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DTSTART;TZID=Europe/Madrid:20261124T230000
DTEND;TZID=Europe/Madrid:20261125T150000
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CREATED:20260416T172315Z
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UID:2038-1795561200-1795618800@astrofarm.one
SUMMARY:The Supermoon Debate Is Back
DESCRIPTION:The Supermoon Debate Is Back — Here's Whether The November 24 Moon Is Actually Bigger Or If Everyone Is Just Being Dramatic\n\nSpoiler: It's both. And neither. Let us explain.\n\nEvery time it happens\, the same fight starts:\n\n"Is the Moon actually bigger tonight?"\n\n"Or does it just look bigger?"\n\n"Or is this just one of those things people overhype every year?"\n\nThe answer is: yes. And no. And also... kind of.\n\nOn November 24\, 2026\, the full Moon reaches what's commonly called a "supermoon" — the closest full Moon of the year. And before you roll your eyes\, let's actually break down what's real and what's your brain being dramatic.\n\nFirst: The Illusion That Tricks Everyone\n\nMost of the time\, when people say the Moon looks HUGE\, they're not talking about a supermoon at all.\n\nThey're talking about the "Moon illusion."\n\nThat's the effect where the Moon looks massive when it's near the horizon\, especially next to buildings\, trees\, or mountains. It's your brain being weird about scale and distance.\n\nThat's not physical. That's perception.\n\nSo when people hear "supermoon\," they assume it's just more of that. Another overhyped internet thing.\n\nBut it isn't.\n\nThe Actual Science (Which Is Real)\n\nA supermoon is a real phenomenon. Here's how it works:\n\nThe Moon's orbit around Earth isn't a perfect circle — it's slightly elliptical. That means there are points where it's closer (perigee) and points where it's farther (apogee).\n\nWhen a full Moon happens near perigee = supermoon.\n\nThe 2026 supermoon is the closest full Moon of the year.\n\nSo yes\, it IS bigger:\n\nAbout 7% larger than an average full Moon.\n\nAbout 14% larger than the smallest full Moon (a "micromoon").\n\nThose numbers are measurable\, verifiable\, real.\n\nHere's The Catch (There's Always A Catch)\n\nYour eyes aren't great at detecting a 7% difference.\n\nIf you see the Moon on two different nights without direct comparison\, you probably won't notice anything dramatic. Which is why people argue about it. The physical change is subtle.\n\nBUT.\n\nIf you catch the Moon rising\, low on the horizon\, during this supermoon\, BOTH effects combine:\n\nThe real size increase + the Moon illusion = MASSIVE.\n\nThat's when the Moon looks almost too big for the sky. Dominant. Unreal. The kind of Moon that makes you stop walking and just stare.\n\nThe Real Effect Isn't Size — It's Attention\n\nHere's the thing about the Moon: You've seen it your entire life. It's the most familiar object in the sky.\n\nSo when it suddenly feels different — even slightly — it stands out immediately. It feels wrong. Or at least unusual.\n\nAnd that's what makes the supermoon powerful.\n\nNot because it's dramatically larger. But because it's just different enough to break your expectations.\n\nAnd once that happens\, you start paying attention again. To something you normally ignore.\n\nThat's the real effect. Not size. Attention.\n\nNovember 24\, 2026. Catch it at moonrise. Let both effects hit you at once.\n\nSources\n\nNASA Moon Phases & Supermoon — https://science.nasa.gov/moon\n\nEuropean Space Agency — https://www.esa.int/Science_Exploration\n\nRoyal Museums Greenwich — https://www.rmg.co.uk/stories/topics/supermoon
URL:https://astrofarm.one/event/the-supermoon-debate-is-back/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Supermoon-November.png
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BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261125T230000
DTEND;TZID=Europe/Madrid:20261126T033000
DTSTAMP:20260530T042915
CREATED:20260416T172536Z
LAST-MODIFIED:20260523T101905Z
UID:2041-1795647600-1795663800@astrofarm.one
SUMMARY:See Uranus with your own eyes
