December 1982 lunar eclipse

{{Short description|Total lunar eclipse December 30, 1982}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-1982Dec30.png

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

| date = December 30, 1982

| gamma = 0.3758

| magnitude = 1.1822

| saros_ser = 134

| saros_no = 25 of 73

| totality = 60 minutes, 3 seconds

| partiality = 195 minutes, 53 seconds

| penumbral = 310 minutes, 34 seconds

| p1 = 8:53:27

| u1 = 9:50:48

| u2 = 10:58:43

| greatest = 11:28:44

| u3 = 11:58:46

| u4 = 13:06:41

| p4 = 14:04:01

| previous = July 1982

| next = June 1983

}}

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, December 30, 1982,{{cite web|title=December 29–30, 1982 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/1982-december-30|publisher=timeanddate|access-date=6 January 2025}} with an umbral magnitude of 1.1822. 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 only about 10.5 hours before perigee (on December 30, 1982, at 22:00 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=1982&n=136|publisher=timeanddate|access-date=6 January 2025}}

This was a supermoon since perigee was on the same day. It was also a blue moon, the second full moon of December for the eastern hemisphere where the previous full moon was on December 1.{{cite web | url=https://www.nationalgeographic.com/science/article/super-blue-blood-moon-explained-space-astronomy-science | title=Rare 'Super Blue Blood Moon' Coming—First in 35 Years | date=29 January 2018 | last1=Fazekas | first1=Andrew | archive-url=https://web.archive.org/web/20180129221332/https://news.nationalgeographic.com/2018/01/super-blue-blood-moon-explained-space-astronomy-science/ | archive-date=29 January 2018 | website=National Geographic}} Since total lunar eclipses are also known as blood moons, this combination (which would not recur until January 31, 2018) is known as a super blue blood moon.

Visibility

The eclipse was completely visible over north and northeast Asia, western and central North America, and the central Pacific Ocean, seen rising over northern Europe, much of Asia, and Australia and setting over eastern North America and western South America.{{cite web|title=Total Lunar Eclipse of 1982 Dec 30|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1982Dec30T.pdf|publisher=NASA|access-date=6 January 2025}}

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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 1982 Dec 30|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1982Dec30Tprime.html|publisher=EclipseWise.com|access-date=6 January 2025}}

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|+December 30, 1982 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.15450

Umbral Magnitude

| 1.18219

Gamma

| 0.37579

Sun Right Ascension

| 18h36m44.9s

Sun Declination

| -23°10'20.5"

Sun Semi-Diameter

| 16'15.9"

Sun Equatorial Horizontal Parallax

| 08.9"

Moon Right Ascension

| 06h36m41.3s

Moon Declination

| +23°33'23.8"

Moon Semi-Diameter

| 16'43.7"

Moon Equatorial Horizontal Parallax

| 1°01'23.7"

ΔT

| 53.0 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 December 1982

! December 15
Descending node (new moon)

December 30
Ascending node (full moon)
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| Partial solar eclipse
Solar Saros 122

Total lunar eclipse
Lunar Saros 134

Related eclipses

= Eclipses in 1982 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 134 =

= Inex =

= Triad =

= Lunar eclipses of 1980–1984 =

{{Lunar eclipse set 1980-1984}}

= Saros 134 =

{{Lunar Saros series 134}}

= Tritos series =

{{Lunar Tritos series October 2004}}

= Inex series =

{{Lunar Inex series December 2011}}

= 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 141.

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!December 24, 1973

!January 4, 1992

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See also

Notes

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