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Showing posts with label Pacific Ocean total lunar eclipse. Show all posts
Showing posts with label Pacific Ocean total lunar eclipse. Show all posts

Friday, April 3, 2015

First Total Lunar Eclipse of 2015 Occurs as Blood Moon on Holy Saturday, April 4


Summary: The first total lunar eclipse of 2015 appears Holy Saturday, April 4, as a blood moon.


graphics and details of total lunar eclipse Saturday, April 4, 2015: "Permission is freely granted to reproduce this data when accompanied by an acknowledgment, Eclipse Predictions by Fred Espenak, NASA GSFC Emeritus," via NASA Eclipse Web Site

The first total lunar eclipse of 2015 appears on the first Saturday in April as the third of a quartet of total lunar eclipses occurring at intervals of approximately six months over a span of 17 months.
In astronomy, the phenomenon of four closely spaced total lunar eclipses, separated successively by about six months, is termed as a tetrad (Ancient Greek: τέσσαρες, téssares, "four"). The total lunar eclipse Tuesday, April 15, 2014, initiated the tetrad. The second in the series occurred Wednesday, Oct. 8, 2014. The fourth occurrence will close the tetrad of 2014-2015 on Monday, Sept. 28, 2015. A popular name for the moons in a lunar tetrad is blood moon.
A total lunar eclipse (Ancient Greek: ἐκ, ek, “out” + λείπω, leípō, “I leave behind”) occurs during the full moon phase of the eight phase monthly lunar cycle. During its full phase, the moon is in syzygy (Ancient Greek: σύζυγος, suzugos, “yoked together”), or alignment, with the sun and the Earth. Positioned in the middle in the solar-lunar sandwich, the Earth casts its shadow upon the moon, thereby eclipsing, or obscuring, the lunar surface.
The show demurely begins Holy Saturday, April 4, at 2:01 a.m. Pacific Daylight Time (5:01 a.m. Eastern Daylight Time; 09:01 Greenwich Mean Time).
The moon encounters the penumbra (Latin: paene, "almost" + umbra, "shadow"), the faint, outer region of Earth's shadow. Apparent within 55 minutes, the penumbral effect imparts a smudginess to the moon's left rim.
Drama vividly commences at 3:16 a.m. PDT (6:16 a.m. EDT; 10:16 GMT), with the moon's passage behind the Earth into the terrestrial umbra (Latin: umbra, "shade, shadow"), or amber-colored shadow. The umbra travels across the lunar disk for 103 minutes (1 hour 43 minutes). At 4:58 a.m. PDT (7:58 a.m. EDT; 11:58 GMT), the umbra completely obscures the moon, as viewed by Earthlings.
Depending upon location, the eclipse is viewable in totality or in partiality. The interruption of the eclipse by sunrise creates a partial eclipse for U.S. locations east of the Mississippi River. Totality, or the total eclipsing of the moon within the earthly shadow, is available for eastern Asia, Oceania, western Canada, mostly Mexico, and U.S. locations west of the mighty Mississippi.
The National Aeronautics and Space Administration (NASA) is providing a live viewing of the first total lunar eclipse of 2015 via Marshall Space Flight Center's Ustream channel.
The live webcast, which starts at 6 a.m. EDT (3 a.m. PDT; 10 GMT), is available at: http://www.ustream.tv/channel/nasa-msfc
This first total lunar eclipse of 2015 stands out as the shortest in duration of totality for the 21st century. Totality only lasts for 4 minutes 43 seconds (283 seconds) because the moon is passing on the periphery, or outskirts, of Earth's sunlight-induced shadow.
Although brief, spring 2015's total lunar eclipse is nonetheless stunningly ablaze as a blood moon. On the other side of the Earth, the sun's light inflames the terrestrial rim so that all the Earth's sunrises and sunsets, through refraction, or bending, bathe the Earth's coverage of the moon with a blood red shadow.

total lunar eclipse Saturday, April 4, 2015, as viewed from the center of the moon during greatest eclipse: Tom Ruen (SockPuppetForTomruen at English Wikipedia), Public Domain, via Wikimedia Commons

Acknowledgment
My special thanks to talented artists and photographers/concerned organizations who make their fine images available on the internet.