DESCRIPTION:You Can Technically See Uranus With Your Naked Eyes — And Almost Nobody Ever Does\n\nNovember 25\, 2026 is your best chance to spot a planet that's 2.9 billion kilometers away. Without a telescope. Yes\, really.\n\nHere's a strange fact:\n\nYou might be able to see Uranus with your own eyes.\n\nNo telescope. No camera. No apps. Just you\, your eyeballs\, and 2.9 billion kilometers of empty space.\n\nAnd yet\, almost nobody ever does.\n\nOn November 25\, 2026\, Uranus reaches opposition — the point where it's closest to Earth\, fully illuminated\, and visible all night.\n\nThis is literally the best it gets.\n\nAnd still... most people won't see it.\n\nThe Problem: Uranus Doesn't Want To Be Found\n\nAt around magnitude 5.6\, Uranus is technically bright enough to be seen under very dark skies.\n\nBut "technically visible" and "actually noticeable" are two VERY different things.\n\nUranus doesn't stand out. It doesn't sparkle. It doesn't demand attention. It just... sits there. A tiny\, faint point\, almost indistinguishable from the surrounding stars.\n\nThis is the challenge.\n\nTo see Uranus\, you need more than just eyesight. You need intention. You need to know exactly where to look. And you need to trust that what you're seeing is actually it.\n\nJupiter Finds You. Uranus Makes You Work For It.\n\nPlanets like Jupiter and Venus are attention seekers. They're bright. They're obvious. You spot them without trying.\n\nUranus doesn't do that.\n\nYou have to go find it. And when you do\, the experience feels completely different.\n\nBecause suddenly\, you're not just looking at the sky. You're SEARCHING it. You're comparing star brightness. You're noticing patterns. You're paying attention to details you would normally ignore.\n\nAnd then\, eventually\, you see it.\n\nOr at least\, you THINK you do.\n\nThat moment — that uncertainty — is part of the experience.\n\nUranus doesn't confirm your observation. It doesn't announce itself. It just exists. Quietly. 2.9 billion kilometers away.\n\nWhat You're Actually Looking At\n\nA cold\, distant world\, tilted almost completely on its side — 98 degrees\, basically rolling around the Sun like a barrel. It rotates in a way that makes it unlike any other planet in the solar system.\n\nIt has 27 known moons\, named after characters from Shakespeare and Alexander Pope.\n\nIts atmosphere is made of hydrogen\, helium\, and methane — which gives it that faint blue-green color you'd see in photos.\n\nNone of that is visible to your eyes.\n\nWhat you see is a point. But what you understand is something much bigger.\n\nYou've crossed a threshold. You've gone from passively looking at the sky to actively engaging with it.\n\nAnd that's rare. Because most of the time\, we only notice what's easy.\n\nUranus isn't. And that's exactly why it matters.\n\nSources\n\nNASA Solar System Exploration — https://solarsystem.nasa.gov\n\nEuropean Southern Observatory — https://www.eso.org/public/science/\n\nESA Science — https://www.esa.int/Science_Exploration
URL:https://astrofarm.one/event/see-uranus-with-your-own-eyes/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Uranus.png
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BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261129T230000
DTEND;TZID=Europe/Madrid:20261130T033000
DTSTAMP:20260530T042915
CREATED:20260416T173043Z
LAST-MODIFIED:20260523T102015Z
UID:2045-1795993200-1796009400@astrofarm.one
SUMMARY:The brightest Venus
