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"content": "\u003cp>On Thursday night into early Friday morning, residents in the Bay Area will be able to witness a spectacular total lunar eclipse — often called a “\u003ca href=\"https://www.kqed.org/science/1979293/how-to-see-sundays-blood-moon-total-lunar-eclipse-in-the-bay-area\">blood moon\u003c/a>” due to its deep red hue.\u003c/p>\n\u003cul>\n\u003cli>\u003cstrong>\u003ca href=\"#how-to-see-blood-moon\">Jump straight to: What time is the lunar eclipse in the Bay Area tonight?\u003c/a>\u003c/strong>\u003c/li>\n\u003c/ul>\n\u003cp>This celestial event happens when the Earth moves directly between the sun and the moon, casting a shadow that darkens the moon and turns it into a striking shade of red during totality. And unlike solar eclipses, which require special glasses, you can enjoy the lunar eclipse with the naked eye.\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>The last time a \u003ca href=\"https://www.kqed.org/science/1994403/a-celestial-trifecta-what-to-know-about-tuesdays-lunar-eclipse\">total lunar eclipse was visible\u003c/a> from North America was just two years ago, in November 2022. “These total eclipses of the moon happen much more frequently than the total eclipses of the sun at any given location because you can see the full moon all over part of the Earth,” said Andrew Fraknoi, astronomer and professor at the University of San Francisco’s Fromm Institute.\u003c/p>\n\u003cp>A lunar eclipse is visible to anyone on the night side of Earth. In contrast, total solar eclipses are only visible along a narrow path of totality — sometimes just a few hundred miles wide.\u003c/p>\n\u003cfigure id=\"attachment_1996241\" class=\"wp-caption aligncenter\" style=\"max-width: 1041px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1996241\" src=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy.jpg\" alt=\"\" width=\"1041\" height=\"783\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy.jpg 1041w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-768x578.jpg 768w\" sizes=\"auto, (max-width: 1041px) 100vw, 1041px\">\u003cfigcaption class=\"wp-caption-text\">When Earth passes directly between the sun and the moon, a lunar eclipse takes place. \u003ccite>(National Aeronautics and Space Administration)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>\u003cstrong>\u003ca id=\"how-to-see-blood-moon\">\u003c/a>What time is the lunar eclipse tonight, and where can I see it in the Bay Area?\u003c/strong>\u003c/h2>\n\u003cp>This upcoming total lunar eclipse will be fully visible across the Bay Area tonight as long as you have a clear view of the moon.\u003c/p>\n\u003cp>It will begin at around 10 p.m. P.S.T. on Thursday, March 13, and totality will occur at 11:26 p.m. The maximum eclipse — when the moon will be its reddest — will occur at 11:59 p.m. and last for about 30 minutes into the early hours of Friday, March 14.\u003c/p>\n\u003cp>The whole eclipse phase will last for about 64 minutes, from 10 p.m. to 1:47 a.m., with the best views occurring between 11:26 p.m. to 12:31 a.m.[aside postID=science_1996198 hero='https://cdn.kqed.org/wp-content/uploads/sites/35/2025/02/GettyImages-1242378655-1020x680.jpg']\u003c/p>\n\u003cp>“As the moon moves slowly through the Earth’s shadow, we first see only part of the moon darkening,” Fraknoi said of the partial eclipse. “But then, as the Moon moves fully into the Earth’s shadow, we see its entire disk of the Moon become dark and reddish.”\u003c/p>\n\u003cp>During totality, the moon glows red because of \u003ca href=\"https://www.britannica.com/science/Rayleigh-scattering\">Rayleigh scattering,\u003c/a> the same phenomenon that makes \u003ca href=\"https://www.kqed.org/news/11979339/bay-areas-best-sunset-hikes-now-that-your-days-are-longer\">sunsets appear orange and red\u003c/a>. As sunlight passes through Earth’s atmosphere, it filters out blue light and bends red light toward the moon, giving it that signature “blood” color.\u003c/p>\n\u003cp>The exact shade of red depends on atmospheric conditions like dust, pollution and volcanic activity elsewhere, which can intensify the red hue, Fraknoi said.\u003c/p>\n\u003cp>Astronomers have used calculations to predict lunar eclipses for centuries. “It’s a really nice indication that even if things are in turmoil on Earth, the heavens are doing their thing in a routine way,” Fraknoi said.\u003c/p>\n\u003cp>“It shows the clockwork motion of the heavens.”\u003c/p>\n\u003cp>\u003c/p>\n",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>On Thursday night into early Friday morning, residents in the Bay Area will be able to witness a spectacular total lunar eclipse — often called a “\u003ca href=\"https://www.kqed.org/science/1979293/how-to-see-sundays-blood-moon-total-lunar-eclipse-in-the-bay-area\">blood moon\u003c/a>” due to its deep red hue.\u003c/p>\n\u003cul>\n\u003cli>\u003cstrong>\u003ca href=\"#how-to-see-blood-moon\">Jump straight to: What time is the lunar eclipse in the Bay Area tonight?\u003c/a>\u003c/strong>\u003c/li>\n\u003c/ul>\n\u003cp>This celestial event happens when the Earth moves directly between the sun and the moon, casting a shadow that darkens the moon and turns it into a striking shade of red during totality. And unlike solar eclipses, which require special glasses, you can enjoy the lunar eclipse with the naked eye.\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>The last time a \u003ca href=\"https://www.kqed.org/science/1994403/a-celestial-trifecta-what-to-know-about-tuesdays-lunar-eclipse\">total lunar eclipse was visible\u003c/a> from North America was just two years ago, in November 2022. “These total eclipses of the moon happen much more frequently than the total eclipses of the sun at any given location because you can see the full moon all over part of the Earth,” said Andrew Fraknoi, astronomer and professor at the University of San Francisco’s Fromm Institute.\u003c/p>\n\u003cp>A lunar eclipse is visible to anyone on the night side of Earth. In contrast, total solar eclipses are only visible along a narrow path of totality — sometimes just a few hundred miles wide.\u003c/p>\n\u003cfigure id=\"attachment_1996241\" class=\"wp-caption aligncenter\" style=\"max-width: 1041px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1996241\" src=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy.jpg\" alt=\"\" width=\"1041\" height=\"783\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy.jpg 1041w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2025/03/lunar-eclipse-diagram_0-copy-768x578.jpg 768w\" sizes=\"auto, (max-width: 1041px) 100vw, 1041px\">\u003cfigcaption class=\"wp-caption-text\">When Earth passes directly between the sun and the moon, a lunar eclipse takes place. \u003ccite>(National Aeronautics and Space Administration)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>\u003cstrong>\u003ca id=\"how-to-see-blood-moon\">\u003c/a>What time is the lunar eclipse tonight, and where can I see it in the Bay Area?\u003c/strong>\u003c/h2>\n\u003cp>This upcoming total lunar eclipse will be fully visible across the Bay Area tonight as long as you have a clear view of the moon.\u003c/p>\n\u003cp>It will begin at around 10 p.m. P.S.T. on Thursday, March 13, and totality will occur at 11:26 p.m. The maximum eclipse — when the moon will be its reddest — will occur at 11:59 p.m. and last for about 30 minutes into the early hours of Friday, March 14.\u003c/p>\n\u003cp>The whole eclipse phase will last for about 64 minutes, from 10 p.m. to 1:47 a.m., with the best views occurring between 11:26 p.m. to 12:31 a.m.\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>“As the moon moves slowly through the Earth’s shadow, we first see only part of the moon darkening,” Fraknoi said of the partial eclipse. “But then, as the Moon moves fully into the Earth’s shadow, we see its entire disk of the Moon become dark and reddish.”\u003c/p>\n\u003cp>During totality, the moon glows red because of \u003ca href=\"https://www.britannica.com/science/Rayleigh-scattering\">Rayleigh scattering,\u003c/a> the same phenomenon that makes \u003ca href=\"https://www.kqed.org/news/11979339/bay-areas-best-sunset-hikes-now-that-your-days-are-longer\">sunsets appear orange and red\u003c/a>. As sunlight passes through Earth’s atmosphere, it filters out blue light and bends red light toward the moon, giving it that signature “blood” color.\u003c/p>\n\u003cp>The exact shade of red depends on atmospheric conditions like dust, pollution and volcanic activity elsewhere, which can intensify the red hue, Fraknoi said.\u003c/p>\n\u003cp>Astronomers have used calculations to predict lunar eclipses for centuries. “It’s a really nice indication that even if things are in turmoil on Earth, the heavens are doing their thing in a routine way,” Fraknoi said.\u003c/p>\n\u003cp>“It shows the clockwork motion of the heavens.”\u003c/p>\n\u003cp>\u003c/p>\n\u003c/div>\u003c/p>",
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"title": "A Rare and Beautiful Total Lunar Eclipse: What Time to Watch It on Tuesday Morning",
