February 2017 lunar eclipse

{{Short description|Penumbral lunar eclipse 11 February 2017}}

{{Use dmy dates|date=April 2017}}

{{Infobox lunar eclipse

| type = penumbral

| image = Penumbral lunar eclipse 2017.02.11.jpg

| caption = Penumbral eclipse as viewed from Rabka-Zdrój, Poland, 0:51 UTC

| date = February 11, 2017

| gamma = -1.0254

| magnitude = −0.0342

| saros_ser = 114

| saros_no = 59 of 71

| penumbral = 259 minutes, 10 seconds

| p1 = 22:34:16

| greatest = 0:43:53

| p4 = 2:53:26

| previous = September 2016

| next = August 2017

}}

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, February 11, 2017,{{cite web|title=February 10–11, 2017 Penumbral Lunar Eclipse|url=https://www.timeanddate.com/eclipse/lunar/2017-february-11|publisher=timeanddate|access-date=16 November 2024}} with an umbral magnitude of −0.0342. It was not quite a total penumbral lunar eclipse. 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 4.6 days before perigee (on February 6, 2017, at 9:00 UTC), the Moon's apparent diameter was larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2017&n=136|publisher=timeanddate|access-date=16 November 2024}}

This eclipse occurred the same day as comet 45P/Honda–Mrkos–Pajdušáková made a close approach to Earth (0.08318 AU). It also occurred on the Lantern Festival, the first eclipse to do so since February 9, 2009.

Visibility

The eclipse was completely visible over northeastern North America, eastern South America, Europe, Africa, and west Asia, seen rising over much of North America and western South America and setting over south and east Asia.{{cite web|title=Penumbral Lunar Eclipse of 2017 Feb 11|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2017Feb11N.pdf|publisher=NASA|access-date=17 November 2024}}

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Hourly motion shown right to left

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Visibility map

Gallery

Eclipse penumbral de luna 10 de febrero de 2017 (32113541604).jpg|Popayán, Colombia, 23:43 UTC (10 February)

"Snow Moon" (32828803125).jpg|Kissimmee, Florida, 0:00 UTC

Moon (32787383146).jpg|Tampa, Florida, 0:11 UTC

Full Snow Moon and Eclipse. (32830589985).jpg|Time lapse images from Melbourne, Florida

Penumbral eclipse of the Moon 2017 (32705078711).jpg|Bracciano, Italy, 0:29 UTC

Full Moon and Penumbral Eclipse on 2-10-17 (32707190401).jpg|Macon, Georgia, 0:38 UTC

Lunar eclipse 2-10 (32850077545).jpg|Naperville, Illinois, 1:23 UTC

Innsbruck, Austria (Unsplash XA6OmUYqn4k).jpg|Innsbruck, Austria, ~2:00 UTC

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 2017 Feb 11|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2017Feb11Nprime.html|publisher=EclipseWise.com|access-date=17 November 2024}}

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|+February 11, 2017 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 0.98956

Umbral Magnitude

| −0.03421

Gamma

| −1.02548

Sun Right Ascension

| 21h39m19.2s

Sun Declination

| -14°01'07.8"

Sun Semi-Diameter

| 16'12.3"

Sun Equatorial Horizontal Parallax

| 08.9"

Moon Right Ascension

| 09h38m22.6s

Moon Declination

| +13°03'10.2"

Moon Semi-Diameter

| 15'49.8"

Moon Equatorial Horizontal Parallax

| 0°58'05.6"

ΔT

| 68.3 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 February 2017

! February 11
Ascending node (full moon)
!! February 26
Descending node (new moon)

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| Penumbral lunar eclipse
Lunar Saros 114

Annular solar eclipse
Solar Saros 140

Related eclipses

= Eclipses in 2017 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 114 =

= Inex =

= Triad =

= Lunar eclipses of 2016–2020 =

{{Lunar eclipse set 2016-2020}}

= Saros 114 =

{{Lunar Saros series 114}}

= Tritos series =

{{Lunar Tritos series March 2006}}

= Inex series =

{{Lunar Inex series February 2017}}

= 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 121.

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!February 7, 2008

!February 17, 2026

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See also

References

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