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DTSTART;TZID=Europe/Madrid:20260827T230000
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DTSTAMP:20260529T213635
CREATED:20260412T165616Z
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UID:1998-1787871600-1787889600@astrofarm.one
SUMMARY:Lunar Eclipse
DESCRIPTION:Partial Lunar Eclipse 2026 — When the Moon Slips Into Shadow\n\nUnlike a solar eclipse\, a lunar eclipse does not interrupt the day.\n\nIt doesn’t arrive suddenly. It doesn’t darken the sky or force you to stop what you’re doing and look up. Instead\, it unfolds slowly — so slowly that\, if you are not paying attention\, you might not notice it at all.\n\nOn the night of August 27 to 28\, 2026\, the Moon will pass through Earth’s shadow.\n\nNot completely.\n\nBut deeply enough that something changes.\n\nAt first\, the Moon looks the same as always — bright\, familiar\, almost static against the background of stars. But as the eclipse begins\, a subtle darkening appears along one edge. It is not sharp. Not dramatic. It is gradual.\n\nThe shadow grows.\n\nAnd as it does\, the Moon begins to lose its brightness.\n\nThis is what defines a lunar eclipse: not a sudden disappearance\, but a slow transformation.\n\nThe Earth\, positioned directly between the Sun and the Moon\, casts a shadow into space. That shadow extends far beyond the planet itself\, forming two distinct regions — the penumbra\, where sunlight is only partially blocked\, and the umbra\, where the Sun is completely obscured.\n\nDuring this eclipse\, the Moon will move almost entirely into the umbra — about 96 percent of its surface will be covered.\n\nAnd that is where things become interesting.\n\nBecause even inside Earth’s shadow\, the Moon does not disappear.\n\nIt changes color.\n\nThe familiar bright white fades\, replaced by a deep\, muted red.\n\nThis is not because the Moon is glowing on its own.\n\nIt is because of Earth.\n\nAs sunlight passes through Earth’s atmosphere\, shorter wavelengths — blues and violets — are scattered in all directions. This is the same process that makes the sky appear blue during the day.\n\nThe remaining light\, dominated by reds and oranges\, is bent and filtered through the atmosphere and projected into Earth’s shadow.\n\nAnd that light reaches the Moon.\n\nWhat you see is not the absence of light.\n\nIt is the presence of filtered light.\n\nA reflection of all the sunrises and sunsets happening around the edge of the Earth at that moment.\n\nThis is why lunar eclipses are sometimes called “blood moons.”\n\nBut the name doesn’t quite capture the experience.\n\nBecause the change is slow.\n\nYou watch the shadow move. You watch the color shift. You watch something familiar become unfamiliar\, not instantly\, but over time.\n\nAnd that changes how you experience it.\n\nUnlike a solar eclipse\, which demands your attention\, a lunar eclipse invites it.\n\nYou can look away. You can come back. And each time you return\, something has changed.\n\nThe peak of this eclipse occurs in the early hours of the morning\, when the Moon is high in the sky and the shadow has reached its maximum extent.\n\nAt that point\, the Moon appears darker\, softer\, almost detached from its usual presence.\n\nAnd then\, slowly\, it begins to return.\n\nThe shadow recedes. The brightness comes back. The familiar shape reasserts itself.\n\nAnd the sky returns to normal.\n\nBut something about the experience lingers.\n\nBecause you have watched a process unfold in real time.\n\nYou have seen the geometry of Earth\, Sun\, and Moon align in a way that reveals something usually hidden.\n\nNot through sudden change.\n\nBut through gradual transformation.\n\nAnd in that slow movement\, something becomes clear.\n\nEven the most stable objects in the sky are not fixed.\n\nThey are always changing.\n\nSometimes\, we just need to wait long enough to see it.\n\n\n\nSources\n\nNASA Eclipse Page – https://eclipse.gsfc.nasa.gov\n\nEuropean Space Agency – https://www.esa.int/Science_Exploration\n\nInternational Astronomical Union – https://www.iau.org
URL:https://astrofarm.one/event/lunar-eclipse/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Lunar-Eclipse.png
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