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"content": "\u003cp>A rare perfect alignment of sun, Earth and moon will take place in the early morning hours of Tuesday, November 8, setting the stage for one of the most spectacular celestial events of the night sky: \u003ca href=\"https://moon.nasa.gov/moon-in-motion/eclipses/\" target=\"_blank\" rel=\"noopener noreferrer\">a total lunar eclipse\u003c/a>.\u003c/p>\n\u003cp>The full moon will pass through the point in the sky exactly opposite the sun and be painted in inky darkness by Earth’s shadow.\u003c/p>\n\u003cp>A special treat is in store for sky enthusiasts around the Bay Area and along the West Coast, where \u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-november-8\">the eclipse will be visible from beginning to end\u003c/a>, without interruption by moonrise or moonset.\u003c/p>\n\u003cfigure id=\"attachment_1980620\" class=\"wp-caption aligncenter\" style=\"max-width: 1024px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980620 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap.jpg\" alt=\"A map of the world in the background. A red moon in the center foreground with purple, blue, green yellow, orange and red lines extending across the image.\" width=\"1024\" height=\"576\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap.jpg 1024w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-768x432.jpg 768w\" sizes=\"(max-width: 1024px) 100vw, 1024px\">\u003cfigcaption class=\"wp-caption-text\">World map showing where, and how much of, the total lunar eclipse on Nov. 8, 2022, will be visible. The entire sequence of this eclipse (shown as the darkest region on the map) will be visible from half of the Pacific Ocean, including the entire West Coast of the US. Times are shown in Coordinated Universal Time (Greenwich Mean Time). \u003ccite>(NASA/Goddard Space Flight Center/Scientific Visualization Studio)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>When is the eclipse?\u003c/h2>\n\u003cp>The eclipse begins Tuesday morning at 12:02 a.m. PST, when the moon first encounters Earth’s partial, or penumbral, shadow. You may not see much of a change immediately, but over the next hour you can witness a subtle dimming of the full moon’s brightness.\u003c/p>\n\u003cp>The real show begins at 1:09 a.m., when the moon contacts Earth’s full shadow, the \u003ca href=\"https://www.nasa.gov/audience/forstudents/k-4/stories/umbra-and-penumbra\" target=\"_blank\" rel=\"noopener noreferrer\">dark umbra \u003c/a>blocking all sunlight. In the moments after, a prominent darkening will appear at the moon’s edge as the shadow nibbles away at the bright lunar disk. By 1:50 a.m., half of the moon will be consumed.\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>Chabot Space and Science Center is hosting a \u003ca href=\"https://chabotspace.org/calendar/total-lunar-eclipse-2/\">Total Lunar Eclipse Watch Party\u003c/a> from 11:30 p.m. on Monday evening until 4 a.m. Tuesday morning.\u003c/p>\n\u003cfigure id=\"attachment_1980616\" class=\"wp-caption aligncenter\" style=\"max-width: 1920px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980616 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/umbra-penumbra-NASA.jpg\" alt=\"A diagram that shows two grey triangles streaming behind Earth's north and south poles -- that's the Penumbra. And a black triangle, Earth's Umbra, streaming from the equator. \" width=\"1920\" height=\"1080\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA.jpg 1920w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-1536x864.jpg 1536w\" sizes=\"(max-width: 1920px) 100vw, 1920px\">\u003cfigcaption class=\"wp-caption-text\">Illustration of Earth’s partial (penumbral) and full (umbral) shadows. When the moon passes through Earth’s shadow, we witness a lunar eclipse. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>Totality\u003c/h2>\n\u003cp>The climax of the eclipse, what’s known as “totality,” starts at 2:16 a.m. and will last almost an hour and a half. This is when the moon is fully engulfed in Earth’s dark umbra. The moon will be deepest in shadow and darkest at 2:59 a.m. If you’re only interested in waking for a few moments to catch a glimpse of the eclipse, this is the time to set your alarm for.\u003c/p>\n\u003cp>Totality ends at 3:41 a.m., when the moon begins to emerge from the umbral shadow into the partial sunlight of the penumbra, where only some of the sun’s light is blocked. If you’re a die-hard fan of lunar eclipses, you can stay up until the eclipse officially ends at 5:56 a.m. — but totality is the best part of the show, so when that’s over you can go back to bed and not worry about missing much.\u003c/p>\n\u003ch2>Why doesn’t the moon completely disappear at totality?\u003c/h2>\n\u003cp>During a total lunar eclipse, the moon passes through Earth’s full shadow, the umbra, where no direct sunlight falls, yet it is still lit up in a dull orange or reddish light.\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Sunlight that slips around the edges of the Earth is bent and filtered by our atmosphere, its twilight rays \u003ca href=\"https://earthsky.org/space/when-can-you-see-earths-shadow/\">shining into the dark umbra\u003c/a> like a dim night-light. We see the same rosy glow at dusk every evening as sunlight is scattered over the horizon to illuminate the landscape, even after the sun has set. The same atmospheric glow passes on into space, shedding its radiance into Earth’s shadow. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1980621\" class=\"wp-caption aligncenter\" style=\"max-width: 900px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980621 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/Luneclipse-1-20-2000s.jpg\" alt=\"The white moon partially shadowed in red and white. \" width=\"900\" height=\"599\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s.jpg 900w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-800x532.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-160x106.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-768x511.jpg 768w\" sizes=\"(max-width: 900px) 100vw, 900px\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse on Jan. 20, 2000. This photograph was taken during totality; one edge of the moon appears brighter since it was crossing near the edge of Earth’s dark umbral shadow, and not deeply through the center. \u003ccite>(Chabot Space and Science Center/Conrad Jung)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400\">An astronaut standing on the moon and looking back at the Earth during a total lunar eclipse would see a black disk rimmed in a ring of fiery light that includes all the Earth’s sunrises and sunsets in one stunning view.\u003c/span>\u003c/p>\n\u003ch2>How often do lunar eclipses occur?\u003c/h2>\n\u003cp>\u003ca href=\"https://nineplanets.org/total-lunar-eclipse/\">Lunar eclipses occur regularly\u003c/a>, anywhere between two and four times per year. Some are partial eclipses, when the moon only grazes Earth’s umbral shadow. Some are penumbral eclipses, where the moon misses the umbra completely and only passes through Earth’s half-shadow, its light dimming so subtly it might not even be noticed.\u003c/p>\n\u003cp>A total lunar eclipse happens about every two and a half years, on average, and is only visible from half of our planet, and in some locations only partially. So, November’s full, end-to-end eclipse is a very rare treat for people on the West Coast who can enjoy it — and well worth getting up in the middle of the night to witness.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>\u003cem>Benjamin Burress has been a staff astronomer at Chabot Space and Science Center since July 1999.\u003c/em>\u003c/p>\n\n",
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"excerpt": "A rare perfect alignment of sun, Earth and moon will produce a total lunar eclipse in the early morning hours of Tuesday, November 8. The climax of the eclipse starts at 2:16 a.m.",
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"description": "A rare perfect alignment of sun, Earth and moon will produce a total lunar eclipse in the early morning hours of Tuesday, November 8. The climax of the eclipse starts at 2:16 a.m.",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>A rare perfect alignment of sun, Earth and moon will take place in the early morning hours of Tuesday, November 8, setting the stage for one of the most spectacular celestial events of the night sky: \u003ca href=\"https://moon.nasa.gov/moon-in-motion/eclipses/\" target=\"_blank\" rel=\"noopener noreferrer\">a total lunar eclipse\u003c/a>.\u003c/p>\n\u003cp>The full moon will pass through the point in the sky exactly opposite the sun and be painted in inky darkness by Earth’s shadow.\u003c/p>\n\u003cp>A special treat is in store for sky enthusiasts around the Bay Area and along the West Coast, where \u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-november-8\">the eclipse will be visible from beginning to end\u003c/a>, without interruption by moonrise or moonset.\u003c/p>\n\u003cfigure id=\"attachment_1980620\" class=\"wp-caption aligncenter\" style=\"max-width: 1024px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980620 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap.jpg\" alt=\"A map of the world in the background. A red moon in the center foreground with purple, blue, green yellow, orange and red lines extending across the image.\" width=\"1024\" height=\"576\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap.jpg 1024w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/nov0822-totallunareclipse-worldmap-768x432.jpg 768w\" sizes=\"(max-width: 1024px) 100vw, 1024px\">\u003cfigcaption class=\"wp-caption-text\">World map showing where, and how much of, the total lunar eclipse on Nov. 8, 2022, will be visible. The entire sequence of this eclipse (shown as the darkest region on the map) will be visible from half of the Pacific Ocean, including the entire West Coast of the US. Times are shown in Coordinated Universal Time (Greenwich Mean Time). \u003ccite>(NASA/Goddard Space Flight Center/Scientific Visualization Studio)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>When is the eclipse?\u003c/h2>\n\u003cp>The eclipse begins Tuesday morning at 12:02 a.m. PST, when the moon first encounters Earth’s partial, or penumbral, shadow. You may not see much of a change immediately, but over the next hour you can witness a subtle dimming of the full moon’s brightness.\u003c/p>\n\u003cp>The real show begins at 1:09 a.m., when the moon contacts Earth’s full shadow, the \u003ca href=\"https://www.nasa.gov/audience/forstudents/k-4/stories/umbra-and-penumbra\" target=\"_blank\" rel=\"noopener noreferrer\">dark umbra \u003c/a>blocking all sunlight. In the moments after, a prominent darkening will appear at the moon’s edge as the shadow nibbles away at the bright lunar disk. By 1:50 a.m., half of the moon will be consumed.\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>Chabot Space and Science Center is hosting a \u003ca href=\"https://chabotspace.org/calendar/total-lunar-eclipse-2/\">Total Lunar Eclipse Watch Party\u003c/a> from 11:30 p.m. on Monday evening until 4 a.m. Tuesday morning.\u003c/p>\n\u003cfigure id=\"attachment_1980616\" class=\"wp-caption aligncenter\" style=\"max-width: 1920px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980616 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/umbra-penumbra-NASA.jpg\" alt=\"A diagram that shows two grey triangles streaming behind Earth's north and south poles -- that's the Penumbra. And a black triangle, Earth's Umbra, streaming from the equator. \" width=\"1920\" height=\"1080\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA.jpg 1920w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/umbra-penumbra-NASA-1536x864.jpg 1536w\" sizes=\"(max-width: 1920px) 100vw, 1920px\">\u003cfigcaption class=\"wp-caption-text\">Illustration of Earth’s partial (penumbral) and full (umbral) shadows. When the moon passes through Earth’s shadow, we witness a lunar eclipse. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>Totality\u003c/h2>\n\u003cp>The climax of the eclipse, what’s known as “totality,” starts at 2:16 a.m. and will last almost an hour and a half. This is when the moon is fully engulfed in Earth’s dark umbra. The moon will be deepest in shadow and darkest at 2:59 a.m. If you’re only interested in waking for a few moments to catch a glimpse of the eclipse, this is the time to set your alarm for.\u003c/p>\n\u003cp>Totality ends at 3:41 a.m., when the moon begins to emerge from the umbral shadow into the partial sunlight of the penumbra, where only some of the sun’s light is blocked. If you’re a die-hard fan of lunar eclipses, you can stay up until the eclipse officially ends at 5:56 a.m. — but totality is the best part of the show, so when that’s over you can go back to bed and not worry about missing much.\u003c/p>\n\u003ch2>Why doesn’t the moon completely disappear at totality?\u003c/h2>\n\u003cp>During a total lunar eclipse, the moon passes through Earth’s full shadow, the umbra, where no direct sunlight falls, yet it is still lit up in a dull orange or reddish light.\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Sunlight that slips around the edges of the Earth is bent and filtered by our atmosphere, its twilight rays \u003ca href=\"https://earthsky.org/space/when-can-you-see-earths-shadow/\">shining into the dark umbra\u003c/a> like a dim night-light. We see the same rosy glow at dusk every evening as sunlight is scattered over the horizon to illuminate the landscape, even after the sun has set. The same atmospheric glow passes on into space, shedding its radiance into Earth’s shadow. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1980621\" class=\"wp-caption aligncenter\" style=\"max-width: 900px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1980621 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/10/Luneclipse-1-20-2000s.jpg\" alt=\"The white moon partially shadowed in red and white. \" width=\"900\" height=\"599\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s.jpg 900w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-800x532.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-160x106.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/10/Luneclipse-1-20-2000s-768x511.jpg 768w\" sizes=\"(max-width: 900px) 100vw, 900px\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse on Jan. 20, 2000. This photograph was taken during totality; one edge of the moon appears brighter since it was crossing near the edge of Earth’s dark umbral shadow, and not deeply through the center. \u003ccite>(Chabot Space and Science Center/Conrad Jung)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400\">An astronaut standing on the moon and looking back at the Earth during a total lunar eclipse would see a black disk rimmed in a ring of fiery light that includes all the Earth’s sunrises and sunsets in one stunning view.\u003c/span>\u003c/p>\n\u003ch2>How often do lunar eclipses occur?\u003c/h2>\n\u003cp>\u003ca href=\"https://nineplanets.org/total-lunar-eclipse/\">Lunar eclipses occur regularly\u003c/a>, anywhere between two and four times per year. Some are partial eclipses, when the moon only grazes Earth’s umbral shadow. Some are penumbral eclipses, where the moon misses the umbra completely and only passes through Earth’s half-shadow, its light dimming so subtly it might not even be noticed.\u003c/p>\n\u003cp>A total lunar eclipse happens about every two and a half years, on average, and is only visible from half of our planet, and in some locations only partially. So, November’s full, end-to-end eclipse is a very rare treat for people on the West Coast who can enjoy it — and well worth getting up in the middle of the night to witness.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>\u003cem>Benjamin Burress has been a staff astronomer at Chabot Space and Science Center since July 1999.\u003c/em>\u003c/p>\n\n\u003c/div>\u003c/p>",
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"title": "How to See Sunday's 'Blood Moon' Total Lunar Eclipse in the Bay Area",
"headTitle": "How to See Sunday’s ‘Blood Moon’ Total Lunar Eclipse in the Bay Area | KQED",
"content": "\u003cp>\u003cspan style=\"font-weight: 400\">One of the most beautiful sights of the night sky is the appearance of a \u003c/span>\u003ca href=\"https://moon.nasa.gov/moon-in-motion/eclipses/\">\u003cspan style=\"font-weight: 400\">total lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\">, when the moon makes a rare passage straight through Earth’s shadow.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Rare, yes, but on the West Coast, the spheres will align on \u003c/span>\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2022May16T.pdf\">\u003cspan style=\"font-weight: 400\">May 15 \u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\">to give us a front-row seat to the spectacle — and at a convenient time of night, as well.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>When is the eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">When the moon rises, shortly after 8 p.m. PDT on Sunday, the eclipse will already be in progress. But don’t worry about missing the beginning; The best is yet to come.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">The eclipse will enter “\u003c/span>\u003cspan style=\"font-weight: 400\">totality”\u003c/span>\u003cspan style=\"font-weight: 400\"> — when the moon is fully engulfed in Earth’s shadow — at 8:29 p.m., reach maximum darkness at 9:11 p.m., and end at 9:54 p.m. When totality ends, the moon will reenter a partial eclipse phase, gradually moving back into the sun’s light.\u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1979299\" class=\"wp-caption aligncenter\" style=\"max-width: 1041px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1979299\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/lunar-eclipse-diagram_0.jpg\" alt=\"\" width=\"1041\" height=\"783\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0.jpg 1041w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-768x578.jpg 768w\" sizes=\"(max-width: 1041px) 100vw, 1041px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the relationship of the Sun, Earth and moon during a total lunar eclipse, when the moon passes through Earth’s full ‘umbral’ shadow. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>\u003cb>How do you see the eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">The moon will rise in the southeast, and by the time totality begins at 8:29 p.m., it will have risen 12 degrees above the southeastern horizon — about the span of your open hand. So, you simply need to find a moon-watching spot with a clear view of the southeastern horizon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Unlike observing fainter celestial events like meteor showers, you don’t need to travel to a dark sky location to enjoy the eclipse. Even when the moon is dimmest, at maximum eclipse, it will be a prominent object in the heavens.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>What will you see?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">Since \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-may-16\">\u003cspan style=\"font-weight: 400\">this lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> will already be in progress when the moon rises, what would be a full moon will have a large, dark “bite” taken out of one side. Some ancient cultures even explained a lunar eclipse as a celestial being — a dragon, or a dog — devouring the moon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">During totality, the moon will darken significantly, as well as change color from full-moon-white to a rusty orange or even blood red, depending on atmospheric conditions. That’s why a total lunar eclipse is often called a blood moon. The effect can make the moon look three-dimensional, like a coppery ball hanging in the sky — almost like you could reach out and touch it.\u003c/span>\u003c/p>\n\u003cp>The orange and red tones during totality are caused by the filtering of sunlight by Earth’s atmosphere.\u003c/p>\n\u003cfigure id=\"attachment_1979338\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003ca href=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/suns-light-around-Earth.jpg\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1979338\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/suns-light-around-Earth-800x450.jpg\" alt=\"On the left is a blue ball representing Earth. On the top and bottom of Earth, cone-shaped rainbows of light from an unpictured sun extend off into space. the image shows the blue light heading off into space, while the red spectrum of light shines on the moon, hidden in Earth's shadow. \" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth.jpg 987w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003c/a>\u003cfigcaption class=\"wp-caption-text\">During a lunar eclipse, Earth’s atmosphere scatters sunlight. The blue light from the sun scatters away, and longer-wavelength red, orange and yellow light passes through, turning our moon red. This image is not to scale. \u003ccite>(NASA Goddard Space Flight Center/Scientific Visualization Studio)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400\">As the sun’s light grazes around Earth’s edges, it passes through hundreds of miles of atmosphere, and its bluer tones are partially blocked and scattered by atmospheric gas molecules. But redder tones of sunlight pass through more freely, slipping around the sides of our planet and shining onto the moon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">You can \u003c/span>\u003ca href=\"https://www.physicscentral.com/explore/pictures/sunset.cfm\">\u003cspan style=\"font-weight: 400\">see the same effect\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> on the sun’s light every day when you watch a sunrise or sunset, when the sun is near the horizon and filtered to appear orange or red. And even in twilight, when the sun is below the horizon, the sky is still glowing with rosy light scattered in the atmosphere.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>When’s the next eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">Though eclipses, both lunar and solar, are rare events to witness, \u003ca href=\"https://eclipse.gsfc.nasa.gov/LEdecade/LEdecade2021.html\">they occur more often than you might think\u003c/a>. There was a partial solar eclipse on April 30, but you had to be at the southern tip of Chile or in parts of the extreme southern Pacific Ocean to see it. Another partial solar eclipse will be visible from Europe and the Middle East in October.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">But here on the West Coast we’re in luck, for another total lunar eclipse will be visible in 2022, starting around midnight on \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-november-8\">\u003cspan style=\"font-weight: 400\">Nov. 8\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> and reaching maximum eclipse a few hours before sunrise — not as convenient as this month’s, but we’ll be able to see the entire eclipse from beginning to end.\u003c/span>\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>\u003c/p>\n",
