WEBVTT

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So I want you to picture yourself on a just a

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really warm, lazy afternoon. You're sitting right

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under this large leafy tree. Oh, nice. Setting

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the scene. Right. And if you look down at the

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footpath around you, you'll see what you always

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see under a tree on a sunny day. Just thousands

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of those ordinary scattered round patches of

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dappled light filtering down through the canopy.

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Yeah, totally mundane. everyday physics exactly

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it's a completely mundane site but now picture

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that exact same afternoon that same tree but

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uh during a partial solar eclipse oh things get

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weird they get so weird the moon has just taken

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a little bite out of the sun's disc up in the

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sky right and if you look down at the footpath

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now suddenly All those patches of light are not

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round anymore. Not at all. Every single gap between

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the leaves above you has completely transformed.

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You are looking at a footpath scattered with

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thousands of tiny repeated crescents. It's honestly

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one of the most beautiful accidental science

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demonstrations in all of nature. Right, because

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it is a perfect miniature copy of whatever shape

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the sun currently is, just repeated over and

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over again on the ground. Yeah, and nobody arranged

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those leaves to do that. You know, it happens

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purely because of a phenomenon known as the pinhole

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camera effect. OK, so break that down for us.

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For anyone who hasn't encountered that term before,

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what is a pinhole camera? Well, it's a very simple

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optical trick, really. When light passes through

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a remarkably small opening. like the tiny gaps

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between overlapping leaves, that opening actually

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acts like a simple optical lens. Wow. Yeah. It

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takes the light from the source, which in this

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case is the sun, and faithfully projects an inverted

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image of that source onto whatever surface happens

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to be behind it. So the ground. So instead of

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just letting a generic, you know. blob of light

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through, the leaves are literally acting as thousands

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of tiny natural movie projectors. That's a great

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way to put it. Yeah. They're beaming the live

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status of the sun directly onto the dirt. Which

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is really the perfect entry point for what we

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are exploring today, because an eclipse itself

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is, I mean, it's really just a much grander version

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of that exact same basic idea. It really is.

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And the goal for this deep dive is to take an

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unhurried walk through the mathematically precise

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shadow play of eclipses. I love that. Shadow

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play. Yeah. We're going to explore the geometry

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that makes them possible, the history of how

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early humans figured out the patterns, and just

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the sheer visceral mechanics. of these cosmic

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alignments. Well, to really understand that grand

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shadow play, we have to zoom out from that tree

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for a second and look at the solar system as

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a whole. Okay, zooming out. An eclipse, fundamentally,

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is just one object in space blocking light on

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its way to another object. It's casting a shadow

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shaped by very simple geometry. Right, and there

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are two main types, solar and lunar. And the

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difference basically comes down to which object

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is doing the blocking. Exactly. So in a solar

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eclipse, the moon steps between the sun and earth.

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The moon's shadow falls on us. But in a lunar

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eclipse, Earth steps between the sun and the

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moon, and our massive shadow falls onto the lunar

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surface. Right. But if we start with solar eclipses,

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there is this fundamental question of scale that

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always kind of blows my mind. But the perfect

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fit. Yes. When you look up during a total solar

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eclipse, the moon seems to perfectly, exactly

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cover the sun. It's not too big, not too small.

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Does the math just happen to work out that they

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are physically the same size? Oh, not even close.

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The sun is massive. I mean, it is roughly 400

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times wider than the moon. 400 times. Yeah, but

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there's this staggering geometric coincidence

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at play here. The sun is also, on average, roughly

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400 times further away from Earth than the moon

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is. Wait, let me make sure I'm visualizing this

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correctly. So it would be like holding a tiny

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little coin right at arm's length and realizing

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that this tiny coin perfectly covers up a massive

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dinner plate that somebody's holding all the

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way on the other side of a long room. That is

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precisely how it works. When you multiply those

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two facts together, the 400 times width and the

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400 times distance, you get this extraordinary

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visual trick. It's like an optical illusion built

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into the solar system. Exactly. Seen from our

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vantage point here on Earth, The sun and the

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moon appear to be almost exactly the same size

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in the sky. They are so perfectly matched that

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during a total solar eclipse, the moon can precisely

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cover the sun's bright disk. No more. And no

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less. Which, I mean, that raises the question

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of why. Is there some gravitational law or, I

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don't know, physics rule that mandates this exact

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ratio in planetary systems? Yeah, and that's

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the wild part. As far as anyone in astronomy

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or astrophysics can tell, there is absolutely

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no known physical reason why those two objects

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have to line up this neatly. Wait, really? It's

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just random. It is simply a pure coincidence

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of how our particular solar system happened to

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form. That is wild. Well, this perfect match

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isn't even a permanent fixture. Because the moon

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isn't stationary, right? Like it's slowly drifting.

