 3.25 days after perigee (on May 9, 1957, at 4:30 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=1957&n=136|publisher=timeanddate|access-date=25 December 2024}}

This lunar eclipse was the third of an almost tetrad, with the others being on May 24, 1956 (partial); November 18, 1956 (total); and November 7, 1957 (total).

Visibility

The eclipse was completely visible over Europe, Africa, the Middle East, and Antarctica, seen rising over eastern North America and South America and setting over much of Asia and Australia.{{cite web|title=Total Lunar Eclipse of 1957 May 13|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1957May13T.pdf|publisher=NASA|access-date=25 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 1957 May 13|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1957May13Tprime.html|publisher=EclipseWise.com|access-date=25 December 2024}}

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|+May 13, 1957 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.30005

Umbral Magnitude

| 1.29822

Gamma

| 0.30457

Sun Right Ascension

| 03h21m53.2s

Sun Declination

| +18°29'35.8"

Sun Semi-Diameter

| 15'49.4"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 15h22m04.8s

Moon Declination

| -18°12'09.6"

Moon Semi-Diameter

| 15'47.7"

Moon Equatorial Horizontal Parallax

| 0°57'58.1"

ΔT

| 32.0 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 1957

! April 30
Descending node (new moon)
!! May 13
Ascending node (full moon)

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| Annular solar eclipse
Solar Saros 118

Total lunar eclipse
Lunar Saros 130

Related eclipses

= Eclipses in 1957 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 130 =

= Inex =

= Triad =

= Lunar eclipses of 1955–1958 =

{{Lunar eclipse set 1955–1958}}

= Saros 130 =

{{Lunar Saros series 130}}

= Tritos series =

{{Lunar Tritos series January 2001}}

= Inex series =

{{Lunar Inex series April 2015}}

= 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 annular solar eclipses of Solar Saros 137.

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!May 9, 1948

!May 20, 1966

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See also

Notes

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