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"excerpt": "A total lunar eclipse is called a blood moon for the reddish color the moon turns when it is fully inside Earth's shadow.",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>\u003cspan style=\"font-weight: 400\">One of the most beautiful sights of the night sky is the appearance of a \u003c/span>\u003ca href=\"https://moon.nasa.gov/moon-in-motion/eclipses/\">\u003cspan style=\"font-weight: 400\">total lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\">, when the moon makes a rare passage straight through Earth’s shadow.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Rare, yes, but on the West Coast, the spheres will align on \u003c/span>\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2022May16T.pdf\">\u003cspan style=\"font-weight: 400\">May 15 \u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\">to give us a front-row seat to the spectacle — and at a convenient time of night, as well.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>When is the eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">When the moon rises, shortly after 8 p.m. PDT on Sunday, the eclipse will already be in progress. But don’t worry about missing the beginning; The best is yet to come.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">The eclipse will enter “\u003c/span>\u003cspan style=\"font-weight: 400\">totality”\u003c/span>\u003cspan style=\"font-weight: 400\"> — when the moon is fully engulfed in Earth’s shadow — at 8:29 p.m., reach maximum darkness at 9:11 p.m., and end at 9:54 p.m. When totality ends, the moon will reenter a partial eclipse phase, gradually moving back into the sun’s light.\u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1979299\" class=\"wp-caption aligncenter\" style=\"max-width: 1041px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1979299\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/lunar-eclipse-diagram_0.jpg\" alt=\"\" width=\"1041\" height=\"783\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0.jpg 1041w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/lunar-eclipse-diagram_0-768x578.jpg 768w\" sizes=\"(max-width: 1041px) 100vw, 1041px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the relationship of the Sun, Earth and moon during a total lunar eclipse, when the moon passes through Earth’s full ‘umbral’ shadow. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003ch2>\u003cb>How do you see the eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">The moon will rise in the southeast, and by the time totality begins at 8:29 p.m., it will have risen 12 degrees above the southeastern horizon — about the span of your open hand. So, you simply need to find a moon-watching spot with a clear view of the southeastern horizon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">Unlike observing fainter celestial events like meteor showers, you don’t need to travel to a dark sky location to enjoy the eclipse. Even when the moon is dimmest, at maximum eclipse, it will be a prominent object in the heavens.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>What will you see?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">Since \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-may-16\">\u003cspan style=\"font-weight: 400\">this lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> will already be in progress when the moon rises, what would be a full moon will have a large, dark “bite” taken out of one side. Some ancient cultures even explained a lunar eclipse as a celestial being — a dragon, or a dog — devouring the moon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">During totality, the moon will darken significantly, as well as change color from full-moon-white to a rusty orange or even blood red, depending on atmospheric conditions. That’s why a total lunar eclipse is often called a blood moon. The effect can make the moon look three-dimensional, like a coppery ball hanging in the sky — almost like you could reach out and touch it.\u003c/span>\u003c/p>\n\u003cp>The orange and red tones during totality are caused by the filtering of sunlight by Earth’s atmosphere.\u003c/p>\n\u003cfigure id=\"attachment_1979338\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003ca href=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/suns-light-around-Earth.jpg\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1979338\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2022/05/suns-light-around-Earth-800x450.jpg\" alt=\"On the left is a blue ball representing Earth. On the top and bottom of Earth, cone-shaped rainbows of light from an unpictured sun extend off into space. the image shows the blue light heading off into space, while the red spectrum of light shines on the moon, hidden in Earth's shadow. \" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2022/05/suns-light-around-Earth.jpg 987w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003c/a>\u003cfigcaption class=\"wp-caption-text\">During a lunar eclipse, Earth’s atmosphere scatters sunlight. The blue light from the sun scatters away, and longer-wavelength red, orange and yellow light passes through, turning our moon red. This image is not to scale. \u003ccite>(NASA Goddard Space Flight Center/Scientific Visualization Studio)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400\">As the sun’s light grazes around Earth’s edges, it passes through hundreds of miles of atmosphere, and its bluer tones are partially blocked and scattered by atmospheric gas molecules. But redder tones of sunlight pass through more freely, slipping around the sides of our planet and shining onto the moon.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">You can \u003c/span>\u003ca href=\"https://www.physicscentral.com/explore/pictures/sunset.cfm\">\u003cspan style=\"font-weight: 400\">see the same effect\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> on the sun’s light every day when you watch a sunrise or sunset, when the sun is near the horizon and filtered to appear orange or red. And even in twilight, when the sun is below the horizon, the sky is still glowing with rosy light scattered in the atmosphere.\u003c/span>\u003c/p>\n\u003ch2>\u003cb>When’s the next eclipse?\u003c/b>\u003c/h2>\n\u003cp>\u003cspan style=\"font-weight: 400\">Though eclipses, both lunar and solar, are rare events to witness, \u003ca href=\"https://eclipse.gsfc.nasa.gov/LEdecade/LEdecade2021.html\">they occur more often than you might think\u003c/a>. There was a partial solar eclipse on April 30, but you had to be at the southern tip of Chile or in parts of the extreme southern Pacific Ocean to see it. Another partial solar eclipse will be visible from Europe and the Middle East in October.\u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400\">But here on the West Coast we’re in luck, for another total lunar eclipse will be visible in 2022, starting around midnight on \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/lunar/2022-november-8\">\u003cspan style=\"font-weight: 400\">Nov. 8\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400\"> and reaching maximum eclipse a few hours before sunrise — not as convenient as this month’s, but we’ll be able to see the entire eclipse from beginning to end.\u003c/span>\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"title": "When and Where to Watch the Total Lunar Eclipse Early Wednesday Morning",
"headTitle": "When and Where to Watch the Total Lunar Eclipse Early Wednesday Morning | KQED",
"content": "\u003cp>\u003cspan style=\"font-weight: 400;\">If it feels like a good celestial event has been lacking in your life since last December’s Great Conjunction of Jupiter and Saturn, get ready for a treat. A \u003c/span>\u003ca href=\"https://www.mreclipse.com/Special/LEprimer.html\">\u003cspan style=\"font-weight: 400;\">total lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> is about to grace the night sky, and, weather permitting, you don’t have to travel far from home to enjoy it.\u003c/span>\u003c/p>\n\u003cp>\u003cb>When and Where\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The \u003c/span>\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2021May26T.pdf\">\u003cspan style=\"font-weight: 400;\">eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> takes place on the morning of Wednesday, May 26, beginning at 1:47 a.m. PDT, when the moon makes first contact with Earth’s partial, penumbral shadow. At this time, the full moon will be in the south — you can’t miss it — positioned about 30 degrees above the horizon. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">You may want to sleep through this part of the eclipse, setting your alarm for a bit later, because the penumbral phase offers only a minor dimming of the moon’s light, when you may notice little change.\u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974879\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974879 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/pdt_print-May262021-nasa-800x450.jpg\" alt=\"\" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa.jpg 1024w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the progression of the May 26, 2021, total lunar eclipse. The moon will first enter Earth’s partial, penumbral shadow at 1:47 a.m. PDT, then by 2:44 will contact the full umbral shadow. By 3:20 it will be halfway into the umbra, and between 4:11 and 4:26 will be fully engulfed in it — the total phase of the eclipse. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The real show starts at 2:44 a.m. at the beginning of the eclipse’s partial phase, when the moon begins to enter the Earth’s full shadow, or umbra. Now you will begin to see a definite bite taken out of one edge of the moon. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974877\" class=\"wp-caption alignleft\" style=\"max-width: 174px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974877 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/2007-03-03_-_Lunar_Eclipse_small-43imgThomas-Knoblauch.gif\" alt=\"\" width=\"174\" height=\"144\">\u003cfigcaption class=\"wp-caption-text\">Time lapse animation of a total lunar eclipse, beginning and ending during the partial eclipse phase. \u003ccite>(Thomas Knoblauch)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you’d like to view the eclipse from the comfort of your home, Chabot Space & Science Center will host a \u003c/span>\u003ca href=\"https://chabotspace.org/calendar/lunar-eclipse-party/\">\u003cspan style=\"font-weight: 400;\">live virtual eclipse-viewing event\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> through observatory telescopes. \u003c/span>\u003c/p>\n\u003cp>\u003cb>Totality\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The darkness will grow across the lunar disk until 4:11 a.m., when the eclipse enters “totality” and the moon is fully engulfed in Earth’s deep shadow. The entire face of the moon will dim and may take on a rosy coloration, from rusty brown to deep blood-red. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">At totality, the moon will loom low in the sky, about 15 degrees high, so be sure to pick a viewing spot with a clear view of the southwestern horizon. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">Totality is a breathtaking sight to behold. The once brilliant full moon transforms into a serene coppery sphere, strange and almost looking out of place. Depending on atmospheric conditions, it may even appear like a ball you can reach up and grab. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974878\" class=\"wp-caption alignright\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974878 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-800x602.jpg\" alt=\"\" width=\"800\" height=\"602\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-768x578.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0.jpg 1041w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">A lunar eclipse occurs when the moon passes through Earth’s shadow, either partly (partial lunar eclipse) or completely (total lunar eclipse). \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">For this particular eclipse, totality won’t last long — less than 15 minutes. For some eclipses, totality can last an hour or longer, but Wednesday morning the moon will \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/in/usa/san-francisco\">\u003cspan style=\"font-weight: 400;\">take a shortcut\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> through the Earth’s umbra, and will be fully engulfed in Earth’s shadow from 4:11 to 4:25 a.m. After that, the moon will brighten again at one edge as it peeks back into the sun’s rays. The moon will depart the umbra completely at 5:52 a.m., only minutes before moonset.\u003c/span>\u003c/p>\n\u003cp>\u003cb>Why Does the Moon Turn Red?\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">You might expect that the moon would go completely dark when it enters the Earth’s full umbral shadow. Instead, it seems as if the moon’s “night light” switch is flipped on, so that it becomes a ruddy, glowing fixture in the starry sky. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974880\" class=\"wp-caption alignleft\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974880 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/totallunareclipse-nasa-800x629.jpg\" alt=\"\" width=\"800\" height=\"629\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-800x629.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-160x126.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-768x604.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa.jpg 896w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The moon during the total phase of a lunar eclipse, when the moon is fully covered by Earth’s deep umbral shadow. The red coloration comes from sunlight filtering through Earth’s atmosphere around the edges and being bent into its shadow. The reddening is caused by the same phenomenon that makes a sunset or a sunrise red. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The \u003c/span>\u003ca href=\"https://earthsky.org/space/why-does-the-moon-look-red-during-a-total-lunar-eclipse#:~:text=The%20moon%20passes%20through%20Earth's%20shadow.&text=Bottom%20line%3A%20The%20moon%20can,and%20refracted%20by%20Earth's%20atmosphere.\">\u003cspan style=\"font-weight: 400;\">answer to this puzzle\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> is found in the Earth’s atmosphere. While the Earth itself blocks sunlight from shining directly into the umbral shadow, the atmosphere bends and scatters some of the light slipping around the edges, casting a glow into the shadow. Bluer tones of sunlight are filtered out by atmospheric gases, while redder shades can pass through more freely. The effect is similar to how a piece of red glass lets red light pass through while blocking other colors. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you stood on the moon during this eclipse and looked back at the Earth, you would see the dark disk of the Earth blocking the sun, rimmed with brilliant reddish light, the glow of all the sunrises and sunsets happening on Earth at that moment. \u003c/span>\u003c/p>\n\u003cp>\u003cb>When’s the Next Lunar Eclipse?\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you miss this one, there won’t be another total lunar eclipse visible from the Americas until almost a year from now, on May 16, 2022. So now’s your chance. \u003c/span>\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>\u003c/p>\n",
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"excerpt": "A total lunar eclipse will grace the night sky on Wednesday morning, May 26, starting at 1:47 a.m. PDT. ",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>\u003cspan style=\"font-weight: 400;\">If it feels like a good celestial event has been lacking in your life since last December’s Great Conjunction of Jupiter and Saturn, get ready for a treat. A \u003c/span>\u003ca href=\"https://www.mreclipse.com/Special/LEprimer.html\">\u003cspan style=\"font-weight: 400;\">total lunar eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> is about to grace the night sky, and, weather permitting, you don’t have to travel far from home to enjoy it.\u003c/span>\u003c/p>\n\u003cp>\u003cb>When and Where\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The \u003c/span>\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2021May26T.pdf\">\u003cspan style=\"font-weight: 400;\">eclipse\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> takes place on the morning of Wednesday, May 26, beginning at 1:47 a.m. PDT, when the moon makes first contact with Earth’s partial, penumbral shadow. At this time, the full moon will be in the south — you can’t miss it — positioned about 30 degrees above the horizon. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">You may want to sleep through this part of the eclipse, setting your alarm for a bit later, because the penumbral phase offers only a minor dimming of the moon’s light, when you may notice little change.\u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974879\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974879 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/pdt_print-May262021-nasa-800x450.jpg\" alt=\"\" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-800x450.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-1020x574.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/pdt_print-May262021-nasa.jpg 1024w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the progression of the May 26, 2021, total lunar eclipse. The moon will first enter Earth’s partial, penumbral shadow at 1:47 a.m. PDT, then by 2:44 will contact the full umbral shadow. By 3:20 it will be halfway into the umbra, and between 4:11 and 4:26 will be fully engulfed in it — the total phase of the eclipse. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The real show starts at 2:44 a.m. at the beginning of the eclipse’s partial phase, when the moon begins to enter the Earth’s full shadow, or umbra. Now you will begin to see a definite bite taken out of one edge of the moon. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974877\" class=\"wp-caption alignleft\" style=\"max-width: 174px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974877 size-full\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/2007-03-03_-_Lunar_Eclipse_small-43imgThomas-Knoblauch.gif\" alt=\"\" width=\"174\" height=\"144\">\u003cfigcaption class=\"wp-caption-text\">Time lapse animation of a total lunar eclipse, beginning and ending during the partial eclipse phase. \u003ccite>(Thomas Knoblauch)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you’d like to view the eclipse from the comfort of your home, Chabot Space & Science Center will host a \u003c/span>\u003ca href=\"https://chabotspace.org/calendar/lunar-eclipse-party/\">\u003cspan style=\"font-weight: 400;\">live virtual eclipse-viewing event\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> through observatory telescopes. \u003c/span>\u003c/p>\n\u003cp>\u003cb>Totality\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The darkness will grow across the lunar disk until 4:11 a.m., when the eclipse enters “totality” and the moon is fully engulfed in Earth’s deep shadow. The entire face of the moon will dim and may take on a rosy coloration, from rusty brown to deep blood-red. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">At totality, the moon will loom low in the sky, about 15 degrees high, so be sure to pick a viewing spot with a clear view of the southwestern horizon. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">Totality is a breathtaking sight to behold. The once brilliant full moon transforms into a serene coppery sphere, strange and almost looking out of place. Depending on atmospheric conditions, it may even appear like a ball you can reach up and grab. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974878\" class=\"wp-caption alignright\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974878 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-800x602.jpg\" alt=\"\" width=\"800\" height=\"602\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-800x602.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-1020x767.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-160x120.