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Exactly. The moon is gradually moving away from

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Earth over these extremely long time scales,

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which means that total eclipses, as we experience

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them right now, are a temporary feature. Wow.

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Yeah. In the very long run of our planet's multi

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-billion year history, this... Perfect alignment

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is just a passing phase. We just happen to exist

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during the exact right window of time to see

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it. Okay, so we have this perfect temporary alignment.

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But the moon is orbiting the Earth, completing

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a lap roughly once a month, right? Correct. And

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it passes between us and the sun during every

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single new moon phase. Right, exactly. So if

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it's passing between us and the sun every single

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month, why aren't we plunged into darkness every

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30 days? Right, that's the obvious question.

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And it all comes down to what you could call

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orbital fussiness. Orbital fussiness, I like

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that. The key is that the moon's orbit is not

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perfectly flat relative to Earth's orbit. Okay.

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If you imagine the flat plane that the Earth

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travels on as it orbits the sun. Astronomers

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call this flat plane the ecliptic. Ecliptic,

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right. Yeah. So the moon's orbit around Earth

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doesn't sit perfectly level on that ecliptic.

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It is actually tilted by about five degrees.

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Okay, so if I picture like two hula hoops, one

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inside the other. Like an analogy. The outer

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hula hoop is the Earth going around the sun.

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And the inner hula hoop is the moon going around

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the Earth. But the inner one is just slightly

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tipped. Yes. So most of the time, the edges just

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don't actually line up. Exactly. I mean, five

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degrees sounds pretty negligible, right? But

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in the vastness of space, it is huge. Right,

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because of the distance. Exactly. It's more than

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enough that during most months, when the new

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moon passes in front of the sun, from our perspective,

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it actually passes slightly above the sun. you

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know slightly below it so it just misses the

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mark completely yeah his shadow gets cast out

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into empty space completely missing earth what

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actually has to happen for the shadow to hit

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us then well for an eclipse to occur a new moon

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has to happen very close to what astronomers

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call nodes yeah nodes these are the exact specific

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intersection points where that tilted lunar orbit

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physically crosses the flat plane of the Earth's

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orbit. So you need the moon to be at the new

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moon phase, and you need it to be sitting right

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at one of those precise intersection nodes. That's

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why eclipses are these rare, geometrically fussy

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events, and not just a monthly routine. Right.

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But even when they do hit those nodes and cast

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a shadow on Earth, the shadow doesn't always

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look the same, right? Like, we don't always get

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a total eclipse. Right, exactly. Sometimes we

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get an annular eclipse or a partial one. But

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if the ratio of the sun and moon size is so perfect,

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like we just talked about, what causes those

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variations? That comes down to another slight

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imperfection in the system. The moon's orbit

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isn't a perfect circle. It is slightly elliptical,

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meaning it's a bit oval -shaped. Oh, I see. So

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the physical distance between the Earth and the

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moon actually changes a bit throughout the month.

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When the moon happens to be at its closest point

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to Earth during one of those node alignments,

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it appears very slightly larger in our sky. And

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that's what gives us a total solar eclipse. Yes.

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The moon completely covers the sun's disk, plunging

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the area beneath the shadow into that eerie,

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temporary daytime darkness. But if the moon happens

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to be on the further end of that oval orbit when

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it crosses the node, then it appears very slightly

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smaller in the sky. So it isn't quite big enough

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to cover the whole solar disk. Right. And this

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is what creates an annular eclipse. People often

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call it a ring of fire. Oh, yeah, the ring of

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fire. Those pictures are incredible. They really

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are. Because a brilliant, thin ring of actual

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sunlight remains visible around the dark silhouette

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of the moon the entire time. And a partial eclipse

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would just be when the alignment isn't perfectly

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dead center? Exactly. Or maybe the observer on

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Earth is standing off to the side, you know,

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in the outer weaker part of the moon shadow.

