March 2016 lunar eclipse

{{Short description|Penumbral lunar eclipse 23 March 2016}}

{{Infobox lunar eclipse

| type = penumbral

| image = Lunar eclipse chart close-2016Mar23.png

| caption = The hourly motion of the Moon shown right to left

| date = March 23, 2016

| gamma = 1.1592

| magnitude = −0.3107

| saros_ser = 142

| saros_no = 18 of 73

| penumbral = 255 minutes, 21 seconds

| p1 = 09:39:29

| greatest = 11:47:12

| p4 = 13:54:50

| previous = September 2015

| next = August 2016

}}

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, March 23, 2016,{{cite web|title=March 23, 2016 Penumbral Lunar Eclipse|url=https://www.timeanddate.com/eclipse/lunar/2016-march-23|publisher=timeanddate|access-date=16 November 2024}} with an umbral magnitude of −0.3107. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. 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. Occurring about 2 days before apogee (on March 25, 2016, at 10:15 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=2016&n=136|publisher=timeanddate|access-date=16 November 2024}}

Visibility

The eclipse was completely visible over Australia and western North America, seen rising over much of Asia and setting over central and eastern North America and western South America.{{cite web|title=Penumbral Lunar Eclipse of 2016 Mar 23|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2016Mar23N.pdf|publisher=NASA|access-date=16 November 2024}}

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Hourly motion shown right to left

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Visibility map

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=Penumbral Lunar Eclipse of 2016 Mar 23|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2016Mar23Nprime.html|publisher=EclipseWise.com|access-date=16 November 2024}}

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|+March 23, 2016 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 0.77585

Umbral Magnitude

| −0.31071

Gamma

| 1.15916

Sun Right Ascension

| 00h12m02.0s

Sun Declination

| +01°18'10.9"

Sun Semi-Diameter

| 16'02.7"

Sun Equatorial Horizontal Parallax

| 08.8"

Moon Right Ascension

| 12h13m18.6s

Moon Declination

| -00°18'21.4"

Moon Semi-Diameter

| 14'46.0"

Moon Equatorial Horizontal Parallax

| 0°54'11.6"

ΔT

| 68.0 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 March 2016

! March 9
Descending node (new moon)
!! March 23
Ascending node (full moon)

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| Total solar eclipse
Solar Saros 130

Penumbral lunar eclipse
Lunar Saros 142

Related eclipses

= Eclipses in 2016 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 142 =

= Inex =

= Triad =

= Lunar eclipses of 2013–2016 =

{{Lunar eclipse set 2013-2016}}

= Saros 142 =

{{Lunar Saros series 142}}

= Tritos series =

{{Lunar Tritos series April 2005}}

= Inex series =

{{Lunar Inex series March 2016}}

= 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 partial solar eclipses of Solar Saros 149.

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!March 19, 2007

!March 29, 2025

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See also

References