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0-768x578.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/lunar-eclipse-diagram_0.jpg 1041w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">A lunar eclipse occurs when the moon passes through Earth’s shadow, either partly (partial lunar eclipse) or completely (total lunar eclipse). \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">For this particular eclipse, totality won’t last long — less than 15 minutes. For some eclipses, totality can last an hour or longer, but Wednesday morning the moon will \u003c/span>\u003ca href=\"https://www.timeanddate.com/eclipse/in/usa/san-francisco\">\u003cspan style=\"font-weight: 400;\">take a shortcut\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> through the Earth’s umbra, and will be fully engulfed in Earth’s shadow from 4:11 to 4:25 a.m. After that, the moon will brighten again at one edge as it peeks back into the sun’s rays. The moon will depart the umbra completely at 5:52 a.m., only minutes before moonset.\u003c/span>\u003c/p>\n\u003cp>\u003cb>Why Does the Moon Turn Red?\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">You might expect that the moon would go completely dark when it enters the Earth’s full umbral shadow. Instead, it seems as if the moon’s “night light” switch is flipped on, so that it becomes a ruddy, glowing fixture in the starry sky. \u003c/span>\u003c/p>\n\u003cfigure id=\"attachment_1974880\" class=\"wp-caption alignleft\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"wp-image-1974880 size-medium\" src=\"https://ww2.kqed.org/app/uploads/sites/35/2021/05/totallunareclipse-nasa-800x629.jpg\" alt=\"\" width=\"800\" height=\"629\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-800x629.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-160x126.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa-768x604.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2021/05/totallunareclipse-nasa.jpg 896w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The moon during the total phase of a lunar eclipse, when the moon is fully covered by Earth’s deep umbral shadow. The red coloration comes from sunlight filtering through Earth’s atmosphere around the edges and being bent into its shadow. The reddening is caused by the same phenomenon that makes a sunset or a sunrise red. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>\u003cspan style=\"font-weight: 400;\">The \u003c/span>\u003ca href=\"https://earthsky.org/space/why-does-the-moon-look-red-during-a-total-lunar-eclipse#:~:text=The%20moon%20passes%20through%20Earth's%20shadow.&text=Bottom%20line%3A%20The%20moon%20can,and%20refracted%20by%20Earth's%20atmosphere.\">\u003cspan style=\"font-weight: 400;\">answer to this puzzle\u003c/span>\u003c/a>\u003cspan style=\"font-weight: 400;\"> is found in the Earth’s atmosphere. While the Earth itself blocks sunlight from shining directly into the umbral shadow, the atmosphere bends and scatters some of the light slipping around the edges, casting a glow into the shadow. Bluer tones of sunlight are filtered out by atmospheric gases, while redder shades can pass through more freely. The effect is similar to how a piece of red glass lets red light pass through while blocking other colors. \u003c/span>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you stood on the moon during this eclipse and looked back at the Earth, you would see the dark disk of the Earth blocking the sun, rimmed with brilliant reddish light, the glow of all the sunrises and sunsets happening on Earth at that moment. \u003c/span>\u003c/p>\n\u003cp>\u003cb>When’s the Next Lunar Eclipse?\u003c/b>\u003c/p>\n\u003cp>\u003cspan style=\"font-weight: 400;\">If you miss this one, there won’t be another total lunar eclipse visible from the Americas until almost a year from now, on May 16, 2022. So now’s your chance. \u003c/span>\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"title": "Turn Around, It's a Total Eclipse of the Super Moon",
"headTitle": "Turn Around, It’s a Total Eclipse of the Super Moon | KQED",
"content": "\u003cp>In the evening hours of Sunday, Jan. 20, a \u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2019Jan21T.pdf\">total lunar eclipse\u003c/a> will transform a full moon into a three-hour-plus celestial extravaganza. Not only will we witness the breathtaking beauty of the eclipse, but we’ll watch it during a super moon, when the moon is near its closest approach to Earth and appears larger in our sky than at any other time.\u003c/p>\n\u003caside class=\"pullquote alignright\">Light from all of Earth’s sunrises and sunsets softly illuminate the eclipsed moon, producing a celestial night light in the sky\u003c/aside>\n\u003cp>The best part of the show, when the moon begins to enter Earth’s full shadow (or umbra), begins at 7:33 p.m. and lasts until 10:50 p.m. Pacific Standard Time, when the moon will slip out of the shadow.\u003c/p>\n\u003cp>The moon will be fully engulfed in Earth’s umbra starting at 8:41 p.m. This state of “totality” will last a full hour — so there’s plenty of time to enjoy the show. During totality, the moon will be high and rising higher in the Eastern sky.\u003c/p>\n\u003cfigure id=\"attachment_1936679\" class=\"wp-caption aligncenter\" style=\"max-width: 466px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1936679\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung.jpg\" alt=\"Total Lunar Eclipse that took place exactly 19 years ago, on January 20, 2000. \" width=\"466\" height=\"337\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung.jpg 466w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-160x116.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-240x174.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-375x271.jpg 375w\" sizes=\"(max-width: 466px) 100vw, 466px\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse that took place exactly 19 years ago, on Jan. 20, 2000. \u003ccite>(Conrad Jung)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Chabot Space & Science Center will be hosting a \u003ca href=\"https://chabotspace.org/calendar/total-lunar-eclipse-viewing/\">special eclipse-viewing event\u003c/a> from 6 p.m. to 11:30 p.m., so come on up if you want to make this breathtaking spectacle of nature a memorable social event. (The forecast is for rain showers during the day on Sunday, becoming partly cloudy by evening. Keep your fingers crossed!)\u003c/p>\n\u003cp>\u003cstrong>What You Will See\u003c/strong>\u003c/p>\n\u003cp>A total lunar eclipse is sometimes referred to as a “\u003ca href=\"https://www.timeanddate.com/eclipse/blood-moon.html\">blood moon\u003c/a>” for the reddish hues it acquires during totality. The color can range from coppery to orange to downright red, depending on atmospheric conditions and the moon’s position in the sky.\u003c/p>\n\u003cp>The reddish color is an effect of Earth’s atmosphere, which filters out the bluer tones of sunlight and lets the redder colors pass through unhindered–like red stained-glass. That reddened, filtered sunlight grazing the edge of the Earth passes on and is bent into Earth’s shadow.\u003c/p>\n\u003cp>This filtering of sunlight by the atmosphere is the same effect that makes the sun appear orange or red at sunrise or sunset.\u003c/p>\n\u003cp> \u003c/p>\n\u003cfigure id=\"attachment_1936682\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1936682\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-800x453.jpg\" alt=\"Diagram showing the sun, Earth, and Moon in relation to Earth's shadow and the Moon's orbit. When in the penumbra (Earth's partial shadow), the Moon will be partially illuminated. Within the umbra (Earth's full shadow) no direct sunlight falls on the Moon, but some reddened rays of sunlight refracted and filtered by Earth's atmosphere provides soft illumination.\" width=\"800\" height=\"453\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-160x91.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-768x435.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-240x136.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-375x212.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-520x294.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the sun, Earth, and Moon in relation to Earth’s shadow and the Moon’s orbit. When in the penumbra (Earth’s partial shadow), the Moon will be partially illuminated. Within the umbra (Earth’s full shadow) no direct sunlight falls on the Moon, but some reddened rays of sunlight refracted and filtered by Earth’s atmosphere provides soft illumination. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Without these effects of Earth’s atmosphere, the moon would go almost completely dark upon entering the umbra. Instead, the light from all of Earth’s sunrises and sunsets softly illuminate the eclipsed moon, producing a celestial night light in the sky.\u003c/p>\n\u003cp>You may find that the eclipsed moon looks more like a three-dimensional ball, rather than the flattish disk the full moon usually appears as. This quality is mostly due to the darkened moon not being overwhelmingly bright, as a full moon tends to be. The ruddy coloration may also have something to do with this, accentuating the moon against the otherwise black-and-white night sky.\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>\u003cstrong>Super Moon?\u003c/strong>\u003c/p>\n\u003cp>If the full moon looks larger than usual on Jan. 20, it may not be your imagination.\u003c/p>\n\u003cp>In fact, Sunday’s full moon is a so-called “super moon.” Though it is not an official astronomical term, a super moon is defined as one that takes place when the moon is within 90 percent of its closest approach to Earth (\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2019Jan21T.pdf\">perigee\u003c/a>).\u003c/p>\n\u003cp>On Sunday the moon will reach perigee, 222,000 miles from Earth, only a few hours after the eclipse, so at the time of eclipse it’ll be almost as close as it can get, and 15,000 miles closer than average. This will make the moon physically larger in the sky than average — thus the super moon label.\u003c/p>\n\u003cp>The actual difference in size between a super moon and nonsuper moon isn’t huge, but it is perceptible to the human eye. The problem is that you can’t compare two different full moons at the same time, side by side, unless you take a photograph of each and compare the pics.\u003c/p>\n\u003cfigure id=\"attachment_1936683\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1936683\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/supermoon-800x450.jpg\" alt=\"Side by side comparison of the apparent size of the moon at apogee (left), at average distance (center), and at perigee (right) — the so-called super moon.\" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-240x135.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-375x211.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-520x293.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Side by side comparison of the apparent size of the moon at apogee (left), at average distance (center), and at perigee (right) — the so-called super moon. \u003ccite>(Chabot Space & Science Center)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>If you could compare the full moon at perigee and at apogee (the moon’s greatest distance from Earth), the size difference would be equivalent to that between a nickel and a penny.\u003c/p>\n\u003cp>The greater effect of a super moon is the brightness, which is 30 percent greater than it is from the apogee full moon. That’s like turning up the dimmer switch on a lamp from two-thirds to full.\u003c/p>\n\u003cp>The coincidence of the eclipse and the super moon gives us a rare opportunity to see what happens when nature cranks the full moon’s dimmer switch from maximum to almost off, then back again. And it’ll all happen within a few hours time.\u003c/p>\n\u003cp>Enjoy!\u003c/p>\n\u003cp>\u003c/p>\n",