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The moon only covers a chunk of the sun. Which

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brings us right back to our opening under the

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tree, producing all those little crescent shapes

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on the footpath. Full circle. Yeah, it's all

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dictated by distance and angles. And because

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this geometry operates basically like clockwork,

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it is incredibly predictable once you actually

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know the mechanics. Right. But early humans didn't

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know the mechanics. No, they definitely did not.

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I mean, before we understood elliptical orbits

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and five degree tilts, an eclipse must have been

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deeply, deeply unsettling. Just imagine you're

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going about your day and the sun just gets eaten

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by a black void. It would be terrifying. There's

00:09:27.419 --> 00:09:29.820
actually an old Chinese legend about two court

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astronomers, Hai and Hou, and they were supposedly

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executed for failing to predict an eclipse and

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warn the emperor in time. Oh, wow. High stakes.

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Right. And whether that's folklore or hard history,

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it really illustrates how early societies viewed

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these events. They weren't fun science demonstrations.

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They were terrifying omens that demanded an urgent

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official response. And because ancient astronomers

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were so heavily motivated to see these omens

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coming, They started noticing patterns. Because

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their lives literally depended on it. Exactly.

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Even without knowing the underlying physics,

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they realized eclipses weren't entirely random.

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And this led to the discovery of the Saros Cycle.

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Okay, the Saros Cycle. How does that cycle actually

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work? It is a marvel of early human observation.

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It is a period of very close to 18 years, 11

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days, and 8 hours. 18 years, 11 days, and 8 hours.

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That is very specific. Extremely specific. And

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after that exact amount of time, the sun, the

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earth, and the moon return to a nearly identical

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relative geometric arrangement. Because of this,

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a very similar eclipse will recur. But the extra

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8 hours is the catch, though, right? Because

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8 hours is a third of a day. meaning the Earth

00:10:43.909 --> 00:10:46.049
has rotated a third of the way around its axis

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since the last eclipse. And you nailed it. So

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the shadow will fall on a completely different

00:10:49.610 --> 00:10:52.309
part of the globe. Exactly right. And the reason

00:10:52.309 --> 00:10:54.929
the Saro cycle works at all is because it represents

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the precise moment when three completely separate

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lunar rhythms happen to sync up simultaneously.

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Wow, okay. Yeah. You have the time it takes the

00:11:04.269 --> 00:11:06.370
moon to return to the same phase. You have the

00:11:06.370 --> 00:11:07.889
time it takes the moon to return to the same

00:11:07.889 --> 00:11:10.690
node, you know, that intersection point in its

00:11:10.690 --> 00:11:12.509
tilted orbit. And you have the time it takes

00:11:12.509 --> 00:11:14.350
the moon to return to the same distance from

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Earth in its oval -shaped orbit. So it's like

00:11:16.990 --> 00:11:19.610
having three different ticking clocks, all with

00:11:19.610 --> 00:11:21.690
slightly different lengths, and just waiting

00:11:21.690 --> 00:11:24.149
for the exact moment they all chime at the same

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second. That is a perfect analogy. What stands

00:11:26.509 --> 00:11:29.490
out to me is that Babylonian, Chinese, and Greek

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observers figured this out through... Through

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sheer brute force pattern spotting. It's incredible.

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They kept meticulous records over centuries just

00:11:39.480 --> 00:11:42.159
to predict these events, long before they understood

00:11:42.159 --> 00:11:45.139
gravity or orbits. Though, you know, we should

00:11:45.139 --> 00:11:47.399
give credit where it's due. The Greek philosopher

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Anaxagoras actually did correctly guess the geometry

00:11:50.559 --> 00:11:53.720
way back in the 5th century BCE. Wait, really?

