June 2076 lunar eclipse

{{Short description|Central lunar eclipse}}

{{Infobox lunar eclipse

| type = total

| image = Lunar eclipse chart close-2076Jun17.png

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

| date = June 17, 2076

| gamma = −0.0452

| magnitude = 1.7959

| saros_ser = 131

| saros_no = 37 of 72

| totality = 100 minutes, 10 seconds

| partiality = 215 minutes, 5 seconds

| penumbral = 325 minutes, 21 seconds

| p1 = 23:54:35

| u1 = 0:49:46

| u2 = 1:47:13

| greatest = 2:37:18

| u3 = 3:27:23

| u4 = 4:24:51

| p4 = 5:19:56

| previous = December 2075

| next = December 2076

}}

A total lunar eclipse will occur at the Moon’s descending node of orbit on Wednesday, June 17, 2076,{{cite web|title=June 16–17, 2076 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2076-june-17|publisher=timeanddate|access-date=14 December 2024}} with an umbral magnitude of 1.7959. 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 18, 2076, at 20:40 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=2076&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 −0.0452 and an umbral eclipse magnitude of 1.7959, this is the second greatest eclipse in Saros series 131 as well as the largest and darkest lunar eclipse between June 26, 2029 and June 28, 2094. Overall, it will be the third largest and darkest lunar eclipse of the 21st century. While it will have similar values to the lunar eclipse of July 16, 2000, totality will not last over 106 minutes due to the moon's relatively large apparent size as seen from Earth and greater speed in its elliptical orbit.

NGC 6401 will be occulted by the Moon during the eclipse over Eastern North America, Cuba, the Atlantic Ocean, Southeast Europe and the northern half of Africa.{{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|160}}

Visibility

The eclipse will be completely visible over South America, west Africa, and Antarctica, seen rising over North America and the eastern Pacific Ocean and setting over Europe, west and south Asia, and central and east Africa.{{cite web|title=Total Lunar Eclipse of 2076 Jun 17|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2051/LE2076Jun17T.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 2076 Jun 17|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2076Jun17Tprime.html|publisher=EclipseWise.com|access-date=14 December 2024}}

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|+June 17, 2076 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.75698

Umbral Magnitude

| 1.79585

Gamma

| −0.04518

Sun Right Ascension

| 05h46m08.2s

Sun Declination

| +23°23'27.6"

Sun Semi-Diameter

| 15'44.6"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 17h46m06.8s

Moon Declination

| -23°26'09.4"

Moon Semi-Diameter

| 16'22.8"

Moon Equatorial Horizontal Parallax

| 1°00'07.0"

ΔT

| 104.8 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. The first and last eclipse in this sequence is separated by one synodic month.

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|+ Eclipse season of June–July 2076

! June 1
Ascending node (new moon)
!! June 17
Descending node (full moon)
!! July 1
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 2076 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 131 =

= Inex =

= Triad =

= Lunar eclipses of 2074–2078 =

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 11, 2074 and August 7, 2074 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 27, 2078 and October 21, 2078 occur in the next lunar year eclipse set.

class="wikitable mw-collapsible mw-collapsed"

!class="nowrap" colspan="9" | Lunar eclipse series sets from 2074 to 2078

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

| 2074 Jul 08

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

| 1.4456

| 116

| 2075 Jan 02

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

| −1.1642

style="text-align: center;"

| 121

| 2075 Jun 28

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

| 0.6897

| 126

| 2075 Dec 22

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

| −0.4945

style="text-align: center;"

| 131

| 2076 Jun 17
80px

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

| −0.0452

| 136

| style="text-align:center;vertical-align:top;" |2076 Dec 10

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

| 0.2102

style="text-align: center;"

| 141

| 2077 Jun 06

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

| −0.8387

| 146

| 2077 Nov 29

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

| 0.8854

style="text-align: center;"

| colspan=4|

| 156

| 2078 Nov 19

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

| 1.5147

= Saros 131 =

{{Lunar Saros series 131}}

= Tritos series =

{{Lunar Tritos series January 2000}}

= Inex series =

{{Lunar Inex series July 2018}}

= 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 11, 2067

!June 22, 2085

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See also

Notes

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