DESCRIPTION:Venus Is About To Be So Ridiculously Bright That People Will Think It's A UFO (Again)\n\nNovember 29\, 2026: The morning star hits -4.7 magnitude and refuses to act like a normal celestial object.\n\nAt some point\, you'll notice it.\n\nNot because you were looking for it. But because it doesn't belong.\n\nA light in the early morning sky that feels too bright\, too stable\, too CLEAN to be a star.\n\nThat's Venus. And she's about to peak.\n\nAround November 29\, 2026\, Venus reaches maximum brightness as a morning star — shining at about -4.7 magnitude. In non-astronomer terms: it's one of the brightest objects in the sky after the Sun and Moon.\n\nAnd people are absolutely going to call the police about it.\n\nWhy Venus Hits Different Than Everything Else In The Sky\n\nVenus doesn't twinkle like stars.\n\nThat's not an aesthetic choice — it's physics. Stars appear to flicker because their light travels immense distances and gets distorted by Earth's atmosphere.\n\nVenus is much closer. Its light is more stable. Less affected by atmospheric turbulence.\n\nSo instead of flickering\, it just... holds its brightness. Steady. Almost artificial.\n\nAnd THAT is why people constantly mistake it for planes\, drones\, helicopters\, government experiments\, and (yes) alien spacecraft.\n\nThe Science Behind The Glow\n\nWhy is Venus THIS bright? Geometry + clouds.\n\nVenus orbits the Sun closer than Earth\, so we see it in phases — like a mini Moon. At maximum brightness\, it's not fully illuminated. It's actually a crescent. But a LARGE crescent\, because it's relatively close to Earth at that moment.\n\nCombine that with Venus's thick cloud layers — composed primarily of sulfuric acid droplets — which give it an extremely high albedo (reflectivity). Venus reflects a huge percentage of the sunlight that hits it.\n\nProximity + phase + ridiculously reflective clouds = a planet that outshines almost everything.\n\nThe Part That's Going To Mess With Your Head\n\nThe morning sky is supposed to be fading. Darkness giving way to light. Objects disappearing as the Sun rises.\n\nVenus doesn't play by those rules.\n\nIt remains visible even as the sky brightens. For a while\, it just... stays there. Refusing to fade. A bright point in a sky that's no longer fully dark but not yet day.\n\nThat liminal quality — existing in the boundary between night and day — is what makes Venus feel slightly out of place.\n\nEven when you know exactly what it is.\n\nNovember 29\, 2026. Look east before sunrise. Watch the morning star do its thing.\n\nSources\n\nNASA Solar System Exploration — https://solarsystem.nasa.gov/planets/venus/overview/\n\nEuropean Space Agency — https://www.esa.int/Science_Exploration/Space_Science/Venus_Express\n\nPeer-reviewed: Mallama et al. (2006)\, 'Venus phase function and forward scattering'\, Icarus Journal
URL:https://astrofarm.one/event/the-brightest-venus-2/
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BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261213T230000
DTEND;TZID=Europe/Madrid:20261215T030000
DTSTAMP:20260530T042915
CREATED:20260416T173314Z
LAST-MODIFIED:20260523T102126Z
UID:2047-1797202800-1797303600@astrofarm.one
SUMMARY:The Geminids
DESCRIPTION:Forget The Perseids — The Geminids Are Actually The Best Meteor Shower And 2026 Conditions Are Perfect\n\n100+ meteors per hour. No Moon interference. December 13-14. This is the one.\n\nIf you've only watched one meteor shower in your life\, there's a good chance it wasn't the best one.\n\nBecause despite the hype around the Perseids\, the Geminids are actually the most intense meteor shower of the year.\n\nAnd in 2026\, they show up under near-perfect conditions.\n\nNo bright Moon. Peak activity around December 13-14. And the potential for OVER 100 METEORS PER HOUR under dark skies.\n\nThat's not marketing. That's physics.\n\nThe Origin Story Is Absolutely Wild\n\nMost meteor showers come from comets — icy bodies that shed dust as they approach the Sun.\n\nThe Geminids don't.\n\nThey come from an object called 3200 Phaethon. And Phaethon is weird.\n\nIt behaves like an asteroid. Rocky. Dense. No classic comet tail. And yet\, it produces one of the most active meteor streams in the solar system.\n\nScientists classify it as a "rock comet" — an object that releases material not through ice sublimation\, but through THERMAL FRACTURING. As it approaches the Sun\, its surface heats up to extreme temperatures\, causing rock to crack and eject particles into space.\n\nSo you're watching pieces of a cracking asteroid burn up in our atmosphere. That's metal.