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The 5th century BCE? Yeah. He argued that a solar

00:11:57.700 --> 00:12:00.240
eclipse was just the moon passing in front of

00:12:00.240 --> 00:12:02.860
the sun. It was a strikingly modern explanation

00:12:02.860 --> 00:12:05.700
for an ancient world that still largely relied

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on mythology. That is amazing. But if Anaxagoras

00:12:09.330 --> 00:12:11.909
was the start of understanding eclipses, the

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absolute pinnacle of eclipse science has to be

00:12:14.730 --> 00:12:17.529
1919. Oh, absolutely. Because this is the moment

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a shadow literally changed how we understand

00:12:19.769 --> 00:12:21.149
the fabric of the universe. You're referring

00:12:21.149 --> 00:12:23.429
to Arthur Eddington's expedition. Yes. In May

00:12:23.429 --> 00:12:26.169
of 1919, the British astronomer Arthur Eddington

00:12:26.169 --> 00:12:29.230
led teams to the island of Principe off West

00:12:29.230 --> 00:12:32.509
Africa and to Sobral in Brazil, specifically

00:12:32.509 --> 00:12:35.629
to observe a total solar eclipse. But he wasn't

00:12:35.629 --> 00:12:37.350
there to study the eclipse itself, though, right?

00:12:37.389 --> 00:12:40.230
No, not at all. He was using the eclipse as a

00:12:40.230 --> 00:12:43.149
tool to test a brand new, highly controversial

00:12:43.149 --> 00:12:45.649
theory published by Albert Einstein. General

00:12:45.649 --> 00:12:48.929
relativity. Precisely. Einstein's theory proposed

00:12:48.929 --> 00:12:52.200
something totally radical. that massy objects

00:12:52.200 --> 00:12:55.559
like our sun actually bend the physical fabric

00:12:55.559 --> 00:12:57.679
of space and time around them. Which sounds completely

00:12:57.679 --> 00:13:00.539
wild. It sounded absurd to a lot of people. But

00:13:00.539 --> 00:13:02.639
because of that bent space, Einstein predicted

00:13:02.639 --> 00:13:04.980
that light traveling from distant stars should

00:13:04.980 --> 00:13:08.620
be deflected or bent very slightly as it passed

00:13:08.620 --> 00:13:11.059
close to the heavy mass of the sun on its way

00:13:11.059 --> 00:13:13.840
to our eyes here on Earth. Right, but the problem

00:13:13.840 --> 00:13:17.279
with testing that... on a normal tuesday is that

00:13:17.279 --> 00:13:19.200
you can't just look at stars right next to the

00:13:19.200 --> 00:13:22.399
sun no definitely not the sun's glare is blinding

00:13:22.399 --> 00:13:25.679
the sky is bright blue and the stars are completely

00:13:25.679 --> 00:13:28.539
invisible which is why totality is so crucial

00:13:28.539 --> 00:13:31.139
for this during those few minutes of a total

00:13:31.139 --> 00:13:34.620
solar eclipse the sun's bright disk is completely

00:13:34.620 --> 00:13:38.730
blocked by the moon the sky goes dark suddenly

00:13:38.730 --> 00:13:41.450
stars close to the sun's position in the sky

00:13:41.450 --> 00:13:44.230
become briefly visible right in the middle of

00:13:44.230 --> 00:13:46.110
the day. It's like turning off the lights in

00:13:46.110 --> 00:13:48.250
a room so you can see out the window. Exactly.

00:13:48.330 --> 00:13:50.450
So Eddington's team photographed those stars

00:13:50.450 --> 00:13:53.570
during the eclipse. Then they compared those

00:13:53.570 --> 00:13:56.149
photos against photos of the exact same stars

00:13:56.149 --> 00:13:59.149
taken months earlier at night when the sun was

00:13:59.149 --> 00:14:01.070
nowhere near them. And when they developed those

00:14:01.070 --> 00:14:03.669
photos, the stars in the eclipse image appeared

00:14:03.669 --> 00:14:06.029
to have shifted. Yes. They had moved by almost

00:14:06.029 --> 00:14:08.629
the exact amount that Einstein's math predicted.

00:14:08.809 --> 00:14:11.450
The sheer mass of the sun had bent the light

00:14:11.450 --> 00:14:14.029
passing by it. It's just phenomenal. A shadow

00:14:14.029 --> 00:14:16.629
lasting just a few minutes provided the perfect

00:14:16.629 --> 00:14:19.169
natural laboratory to prove that space -time

00:14:19.169 --> 00:14:21.740
is flexible. I mean... It established relativity

00:14:21.740 --> 00:14:24.639
as serious, tested physics. It is a beautiful

00:14:24.639 --> 00:14:27.299
convergence of events. Yeah. It really highlights

00:14:27.299 --> 00:14:30.659
just how uniquely valuable totality is for science.

