August 2007 lunar eclipse

{{short description|Central lunar eclipse}}

{{Use dmy dates|date=July 2021}}

{{Infobox lunar eclipse

| type = total

| image = Lunar Eclipse.jpg

| caption = The eclipse as viewed from Wollongong, Australia at 9:48 UTC, shortly before totality

| date = August 28, 2007

| gamma = −0.2145

| magnitude = 1.4777

| saros_ser = 128

| saros_no = 40 of 71

| totality = 90 minutes, 1 second

| partiality = 212 minutes, 12 seconds

| penumbral = 327 minutes, 17 seconds

| p1 = 7:53:40

| u1 = 8:51:16

| u2 = 9:52:21

| greatest = 10:37:21

| u3 = 11:22:22

| u4 = 12:23:28

| p4 = 13:20:57

| previous = March 2007

| next = February 2008

}}

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, August 28, 2007,{{cite web|title=August 27–28, 2007 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2007-august-27|publisher=timeanddate|access-date=14 November 2024}} with an umbral magnitude of 1.4777. It was a central lunar eclipse, in which part of the Moon passed 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 2.4 days before perigee (on August 30, 2007, at 20:10 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=2007&n=136|publisher=timeanddate|access-date=14 November 2024}}

This was the most recent central lunar eclipse of Saros series 128 as well as the "longest and deepest lunar eclipse to be seen in 7 years". In the total lunar eclipse of July 16, 2000 the moon passed within two arc minutes of the center of the Earth's shadow. In comparison, this still very deep eclipse was off-center by over 12 minutes of arc.[http://sunearth.gsfc.nasa.gov/eclipse/LEplot/LEplot1951/LE2000Jul16T.pdf Visibility Map]{{dead link|date=June 2021|bot=medic}}{{cbignore|bot=medic}} for Total Lunar Eclipse of 16 July 2000

The next total lunar eclipse of a longer duration was on June 15, 2011.

Visibility

Viewing from Oceania was favored for the eclipse, because at the moment of greatest eclipse (10:37:22 UTC), the Moon was at the zenith of French Polynesia. The Pacific regions of Canada and the continental United States (including all of Alaska) witnessed the whole event, along with most of eastern Australia, New Zealand and all the Pacific Island regions (except New Guinea), and the tip of the Chukchi Peninsula that includes the town of Uelen, Russia. The majority of the Americas observed an abbreviated eclipse, with moonset occurring at some time during the eclipse. Siberia, far eastern Russia, eastern South Asia, China, the rest of eastern and southeastern Asia, New Guinea, and the rest of Australia missed out on the beginning of the eclipse, because the eclipse occurred at or close to moonrise in those regions.[http://sunearth.gsfc.nasa.gov/eclipse/LEplot/LEplot2001/LE2007Aug28T.pdf Visibility Map]{{dead link|date=June 2021|bot=medic}}{{cbignore|bot=medic}} for Total Lunar Eclipse of 28 August 2007

Luzon (except Visayas and Mindanao) in the Philippines, particularly Metro Manila, missed the rare eclipse entirely, due to clouds in the area due to the rainy season, which saddened many eclipse watchers in the area, but the eclipse was sighted by other amateur astronomers in other parts of the country as the lunar eclipse seen in clear skies. The eclipse was also missed in New Guinea, especially Port Moresby because of clouds. Greenland, Europe (including western Russia), Africa, western Asia, western Central Asia, and western South Asia missed the eclipse completely.{{cite web|title=Total Lunar Eclipse of 2007 Aug 28|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2007Aug28T.pdf|publisher=NASA|access-date=14 November 2024}}

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Hourly motion shown right to left

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The Moon's hourly motion across the Earth's shadow in the constellation of Aquarius.

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Visibility map

Images

Gallery

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|+ Collages

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From the Oregon Coast.

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From Swifts Creek, Australia.
(3 minute intervals)

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From Bakersfield, California.

File:LuckEclipseMoon.JPG|From Nagayo, Nagasaki, 10:33 UTC.

File:Lunar eclipse with stars.JPG|A wider angle shows stars around the moon.

File:Total lunar eclipse and milky way.jpg|A full sky view (moon on left) shows the Milky Way (across the center), which is usually invisible under a full moon.

File:2007-08-28 Melbourne lunar eclipse Dsc 2519.jpg|From Melbourne, Australia.

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Total Lunar Eclipse of 2007 Aug 28|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2007Aug28Tprime.html|publisher=EclipseWise.com|access-date=14 November 2024}}

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|+August 28, 2007 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.45448

Umbral Magnitude

| 1.47769

Gamma

| −0.21456

Sun Right Ascension

| 10h26m26.9s

Sun Declination

| +09°45'56.7"

Sun Semi-Diameter

| 15'50.0"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 22h26m50.4s

Moon Declination

| -09°57'18.5"

Moon Semi-Diameter

| 16'12.5"

Moon Equatorial Horizontal Parallax

| 0°59'29.2"

ΔT

| 65.4 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.

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|+ Eclipse season of August–September 2007

! August 28
Ascending node (full moon)
!! September 11
Descending node (new moon)

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| Total lunar eclipse
Lunar Saros 128

Partial solar eclipse
Solar Saros 154

Related eclipses

= Eclipses in 2007 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 128 =

= Inex =

= Triad =

= Lunar eclipses of 2006–2009 =

{{Lunar eclipse set 2006-2009}}

= Metonic series =

{{Metonic lunar eclipse 1988-2045}}

= Saros 128 =

{{Lunar Saros series 128}}

= Tritos series =

{{Lunar Tritos series August 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 135.

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!August 22, 1998

!September 1, 2016

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See also

Notes

{{reflist|2}}