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"excerpt": "On Sunday night, a total lunar eclipse will transform a full moon into a three-hour-plus celestial extravaganza. ",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>In the evening hours of Sunday, Jan. 20, a \u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2019Jan21T.pdf\">total lunar eclipse\u003c/a> will transform a full moon into a three-hour-plus celestial extravaganza. Not only will we witness the breathtaking beauty of the eclipse, but we’ll watch it during a super moon, when the moon is near its closest approach to Earth and appears larger in our sky than at any other time.\u003c/p>\n\u003caside class=\"pullquote alignright\">Light from all of Earth’s sunrises and sunsets softly illuminate the eclipsed moon, producing a celestial night light in the sky\u003c/aside>\n\u003cp>The best part of the show, when the moon begins to enter Earth’s full shadow (or umbra), begins at 7:33 p.m. and lasts until 10:50 p.m. Pacific Standard Time, when the moon will slip out of the shadow.\u003c/p>\n\u003cp>The moon will be fully engulfed in Earth’s umbra starting at 8:41 p.m. This state of “totality” will last a full hour — so there’s plenty of time to enjoy the show. During totality, the moon will be high and rising higher in the Eastern sky.\u003c/p>\n\u003cfigure id=\"attachment_1936679\" class=\"wp-caption aligncenter\" style=\"max-width: 466px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-1936679\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung.jpg\" alt=\"Total Lunar Eclipse that took place exactly 19 years ago, on January 20, 2000. \" width=\"466\" height=\"337\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung.jpg 466w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-160x116.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-240x174.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/jan202000_eclipse_cjung-375x271.jpg 375w\" sizes=\"(max-width: 466px) 100vw, 466px\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse that took place exactly 19 years ago, on Jan. 20, 2000. \u003ccite>(Conrad Jung)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Chabot Space & Science Center will be hosting a \u003ca href=\"https://chabotspace.org/calendar/total-lunar-eclipse-viewing/\">special eclipse-viewing event\u003c/a> from 6 p.m. to 11:30 p.m., so come on up if you want to make this breathtaking spectacle of nature a memorable social event. (The forecast is for rain showers during the day on Sunday, becoming partly cloudy by evening. Keep your fingers crossed!)\u003c/p>\n\u003cp>\u003cstrong>What You Will See\u003c/strong>\u003c/p>\n\u003cp>A total lunar eclipse is sometimes referred to as a “\u003ca href=\"https://www.timeanddate.com/eclipse/blood-moon.html\">blood moon\u003c/a>” for the reddish hues it acquires during totality. The color can range from coppery to orange to downright red, depending on atmospheric conditions and the moon’s position in the sky.\u003c/p>\n\u003cp>The reddish color is an effect of Earth’s atmosphere, which filters out the bluer tones of sunlight and lets the redder colors pass through unhindered–like red stained-glass. That reddened, filtered sunlight grazing the edge of the Earth passes on and is bent into Earth’s shadow.\u003c/p>\n\u003cp>This filtering of sunlight by the atmosphere is the same effect that makes the sun appear orange or red at sunrise or sunset.\u003c/p>\n\u003cp> \u003c/p>\n\u003cfigure id=\"attachment_1936682\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1936682\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-800x453.jpg\" alt=\"Diagram showing the sun, Earth, and Moon in relation to Earth's shadow and the Moon's orbit. When in the penumbra (Earth's partial shadow), the Moon will be partially illuminated. Within the umbra (Earth's full shadow) no direct sunlight falls on the Moon, but some reddened rays of sunlight refracted and filtered by Earth's atmosphere provides soft illumination.\" width=\"800\" height=\"453\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-160x91.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-768x435.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-240x136.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-375x212.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/lunareclipsediagram_nasa-520x294.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Diagram showing the sun, Earth, and Moon in relation to Earth’s shadow and the Moon’s orbit. When in the penumbra (Earth’s partial shadow), the Moon will be partially illuminated. Within the umbra (Earth’s full shadow) no direct sunlight falls on the Moon, but some reddened rays of sunlight refracted and filtered by Earth’s atmosphere provides soft illumination. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Without these effects of Earth’s atmosphere, the moon would go almost completely dark upon entering the umbra. Instead, the light from all of Earth’s sunrises and sunsets softly illuminate the eclipsed moon, producing a celestial night light in the sky.\u003c/p>\n\u003cp>You may find that the eclipsed moon looks more like a three-dimensional ball, rather than the flattish disk the full moon usually appears as. This quality is mostly due to the darkened moon not being overwhelmingly bright, as a full moon tends to be. The ruddy coloration may also have something to do with this, accentuating the moon against the otherwise black-and-white night sky.\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>\u003cstrong>Super Moon?\u003c/strong>\u003c/p>\n\u003cp>If the full moon looks larger than usual on Jan. 20, it may not be your imagination.\u003c/p>\n\u003cp>In fact, Sunday’s full moon is a so-called “super moon.” Though it is not an official astronomical term, a super moon is defined as one that takes place when the moon is within 90 percent of its closest approach to Earth (\u003ca href=\"https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2019Jan21T.pdf\">perigee\u003c/a>).\u003c/p>\n\u003cp>On Sunday the moon will reach perigee, 222,000 miles from Earth, only a few hours after the eclipse, so at the time of eclipse it’ll be almost as close as it can get, and 15,000 miles closer than average. This will make the moon physically larger in the sky than average — thus the super moon label.\u003c/p>\n\u003cp>The actual difference in size between a super moon and nonsuper moon isn’t huge, but it is perceptible to the human eye. The problem is that you can’t compare two different full moons at the same time, side by side, unless you take a photograph of each and compare the pics.\u003c/p>\n\u003cfigure id=\"attachment_1936683\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1936683\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2019/01/supermoon-800x450.jpg\" alt=\"Side by side comparison of the apparent size of the moon at apogee (left), at average distance (center), and at perigee (right) — the so-called super moon.\" width=\"800\" height=\"450\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-160x90.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-768x432.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-240x135.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-375x211.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2019/01/supermoon-520x293.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">Side by side comparison of the apparent size of the moon at apogee (left), at average distance (center), and at perigee (right) — the so-called super moon. \u003ccite>(Chabot Space & Science Center)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>If you could compare the full moon at perigee and at apogee (the moon’s greatest distance from Earth), the size difference would be equivalent to that between a nickel and a penny.\u003c/p>\n\u003cp>The greater effect of a super moon is the brightness, which is 30 percent greater than it is from the apogee full moon. That’s like turning up the dimmer switch on a lamp from two-thirds to full.\u003c/p>\n\u003cp>The coincidence of the eclipse and the super moon gives us a rare opportunity to see what happens when nature cranks the full moon’s dimmer switch from maximum to almost off, then back again. And it’ll all happen within a few hours time.\u003c/p>\n\u003cp>Enjoy!\u003c/p>\n\u003cp>\u003c/p>\n\u003c/div>\u003c/p>",
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"title": "Blood Moon: A Chance to Watch a Total Lunar Eclipse",
"headTitle": "Blood Moon: A Chance to Watch a Total Lunar Eclipse | KQED",