00:14:30.879 --> 00:14:33.379
And beyond the science, the experience of totality

00:14:33.379 --> 00:14:37.100
itself is described as just a genuinely startling,

00:14:37.100 --> 00:14:40.600
bizarre sensory event. Oh, it is. It's profoundly

00:14:40.600 --> 00:14:43.039
weird. It's not just that the sky gets a bit

00:14:43.039 --> 00:14:46.039
dark, right? In the minutes leading up to totality,

00:14:46.139 --> 00:14:48.580
the quality of the light fundamentally changes.

00:14:48.799 --> 00:14:51.639
It flattens out. Yes, it flattens. Shadows sharpen

00:14:51.639 --> 00:14:53.899
in a way that feels incredibly unnatural. You

00:14:53.899 --> 00:14:55.600
can actually feel the temperature measurably

00:14:55.600 --> 00:14:58.279
drop as the sunlight is suddenly cut off. And

00:14:58.279 --> 00:15:01.240
then for anywhere from a few seconds to maybe

00:15:01.240 --> 00:15:04.139
seven minutes, totality sets in. And to understand

00:15:04.139 --> 00:15:06.019
what you're seeing in that specific moment, we

00:15:06.019 --> 00:15:08.059
need to define two distinct parts of the sun.

00:15:08.240 --> 00:15:11.120
Okay. First, there's the photosphere. That is

00:15:11.120 --> 00:15:14.639
the sun's bright, normally visible disk. It's

00:15:14.639 --> 00:15:16.779
the blinding surface we're used to seeing. Right,

00:15:16.879 --> 00:15:19.250
the part that hurts to look at. Exactly. During

00:15:19.250 --> 00:15:21.610
totality, that photosphere is completely blocked.

00:15:21.830 --> 00:15:24.250
And because it's blocked, something normally

00:15:24.250 --> 00:15:28.100
invisible is unveiled. The corona. The corona

00:15:28.100 --> 00:15:30.539
being the sun's atmosphere. Right. It is this

00:15:30.539 --> 00:15:34.120
wispy pale halo of extremely hot, extremely thin

00:15:34.120 --> 00:15:37.460
plasma that extends millions of kilometers out

00:15:37.460 --> 00:15:39.539
into space from the sun's surface. And it's always

00:15:39.539 --> 00:15:41.820
there, isn't it? It is always there. Under normal

00:15:41.820 --> 00:15:43.440
daylight conditions, it's happening right now.

00:15:43.559 --> 00:15:46.720
But it is roughly a million times dimmer than

00:15:46.720 --> 00:15:49.799
the photosphere. It is just... utterly overwhelmed

00:15:49.799 --> 00:15:53.039
by the glare so totality removes the glare and

00:15:53.039 --> 00:15:56.379
the corona appears exactly and for a huge chunk

00:15:56.379 --> 00:15:59.200
of the 20th century a total eclipse was basically

00:15:59.200 --> 00:16:02.039
the only practical way for scientists to study

00:16:02.039 --> 00:16:04.700
the corona at all it's that dramatic reveal that

00:16:04.700 --> 00:16:06.860
drives you know eclipse chasers to travel the

00:16:06.860 --> 00:16:09.480
globe heading to isolated places like xmith in

00:16:09.480 --> 00:16:12.700
western australia in 2023 or like preparing for

00:16:12.700 --> 00:16:15.799
sydney in july 2028 oh yeah they plan years in

00:16:15.799 --> 00:16:18.139
advance they are chasing these fleeting visual

00:16:18.250 --> 00:16:20.210
phenomena that only happen for seconds, like

00:16:20.210 --> 00:16:22.970
Bailey's beads. Oh, Bailey's beads are spectacular.

00:16:23.370 --> 00:16:26.070
They occur just before and just after totality.

