June 2094 lunar eclipse

{{Short description|Central lunar eclipse}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-2094Jun28.png

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

| date = June 28, 2094

| gamma = 0.0288

| magnitude = 1.8249

| saros_ser = 131

| saros_no = 38 of 72

| totality = 100 minutes, 36 seconds

| partiality = 235 minutes, 42 seconds

| penumbral = 326 minutes, 27 seconds

| p1 = 7:15:31

| u1 = 8:10:57

| u2 = 9:08:29

| greatest = 9:58:47

| u3 = 10:49:06

| u4 = 11:46:39

| p4 = 12:41:59

| previous = January 2094

| next = December 2094

}}

A total lunar eclipse will occur at the Moon’s descending node of orbit on Monday, June 28, 2094,{{cite web|title=June 27–28, 2094 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2094-june-28|publisher=timeanddate|access-date=14 December 2024}} with an umbral magnitude of 1.8249. It will be a central lunar eclipse, in which part of the Moon will pass through the center of the Earth's shadow. 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 1.9 days before perigee (on June 30, 2094, at 7:50 UTC), the Moon's apparent diameter will be larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2094&n=136|publisher=timeanddate|access-date=14 December 2024}}

While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red color at maximum eclipse. With a gamma value of only 0.0288 and an umbral eclipse magnitude of 1.8249, this is the greatest eclipse in Lunar Saros 131 as well as the second largest and darkest lunar eclipse of the 21st century.

During the eclipse, NGC 6629 will be occulted by the Moon over Northeast Australia and the Pacific Ocean; NGC 6642 will be occulted by the Moon over New Guinea, Northern Australia and the Pacific Ocean. Deep-sky objects are rarely occulted during a total eclipse from any given spot on Earth.{{cite book |date=2002 |first=Jan |last=Meeus |chapter=Occultations of deep-sky objects during a total lunar eclipse |pages=157-162 |title=More Mathematical Astronomy Morsels |isbn=0943396743 |url=https://falakmu.id/khgt/dokumen/More%20mathematical%20astronomy%20morsels%20(Jean%20Meeus)%20(Z-Library).pdf}}{{rp|161}}

Visibility

The eclipse will be completely visible over eastern Australia, Antarctica, and the central and eastern Pacific Ocean, seen rising over east Asia and western Australia and setting over North and South America.{{cite web|title=Total Lunar Eclipse of 2094 Jun 28|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2051/LE2094Jun28T.pdf|publisher=NASA|access-date=14 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 2094 Jun 28|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2094Jun28Tprime.html|publisher=EclipseWise.com|access-date=14 December 2024}}

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|+June 28, 2094 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.78793

Umbral Magnitude

| 1.82485

Gamma

| 0.02882

Sun Right Ascension

| 06h31m43.3s

Sun Declination

| +23°13'34.7"

Sun Semi-Diameter

| 15'44.1"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 18h31m43.6s

Moon Declination

| -23°11'51.1"

Moon Semi-Diameter

| 16'20.2"

Moon Equatorial Horizontal Parallax

| 0°59'57.5"

ΔT

| 121.4 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. The first and last eclipse in this sequence is separated by one synodic month.

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|+ Eclipse season of June–July 2094

! June 13
Ascending node (new moon)
!! June 28
Descending node (full moon)
!! July 12
Ascending node (new moon)

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align=center

| Partial solar eclipse
Solar Saros 119

Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Related eclipses

= Eclipses in 2094 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 131 =

= Inex =

= Triad =

= Lunar eclipses of 2092–2096 =

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.{{cite web |last1=van Gent |first1=R.H |title=Solar- and Lunar-Eclipse Predictions from Antiquity to the Present |url=http://www.staff.science.uu.nl/~gent0113/eclipse/eclipsecycles.htm#Sar%20%28Half%20Saros%29 |website=A Catalogue of Eclipse Cycles |publisher=Utrecht University |access-date=6 October 2018}}

The penumbral lunar eclipses on February 23, 2092 and August 17, 2092 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on May 7, 2096 and October 31, 2096 occur in the next lunar year eclipse set.

class="wikitable mw-collapsible mw-collapsed"

!class="nowrap" colspan="9" | Lunar eclipse series sets from 2092 to 2096

scope="col" colspan="4" | Descending node

| rowspan="11" | 

! scope="col" colspan="4" | Ascending node

style="text-align: center;"

! scope="col" | Saros

! scope="col" | Date
Viewing

! scope="col" | Type
Chart

! scope="col" | Gamma

! scope="col" | Saros

! scope="col" | Date
Viewing

! scope="col" | Type
Chart

! scope="col" | Gamma

style="text-align: center;"

| 111

| 2092 Jul 19

| style="text-align:center;" |Penumbral

| 1.5131

| 116

| 2093 Jan 12

| style="text-align:center;" |Penumbral

| −1.1733

style="text-align: center;"

| 121

| 2093 Jul 08

| style="text-align:center;" |Partial

| 0.7632

| 126

| 2094 Jan 01

| style="text-align:center;" |Partial

| −0.5024

style="text-align: center;"

| 131

| 2094 Jun 28
80px

| style="text-align:center;" |Total
80px

| 0.0288

| 136

| style="text-align:center;vertical-align:top;" |2094 Dec 21

| style="text-align:center;" |Total

| 0.2016

style="text-align: center;"

| 141

| 2095 Jun 17

| style="text-align:center;" |Partial

| −0.7653

| 146

| 2095 Dec 11

| style="text-align:center;" |Partial

| 0.8742

style="text-align: center;"

| 151

| 2096 Jun 06

| style="text-align:center;" |Penumbral

| −1.5723

| 156

| 2096 Nov 29

| style="text-align:center;" |Penumbral

| 1.5017

= Saros 131 =

{{Lunar Saros series 131}}

= Tritos series =

{{Lunar Tritos series March 2007}}

= Inex series =

{{Lunar Inex series August 2007}}

= 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 138.

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!June 22, 2085

!July 4, 2103

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See also

Notes

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