"content": "\u003cfigure id=\"attachment_16212\" class=\"wp-caption aligncenter\" style=\"max-width: 640px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-16212\" src=\"http://ww2.kqed.org/science/wp-content/uploads/sites/35/2014/04/Lunar-Eclipse-08-28-07-composite-8bt-small.jpg\" alt=\"Total lunar eclipse August, 28th, 2007. Credit: Conrad Jung\" width=\"640\" height=\"360\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse on August 28th, 2007. (Conrad Jung/Chabot Space and Science Center)\u003c/figcaption>\u003c/figure>\n\u003cp>Bay Area residents will be able to watch one of the moon’s most remarkable displays \u003ca href=\"http://www.timeanddate.com/eclipse/lunar/2014-april-15\" target=\"_blank\" rel=\"noopener\">late on the night of April 14 and early, early on the morning of April 15\u003c/a> when the shadow of Earth crosses the moon in a total lunar eclipse. A cosmic dance between Earth, sun and moon, this total lunar eclipse will be the first in three years to be visible here, weather permitting.\u003c/p>\n\u003cp>\u003cstrong>What Is a Total Lunar Eclipse?\u003c/strong>\u003c/p>\n\u003caside class=\"alignright\">\n\u003cul>\n\u003cli>\u003cstrong>When to watch:\u003c/strong> The eclipse starts at 10:58 p.m. PST. At 12:07 a.m. the total eclipse phase begins. Earth will block the sun completely until 1:25 a.m., and then the moon travels through the semi-shadow until 2:33 a.m.\u003c/li>\n\u003cli>\u003cstrong>Where to watch:\u003c/strong> Just go outside. You can see the eclipse from wherever you can usually see the moon.\u003c/li>\n\u003c/ul>\n\u003c/aside>\n\u003cp> During a total lunar eclipse, Earth passes exactly between the full moon and the sun. As the celestial bodies move, the full moon enters Earth’s shadow until it is completely covered.\u003c/p>\n\u003cp>You may wonder, since the moon is constantly orbiting around the Earth, why there isn’t a lunar eclipse every month.\u003c/p>\n\u003cp>“It turns out the orbit of the moon is tilted relative to the orbit of the Earth around the sun so it doesn’t happen regularly,” says Andrew Fraknoi, Astronomy Department Chair at Foothill College. “Only when the two orbits cross—the orbit of the moon around the Earth and the orbit of the Earth around the sun—can you have an eclipse.”\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>For a visualization of what will be happening in space, check out this animated video from NASA, explaining the movements of celestial bodies during the total lunar eclipse on June 15, 2011.\u003c/p>\n\u003cp>http://www.youtube.com/watch?v=wuhNZejHeBg\u003c/p>\n\u003cp>\u003cstrong>Where and When Can I Watch It?\u003c/strong>\u003c/p>\n\u003cp>Late on the night of April 14, the moon will have risen far above the horizon line when it enters Earth’s shadow, so the timing of this eclipse will make it remarkably accessible.\u003c/p>\n\u003cp>“If it’s clear Monday evening and Tuesday morning,” Fraknoi says, “there should be a spectacular eclipse, pretty high in the sky so that anyone with a good view of the sky can see it.”\u003c/p>\n\u003cp>If you’d like to join a large watching party, you can grab at ticket for the viewing event at the \u003ca href=\"http://www.chabotspace.org/calendar.htm?date=4-14-2014&p=1439355\">Chabot Space and Science Center\u003c/a> or perhaps gather with neighbors on a hill near your home.\u003c/p>\n\u003cp>In the Bay Area, the eclipse will start at 10:58 p.m., when the moon enters the penumbra of Earth, or the semi-shadow. Then at 12:07 a.m., the moon enters Earth’s umbra, directly in line with the sun, and the total eclipse phase begins. Earth will block the sun completely until 1:25 a.m., and then the moon travels through the semi-shadow until 2:33 a.m., when it finally emerges again to reflect the sun’s light. The whole event will last 3 hours and 35 minutes.\u003c/p>\n\u003cp>\u003cstrong>The Blood Moon Effect\u003c/strong>\u003c/p>\n\u003cp>The moon during a total lunar eclipse is also called a “blood moon” because, rather than turning dark when Earth’s shadow passes over it, the moon turns a rusty red or brown.\u003c/p>\n\u003cp>That color comes from the rays of sunlight peeking around the edges of Earth, through its atmosphere. Colors with a shorter wavelength, like the blues, scatter as they hit Earth’s atmosphere, whereas colors with longer wavelengths like red, bend and reach the moon, casting a reddish glow across its surface.\u003c/p>\n\u003cp>A rich color also tells us there are a lot of particles thickening the atmosphere. “The more sooty the atmosphere,” Fraknoi says, “the better this reddening effect.”\u003c/p>\n\u003cp>\u003cstrong>Coming Up\u003c/strong>\u003c/p>\n\u003cp>There’s actually an eclipse season roughly every six months when it’s possible to see either a solar or a lunar eclipse. This total lunar eclipse is the first of four in a row, what astronomers call a tetrad. The other three total lunar eclipses will occur on October 8th, 2014, April 4th, 2015, and September 28th, 2015, and all will be visible in the Bay Area.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>Get your fill because after that, the next total lunar eclipse won’t occur until 2018, and we won’t see another tetrad until 2032-33.\u003c/p>\n\n",
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"excerpt": "It'll be a great view in the Bay Area late on the night of April 14, as long as clouds don't cover up the moon.",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cfigure id=\"attachment_16212\" class=\"wp-caption aligncenter\" style=\"max-width: 640px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-16212\" src=\"http://ww2.kqed.org/science/wp-content/uploads/sites/35/2014/04/Lunar-Eclipse-08-28-07-composite-8bt-small.jpg\" alt=\"Total lunar eclipse August, 28th, 2007. Credit: Conrad Jung\" width=\"640\" height=\"360\">\u003cfigcaption class=\"wp-caption-text\">Total lunar eclipse on August 28th, 2007. (Conrad Jung/Chabot Space and Science Center)\u003c/figcaption>\u003c/figure>\n\u003cp>Bay Area residents will be able to watch one of the moon’s most remarkable displays \u003ca href=\"http://www.timeanddate.com/eclipse/lunar/2014-april-15\" target=\"_blank\" rel=\"noopener\">late on the night of April 14 and early, early on the morning of April 15\u003c/a> when the shadow of Earth crosses the moon in a total lunar eclipse. A cosmic dance between Earth, sun and moon, this total lunar eclipse will be the first in three years to be visible here, weather permitting.\u003c/p>\n\u003cp>\u003cstrong>What Is a Total Lunar Eclipse?\u003c/strong>\u003c/p>\n\u003caside class=\"alignright\">\n\u003cul>\n\u003cli>\u003cstrong>When to watch:\u003c/strong> The eclipse starts at 10:58 p.m. PST. At 12:07 a.m. the total eclipse phase begins. Earth will block the sun completely until 1:25 a.m., and then the moon travels through the semi-shadow until 2:33 a.m.\u003c/li>\n\u003cli>\u003cstrong>Where to watch:\u003c/strong> Just go outside. You can see the eclipse from wherever you can usually see the moon.\u003c/li>\n\u003c/ul>\n\u003c/aside>\n\u003cp> During a total lunar eclipse, Earth passes exactly between the full moon and the sun. As the celestial bodies move, the full moon enters Earth’s shadow until it is completely covered.\u003c/p>\n\u003cp>You may wonder, since the moon is constantly orbiting around the Earth, why there isn’t a lunar eclipse every month.\u003c/p>\n\u003cp>“It turns out the orbit of the moon is tilted relative to the orbit of the Earth around the sun so it doesn’t happen regularly,” says Andrew Fraknoi, Astronomy Department Chair at Foothill College. “Only when the two orbits cross—the orbit of the moon around the Earth and the orbit of the Earth around the sun—can you have an eclipse.”\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>For a visualization of what will be happening in space, check out this animated video from NASA, explaining the movements of celestial bodies during the total lunar eclipse on June 15, 2011.\u003c/p>\u003c/p>\u003cp>\u003cspan class='utils-parseShortcode-shortcodes-__youtubeShortcode__embedYoutube'>\n \u003cspan class='utils-parseShortcode-shortcodes-__youtubeShortcode__embedYoutubeInside'>\n \u003ciframe\n loading='lazy'\n class='utils-parseShortcode-shortcodes-__youtubeShortcode__youtubePlayer'\n type='text/html'\n src='//www.youtube.com/embed/wuhNZejHeBg'\n title='//www.youtube.com/embed/wuhNZejHeBg'\n allowfullscreen='true'\n style='border:0;'>\u003c/iframe>\n \u003c/span>\n \u003c/span>\u003c/p>\u003cp>\u003cp>\u003cstrong>Where and When Can I Watch It?\u003c/strong>\u003c/p>\n\u003cp>Late on the night of April 14, the moon will have risen far above the horizon line when it enters Earth’s shadow, so the timing of this eclipse will make it remarkably accessible.\u003c/p>\n\u003cp>“If it’s clear Monday evening and Tuesday morning,” Fraknoi says, “there should be a spectacular eclipse, pretty high in the sky so that anyone with a good view of the sky can see it.”\u003c/p>\n\u003cp>If you’d like to join a large watching party, you can grab at ticket for the viewing event at the \u003ca href=\"http://www.chabotspace.org/calendar.htm?date=4-14-2014&p=1439355\">Chabot Space and Science Center\u003c/a> or perhaps gather with neighbors on a hill near your home.\u003c/p>\n\u003cp>In the Bay Area, the eclipse will start at 10:58 p.m., when the moon enters the penumbra of Earth, or the semi-shadow. Then at 12:07 a.m., the moon enters Earth’s umbra, directly in line with the sun, and the total eclipse phase begins. Earth will block the sun completely until 1:25 a.m., and then the moon travels through the semi-shadow until 2:33 a.m., when it finally emerges again to reflect the sun’s light. The whole event will last 3 hours and 35 minutes.\u003c/p>\n\u003cp>\u003cstrong>The Blood Moon Effect\u003c/strong>\u003c/p>\n\u003cp>The moon during a total lunar eclipse is also called a “blood moon” because, rather than turning dark when Earth’s shadow passes over it, the moon turns a rusty red or brown.\u003c/p>\n\u003cp>That color comes from the rays of sunlight peeking around the edges of Earth, through its atmosphere. Colors with a shorter wavelength, like the blues, scatter as they hit Earth’s atmosphere, whereas colors with longer wavelengths like red, bend and reach the moon, casting a reddish glow across its surface.\u003c/p>\n\u003cp>A rich color also tells us there are a lot of particles thickening the atmosphere. “The more sooty the atmosphere,” Fraknoi says, “the better this reddening effect.”\u003c/p>\n\u003cp>\u003cstrong>Coming Up\u003c/strong>\u003c/p>\n\u003cp>There’s actually an eclipse season roughly every six months when it’s possible to see either a solar or a lunar eclipse. This total lunar eclipse is the first of four in a row, what astronomers call a tetrad. The other three total lunar eclipses will occur on October 8th, 2014, April 4th, 2015, and September 28th, 2015, and all will be visible in the Bay Area.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>Get your fill because after that, the next total lunar eclipse won’t occur until 2018, and we won’t see another tetrad until 2032-33.\u003c/p>\n\n\u003c/div>\u003c/p>",
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