June 2123 lunar eclipse

{{short description|Spectacular long central lunar eclipse}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-2123Jun09.png

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

| date = June 9, 2123

| gamma = 0.0406

| magnitude = 1.7488

| saros_ser = 132

| saros_no = 36 of 71

| totality = 106 minutes, 6 seconds

| partiality = 235 minutes, 47 seconds

| penumbral = 374 minutes, 23 seconds

| p1 = 1:56:43

| u1 = 3:06:02

| u2 = 4:10:52

| greatest = 5:03:55

| u3 = 5:56:58

| u4 = 7:01:48

| p4 = 8:11:06

| previous = December 2122

| next = December 2123

}}

A total lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, June 9, 2123,{{cite web|title=June 8–9, 2123 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2123-june-9|publisher=timeanddate|access-date=15 December 2024}} with an umbral magnitude of 1.7488. 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 1.4 days after apogee (on June 7, 2123, at 19:20 UTC), the Moon's apparent diameter will be smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2123&n=136|publisher=timeanddate|access-date=15 December 2024}}

This dramatic total eclipse, lasting 106 minutes and 6 seconds, will plunge the full Moon into deep darkness as it passes right through the center of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 56 minutes in total. The penumbral eclipse lasts for 6 hours and 14 minutes. This will be the longest total lunar eclipse since July 16, 2000 (106 minutes, 25 seconds), and the longest one until May 12, 2264 (106 minutes, 13 seconds) and July 27, 3107 (106 minutes, 21 seconds), though the eclipse on June 19, 2141 will be nearly identical in all aspects.{{Cite web|url=http://eclipsewise.com/lunar/LEsaros/LEsaros166.html|title=EclipseWise - Catalog of Lunar Eclipses of Saros 166}} This will also be the longest of the 22nd century and the second longest of the 3rd millennium.{{Cite web|url=http://eclipsewise.com/lunar/LEcatalog/LEcatalog.html|title = EclipseWise - Six Millennium Catalog of Lunar Eclipses}} The eclipse on June 19, 2141 will be the second longest of the 22nd century and the third longest of the third millennium (at 106 minutes 5 seconds).

Visibility

The eclipse will be completely visible over eastern and central North America, South America, and Antarctica, seen rising over western North America, eastern Australia, and the central Pacific Ocean and setting over Europe, Africa, and the Middle East.

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 2123 Jun 09|url=https://eclipsewise.com/lunar/LEprime/2101-2200/LE2123Jun09Tprime.html|publisher=EclipseWise.com|access-date=15 December 2024}}

class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"

|+June 9, 2123 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.81895

Umbral Magnitude

| 1.74877

Gamma

| 0.04055

Sun Right Ascension

| 05h07m45.7s

Sun Declination

| +22°52'47.0"

Sun Semi-Diameter

| 15'45.7"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 17h07m45.6s

Moon Declination

| -22°50'35.5"

Moon Semi-Diameter

| 14'43.7"

Moon Equatorial Horizontal Parallax

| 0°54'03.0"

ΔT

| 153.5 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.

class="wikitable"

|+ Eclipse season of May–June 2123

! May 25
Descending node (new moon)
!! June 9
Ascending node (full moon)
!! June 23
Descending node (new moon)

200px200px200px
align=center

| Partial solar eclipse
Solar Saros 120

Total lunar eclipse
Lunar Saros 132
Partial solar eclipse
Solar Saros 158

Related eclipses

= Eclipses in 2123 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 132 =

= Inex =

= Triad =

= Lunar eclipses of 2121–2125 =

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 2, 2121 and July 30, 2121 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 18, 2125 and October 12, 2125 occur in the next lunar year eclipse set.

class="wikitable mw-collapsible mw-collapsed"

!class="nowrap" colspan="9" | Lunar eclipse series sets from 2121 to 2125

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

| rowspan="11" | 

! scope="col" colspan="4" | Descending 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;"

| 112

| 2121 Jun 30

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

| −1.4272

| 117

| 2121 Dec 24

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

| 1.2261

style="text-align: center;"

| 122

| 2122 Jun 20

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

| −0.7177

| 127

| 2122 Dec 13

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

| 0.4979

style="text-align: center;"

| 132

| style="text-align:center;vertical-align:top;" |2123 Jun 09

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

| 0.0406

| 137

| style="text-align:center;vertical-align:top;" |2123 Dec 03

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

| −0.1755

style="text-align: center;"

| 142

| 2124 May 28

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

| 0.7913

| 147

| 2124 Nov 21

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

| −0.8808

style="text-align: center;"

| 152

| 2125 May 17

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

| 1.4923

= Saros 132 =

{{Lunar Saros series 132}}

= Tritos series =

{{Lunar Tritos series May 2003}}

= 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 total solar eclipses of Solar Saros 139.

class=wikitable

!June 3, 2114

!June 13, 2132

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|240px

References

{{Lunar eclipses}}

{{DEFAULTSORT:Lunar eclipse 2123-06}}

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