October 1985 lunar eclipse

{{Short description|Total lunar eclipse (October 28, 1985)}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-1985Oct28.png

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

| date = October 28, 1985

| gamma = −0.4022

| magnitude = 1.0736

| saros_ser = 126

| saros_no = 44 of 72

| totality = 43 minutes, 52 seconds

| partiality = 214 minutes, 57 seconds

| penumbral = 365 minutes, 3 seconds

| p1 = 14:39:51

| u1 = 15:54:53

| u2 = 17:20:26

| greatest = 17:42:22

| u3 = 18:04:18

| u4 = 19:29:50

| p4 = 20:44:54

| previous = May 1985

| next = April 1986

}}

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, October 28, 1985,{{cite web|title=October 28–29, 1985 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/1985-october-28|publisher=timeanddate|access-date=6 January 2025}} with an umbral magnitude of 1.0736. 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 1.2 days before apogee (on October 29, 1985, at 21:50 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=1985&n=136|publisher=timeanddate|access-date=6 January 2025}}

This lunar eclipse was the second of a tetrad, with four total lunar eclipses in series, the others being on May 4, 1985; April 24, 1986; and October 17, 1986.

Visibility

The eclipse was completely visible over northern Europe, Asia, and western Australia, seen rising over Africa and much of Europe and setting over eastern Australia, northwestern North America, and the central Pacific Ocean.{{cite web|title=Total Lunar Eclipse of 1985 Oct 28|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1985Oct28T.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 1985 Oct 28|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1985Oct28Tprime.html|publisher=EclipseWise.com|access-date=6 January 2025}}

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|+October 28, 1985 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.16733

Umbral Magnitude

| 1.07357

Gamma

| −0.40218

Sun Right Ascension

| 14h11m49.8s

Sun Declination

| -13°16'24.9"

Sun Semi-Diameter

| 16'06.1"

Sun Equatorial Horizontal Parallax

| 08.9"

Moon Right Ascension

| 02h12m27.9s

Moon Declination

| +12°56'45.9"

Moon Semi-Diameter

| 14'43.3"

Moon Equatorial Horizontal Parallax

| 0°54'01.6"

ΔT

| 54.8 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 October–November 1985

! October 28
Ascending node (full moon)
!! November 12
Descending node (new moon)

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| Total lunar eclipse
Lunar Saros 126

Total solar eclipse
Solar Saros 152

Related eclipses

= Eclipses in 1985 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 126 =

= Inex =

= Triad =

= Lunar eclipses of 1984–1987 =

{{Lunar eclipse set 1984-1987}}

= Metonic series =

{{Metonic lunar eclipse 1966-2023}}

= Saros 126 =

{{Lunar Saros series 126}}

= Tritos series =

{{Lunar Tritos series August 2007}}

= Inex series =

{{Lunar Inex series October 2014}}

= 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 133.

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!October 23, 1976

!November 3, 1994

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See also

Notes

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