\n\nWhy These Meteors Look Different\n\nGeminid meteors enter the atmosphere at about 35 km/s — slower than many other showers (like the Leonids at 71 km/s).\n\nThat lower speed changes how they appear:\n\nBright\, often colorful streaks. More visible. More trackable. More noticeable.\n\nThe sky doesn't just have occasional flashes. It becomes a continuous sequence of events.\n\nAnd in 2026\, with minimal moonlight\, the contrast is STRONG.\n\nThe Best Part: You Don't Have To Destroy Your Sleep Schedule\n\nUnlike many meteor showers that peak just before dawn (because nature hates us)\, the Geminid radiant rises earlier in the evening.\n\nWhich means you can start observing BEFORE midnight.\n\nNo 3 AM alarm. No existential crisis about whether staying up is worth it. No falling asleep on a blanket in the cold.\n\nJust go outside around 10 PM\, look up\, and watch the sky do its thing.\n\nThat accessibility turns a "rare astronomical event" into something almost anyone can experience.\n\nAnd when you do\, it doesn't feel subtle. It feels active. Alive. Because for a few hours\, the sky isn't static.\n\nIt's moving. Constantly.\n\nAnd once you see that\, it's hard to go back to thinking of the night sky as quiet.\n\nSources\n\nNASA Meteor Showers — https://science.nasa.gov/meteors\n\nInternational Meteor Organization — https://www.imo.net\n\nPeer-reviewed: Jewitt & Li (2010)\, 'Activity in Geminid Parent 3200 Phaethon'\, AJ Journal
URL:https://astrofarm.one/event/the-geminids/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Geminids.png
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BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261218T230000
DTEND;TZID=Europe/Madrid:20261219T033000
DTSTAMP:20260530T042915
CREATED:20260416T173526Z
LAST-MODIFIED:20260523T102322Z
UID:2049-1797634800-1797651000@astrofarm.one
SUMMARY:Moon and Saturn Repitition
DESCRIPTION:Moon And Saturn Meet Again — And This Time\, The Repetition IS The Point\n\nDecember 18\, 2026: You've seen this before. That's exactly why it matters now.\n\nBy now\, you've seen this before.\n\nThe Moon near Saturn. Two objects\, seemingly close. Two points that instantly draw your attention.\n\nAnd yet\, something about this one feels different.\n\nOn December 18\, 2026\, the Moon once again appears close to Saturn in the evening sky. It's not the first time this year. It's not even the closest.\n\nBut that's exactly why it matters.\n\nRepetition Changes How You See Things\n\nThe first time you see a conjunction like this\, it feels surprising. Unexpected. Two worlds appearing side by side.\n\nBy the third or fourth time? Something shifts.\n\nYou start to understand it. Not just intellectually. VISUALLY.\n\nYou recognize the pattern. You expect the alignment. And that changes the experience from "wow" to something more subtle. Something deeper.\n\nBecause now\, you're not just seeing the event. You're seeing the MOTION behind it.\n\nThe Moon\, moving quickly along its orbit\, catching up to Saturn again and again. Saturn\, barely moving in comparison. Stable. Distant. Almost fixed.\n\nThe Moon passes. Saturn remains.\n\nAnd over time\, that repetition reveals structure. Not randomness. But rhythm.\n\nThis Is The Transition That Changes Everything\n\nThis is one of the most important transitions in astronomy:\n\nThe moment when the sky stops being a collection of events and becomes a SYSTEM.\n\nBecause once you notice repetition\, you start to predict. You start to anticipate.\n\nAnd that's when observation becomes understanding.\n\nThe View Is Still Gorgeous\n\nVisually\, the scene is still striking. The Moon\, a thin crescent again\, hangs low in the evening sky. Soft light. Sharp edge. Earthshine faintly visible.\n\nAnd Saturn sits nearby\, dimmer but distinct. Steady. Unflickering.\n\nIf you use a telescope\, the contrast remains powerful. The Moon reveals its surface. Saturn reveals its rings.\n\nBut by now\, you already know that.\n\nAnd that's the difference. This time\, it's not about discovering something new. It's about recognizing something familiar.\n\nAnd realizing that familiarity doesn't reduce the experience.\n\nIt deepens it.\n\nBecause repetition isn't boring. It's how patterns become visible. And once you see those patterns\, the sky stops feeling random.\n\nIt starts to make sense.\n\nAnd that's a different kind of awe. Less immediate. But much more lasting.\n\nSources\n\nNASA Solar System Exploration — https://solarsystem.nasa.gov\n\nEuropean Southern Observatory — https://www.eso.org/public/science/\n\nESA Science — https://www.esa.int/Science_Exploration