Image credits:
graphics and details of total lunar eclipse Saturday, April 4, 2015: "Permission is freely granted to reproduce this data when accompanied by an acknowledgment, Eclipse Predictions by Fred Espenak, NASA GSFC Emeritus," via NASA Eclipse Web Site @ https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2015Apr04T.pdf
total lunar eclipse Saturday, April 4, 2015, as viewed from the center of the moon during greatest eclipse: Tom Ruen (SockPuppetForTomruen at English Wikipedia), Public Domain, via Wikimedia Commons @ https://commons.wikimedia.org/wiki/File:Lunar_eclipse_from_moon-2015Apr04.png

For further information:
Espenak, Fred. “Penumbral Lunar Eclipse of 2020 Jul 05.” NASA Eclipse Web Site > Lunar Eclipses > Lunar Eclipses: 2011-2020. Available via NASA Eclipse Web Site @ https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2020Jul05N.pdf Phillips, Dr. Tony. “Total Eclipse of the Moon.” NASA Science News > Science@NASA Headline News > 2015. March 30, 2015.
Available @ http://science.nasa.gov/science-news/science-at-nasa/2015/30mar_lunareclipse
Rao, Joe. "Total Lunar Eclipse Saturday: How to See the Blood Moon." Space.com. April 3, 2015.
Available @ http://www.space.com/29008-total-lunar-eclipse-saturday-visibility.html
ScienceAtNASA. "ScienceCasts: Total Eclipse of the Moon." YouTube. March 30, 2015.
Available @ https://www.youtube.com/watch?v=_70M4lkLKPk


Wednesday, December 15, 2010

2010 Total Lunar Eclipse Tuesday, Dec. 21, Favors North America


Summary: As the year’s second eclipse of the moon, the 2010 total lunar eclipse Tuesday, Dec. 21, favors North America.


visibility of the Dec. 21, 2010, lunar eclipse: Fred Espenak/NASA Goddard Space Flight Center (GSFC), Public Domain, via Wikimedia Commons

As the year’s second eclipse of the moon, the 2010 total lunar eclipse Tuesday, Dec. 21, favors North America, northwestern South America (Colombia, Ecuador, Peru, Venezuela), Greenland, Iceland, northern Scandinavia and northern Russia with entire visibility.
NASA’s Eclipse Web Site details the astronomical event as beginning at 5:29:17 Universal Time (12:29 a.m. Eastern Standard Time) with a penumbral eclipse, with the lunar passage through the penumbra, the faint, outer cone of Earth’s shadow. Astronomers designate the penumbral start as P1.
At 6:32:37 UT (1:32 a.m. EST), the event’s partial eclipse begins. Partiality signals the movement of only a portion of the visible lunar surface into the umbra, the darkest, innermost segment of Earth’s shadow. U1 designates the start of partiality.
At 7:40:47 UT (2:40 a.m. EST), the total eclipse begins. Totality indicates the moon’s complete movement into Earth’s umbra. U2 is the astronomical designation for the start of totality.
Greatest eclipse takes place at 8:16:57 UT (3:16 a.m. EST). Greatest eclipse references the instant of the moon's closest passage to the axis of Earth's shadow.
The total eclipse ends at 8:53:08 UT (3:53 a.m. EST). U3 designates the end of totality.
The partial eclipse ends at 10:01:20 UT (5:01 a.m. EST). U4 designates the end of partiality.
At 11:04:31 UT (6:04 a.m. EST) the penumbral eclipse ends. P4 designates the penumbral end.
The penumbral eclipse frames the December 2010 lunar event. The penumbral eclipse, occurring from 5:29:17 UT (12:29 a.m. EST) to 11:04 UT (6:04:31 a.m. EST), accounts for 5 hours 35 minutes 14 seconds.
Like a set of Russian nesting dolls, the penumbral eclipse encompasses a partial eclipse and a total eclipse within its time span. Partiality, spanning 6:32:37 UT (1:32 a.m. EST) to 10:01:20 UT (5:01 a.m. EST), has a duration of 3 hours 28 minutes 43 seconds. Totality, which runs from 7:40 UT (2:40:47 a.m. EST) to 8:53:08 UT (3:53 a.m. EST), has a duration of 1 hour 12 minutes 21 seconds.
The 2010 total lunar eclipse ends a drought of almost 2 years 10 months of no total lunar eclipses. The most recent predecessor of the Dec. 21, 2010, total lunar eclipse took place early in 2008.
Time And Date’s web site frames the 2008 total lunar eclipse with a penumbral eclipse that started at 00:36:36 UT, Thursday, Feb. 21 (7:36 p.m. EST, Wednesday, Feb. 20) and ended Feb. 21 at 6:15:36 UT (1:15 a.m. EST). Totality occurred between 3:01:10 UT, Feb. 21 (10:01 p.m. EST, Feb. 20) and 3:50:54 UT, Feb. 21 (10:50 p.m. EST, Feb. 20).
The 2010 total lunar eclipse also shares its date with the Northern Hemisphere’s winter solstice, which is known as the summer solstice in the Southern Hemisphere. The second of the two annual solstices takes place Dec. 21, 2010, at 23:38 UT (6:38 p.m. EST). A span of about 12 hours 34 minutes separates the end of the day’s lunar eclipse and the solstice’s official start.
The 2010 total lunar eclipse Tuesday, Dec. 21, happens as the second of the year’s two lunar eclipses. The year’s first lunar eclipse occurred Saturday, June 26, as a partial lunar eclipse.
December 2010's total lunar eclipse belongs to Saros 125. The Saros cycle for lunar and solar eclipses encompasses a period of 18 years 11 days 8 hours (approximately 6,585.3 days). The Saros cycle organizes eclipses into families, known as series.
The takeaway for the 2010 total lunar eclipse Tuesday, Dec. 21, is that the event favors North America as the only continent with entire visibility, coincides with the year’s December solstice and ends a 2 year 9-plus month drought of total lunar eclipses.