URL:https://astrofarm.one/event/moon-and-saturn-repitition/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Moon-Saturn-Repetition.png
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BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261223T230000
DTEND;TZID=Europe/Madrid:20261225T033000
DTSTAMP:20260530T042915
CREATED:20260416T173829Z
LAST-MODIFIED:20260523T102445Z
UID:2052-1798066800-1798169400@astrofarm.one
SUMMARY:Christmas Supermoon
DESCRIPTION:The Christmas Supermoon Is Going To Hit Different — And Science Can Actually Explain Why\n\nDecember 23-24\, 2026: The closest full Moon since 2018\, arriving exactly when the whole world slows down.\n\nThere are full Moons you notice.\n\nAnd there are full Moons you remember.\n\nThe one on December 23-24\, 2026 is likely to be both.\n\nNot because it's dramatically different. Not because something rare or unexpected is happening.\n\nBut because timing changes everything.\n\nA supermoon — at its closest point to Earth — appearing just as people across the world slow down\, gather\, pause.\n\nAnd suddenly\, something ordinary feels different.\n\nThe Physics: This Is The Closest Full Moon Since 2018\n\nLet's start with the numbers:\n\nThis full Moon occurs near perigee — the point where the Moon is closest to Earth in its elliptical orbit. At this distance\, the Moon appears about 7% larger than average\, and up to 14% larger than the smallest full Moon of the year.\n\nThat's measurable. But subtle.\n\nOn its own\, you might not notice it.\n\nBut perception is never just about numbers.\n\nContext Is Everything\n\nLate December is different.\n\nThe nights are long. The air is often clearer. People are outside for different reasons. Or they're inside\, but looking out.\n\nAnd the Moon becomes part of that. A fixed point in a moment that otherwise feels temporary.\n\nThat combination changes how it's experienced.\n\nBecause this isn't just a supermoon. It's a shared moment.\n\nAcross cities\, countries\, time zones. The same Moon. Seen by millions of people at roughly the same time.\n\nAnd that creates something subtle\, but real. A sense of connection. Not in a literal sense. But in perception.\n\nBecause even though everyone is looking from a different place\, they're looking at the same object.\n\nAnd that's rare.\n\nNot Everything Meaningful Has To Be Rare\n\nAstronomically\, nothing unusual is happening beyond the geometry. No special alignment. No unique phenomenon. Just orbit. Distance. Light.\n\nBut sometimes\, that's enough.\n\nBecause what makes an observation meaningful isn't always the rarity of the event. It's the moment it exists in.\n\nAnd this one exists at a time when people are already paying attention. Already reflecting. Already slowing down.\n\nSo when the Moon rises — large\, bright\, steady — it feels like more than just another full Moon.\n\nEven if\, physically\, it isn't.\n\nAnd maybe that's the point.\n\nBecause not everything meaningful has to be rare. Sometimes\, it just has to be seen at the right time.\n\nDecember 23-24\, 2026. The closest full Moon since 2018. Arriving exactly when you might actually look up.\n\nSources\n\nNASA Moon — https://science.nasa.gov/moon\n\nEuropean Space Agency — https://www.esa.int/Science_Exploration\n\nPeer-reviewed: Chapront et al. (2002)\, 'Lunar orbital variations and distance'
URL:https://astrofarm.one/event/christmas-supermoon/
ATTACH;FMTTYPE=image/png:https://astrofarm.one/wp-content/uploads/2026/04/Christmas-Supermoon.png
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