moon’s approximate appearance during passage through Earth’s shadows, with red glowing light inside the umbral shadow: SockPuppetForTomruen at English Wikipedia, Public Domain, via Wikimedia Commons

Acknowledgment
My special thanks to talented artists and photographers/concerned organizations who make their fine images available on the internet.

Image credits:
visibility of the Dec. 21, 2010, lunar eclipse: Fred Espenak/NASA Goddard Space Flight Center (GSFC), Public Domain, via Wikimedia Commons @ https://commons.wikimedia.org/wiki/File:Visibility_Lunar_Eclipse_2010-12-21.png
moon’s approximate appearance during passage through Earth’s shadows, with red glowing light inside the umbral shadow: SockPuppetForTomruen at English Wikipedia, Public Domain, via Wikimedia Commons @ https://commons.wikimedia.org/wiki/File:Lunar_eclipse_chart_close-2010Dec21_animation.gif

For further information:
“February 20 / February 21, 2008 -- Total Lunar Eclipse.” Time And Date > Sun & Moon > Eclipses.
Available @ https://www.timeanddate.com/eclipse/lunar/2008-february-21
“December 20 / December 21, 2010 -- Total Lunar Eclipse.” Time And Date > Sun & Moon > Eclipses.
Available @ https://www.timeanddate.com/eclipse/lunar/2010-december-21
“Earth’s Seasons: Equinoxes, Solstices, Perihelion, and Aphelion.” U.S. Naval Observatory Astronomical Applications Department > Data Services.
Available @ http://aa.usno.navy.mil/data/docs/EarthSeasons.php
Espenak, Fred. “2010 Dec 21: Total Lunar Eclipse.” NASA Eclipse Web Site > Eclipses During 2010.
Available @ https://eclipse.gsfc.nasa.gov/OH/OH2010.html
Espenak, Fred; Jean Meeus. "Saros Series 125." NASA Eclipse Web Site > Lunar Eclipses > Catalog of Lunar Eclipse Saros Series.
Available @ https://eclipse.gsfc.nasa.gov/LEsaros/LEsaros125.html
Marriner, Derdriu. "Dec. 21, 2010, Total Lunar Eclipse Belongs to Saros Cycle 125." Earth and Space News. Wednesday, Dec. 8, 2010.
Available @ https://earth-and-space-news.blogspot.com/2010/12/dec-21-2010-total-lunar-eclipse-belongs.html
Marriner, Derdriu. "One Exeligmos Unites Dec. 21, 2010, and Nov. 18, 1956, Lunar Eclipses." Earth and Space News. Wednesday, Dec. 1, 2010.
Available @ https://earth-and-space-news.blogspot.com/2010/12/one-exeligmos-unites-dec-21-2010-and.html
“When Is the Longest/Shortest Day? Summer/Winter Solstices and Spring/Autumn Equinoxes.” Greenwich Mean Time.
Available @ https://greenwichmeantime.com/longest-day/equinox-solstice-2010-2019/