00:16:26.190 --> 00:16:28.610
What causes them? Well, the moon doesn't have

00:16:28.610 --> 00:16:30.950
a perfectly smooth edge, right? It is covered

00:16:30.950 --> 00:16:33.830
in mountains and deep valleys. Oh, right. So

00:16:33.830 --> 00:16:36.309
right at the edge of alignment, sunlight streams

00:16:36.309 --> 00:16:39.049
through those deep lunar valleys, breaking up

00:16:39.049 --> 00:16:41.409
into a scatter of brilliant, distinct points

00:16:41.409 --> 00:16:44.909
of light around the moon's silhouette. It looks

00:16:44.909 --> 00:16:47.840
like a string of glowing lamps. And then as the

00:16:47.840 --> 00:16:51.500
very last bead fades right before totality, or

00:16:51.500 --> 00:16:54.259
as the very first one reappears after, you get

00:16:54.259 --> 00:16:56.220
what is called the diamond ring effect. Yes,

00:16:56.240 --> 00:16:59.710
the classic diamond ring. It is one single intense

00:16:59.710 --> 00:17:02.909
glowing point of light attached to this pale

00:17:02.909 --> 00:17:05.829
ring. It is arguably the most photographed moment

00:17:05.829 --> 00:17:08.250
of any eclipse. Oh, without a doubt. And while

00:17:08.250 --> 00:17:09.970
you're watching this, birds are suddenly falling

00:17:09.970 --> 00:17:12.609
silent, insects start chirping thinking it's

00:17:12.609 --> 00:17:14.990
night, and you might even see shadow bands. Shadow

00:17:14.990 --> 00:17:17.029
bands are such a strange phenomenon. They are

00:17:17.029 --> 00:17:19.670
these fast -moving, rippling patterns of light

00:17:19.670 --> 00:17:22.950
and shadow that can race across pale, flat surfaces

00:17:22.950 --> 00:17:25.809
right around totality. Like ripples at the bottom

00:17:25.809 --> 00:17:29.430
of a pool. Yes. Exactly like that. They're caused

00:17:29.430 --> 00:17:32.230
by that tiny remaining sliver of sunlight being

00:17:32.230 --> 00:17:35.130
refracted unevenly by turbulence in Earth's own

00:17:35.130 --> 00:17:38.369
atmosphere. That is so cool. Okay, so if the

00:17:38.369 --> 00:17:40.690
moon's shadow causes all this daytime drama,

00:17:40.950 --> 00:17:43.869
what happens when we reverse the geometry? Let's

00:17:43.869 --> 00:17:46.470
talk about lunar eclipses. The lunar reverse.

00:17:46.589 --> 00:17:49.269
Right. Earth steps into the middle, and it's

00:17:49.269 --> 00:17:51.650
our massive shadow blocking the sunlight from

00:17:51.650 --> 00:17:53.609
hitting the full moon. The immediate question

00:17:53.609 --> 00:17:56.539
is... If the Earth is completely blocking the

00:17:56.539 --> 00:17:59.079
sun, why doesn't the moon just go pitch black?

00:17:59.319 --> 00:18:01.119
That's a great question. Why does it turn that

00:18:01.119 --> 00:18:04.339
famous deep coppery red, you know, the blood

00:18:04.339 --> 00:18:07.559
moon? The answer to that lies in our own planet's

00:18:07.559 --> 00:18:09.779
atmosphere through a process called Rayleigh

00:18:09.779 --> 00:18:12.519
scattering. Okay, walk us through how Rayleigh

00:18:12.519 --> 00:18:15.599
scattering turns a dark shadow red. Sure. So

00:18:15.599 --> 00:18:17.680
as sunlight travels toward Earth, it hits our

00:18:17.680 --> 00:18:19.960
atmosphere. And our atmosphere acts like a lens

00:18:19.960 --> 00:18:22.559
and a filter combined. It bends some of that

00:18:22.559 --> 00:18:25.119
light inward. toward the shadow behind Earth.

00:18:25.500 --> 00:18:28.359
But as it does this, it filters out the shorter,

00:18:28.500 --> 00:18:31.680
bluer wavelengths of light. This exact scattering

00:18:31.680 --> 00:18:33.980
of blue light is actually the reason our daytime

00:18:33.980 --> 00:18:36.720
sky looks blue to us down on the ground. Because

00:18:36.720 --> 00:18:38.859
the blue light gets trapped and scattered around

00:18:38.859 --> 00:18:41.480
in the atmosphere. Exactly. So if the atmosphere

00:18:41.480 --> 00:18:44.119
scatters away all the blue light, what's left

00:18:44.119 --> 00:18:46.519
to pass through? The longer wavelengths. The

00:18:46.519 --> 00:18:49.759
reds and oranges. Yes. The reds, the oranges.

00:18:50.490 --> 00:18:53.369
The coppery colors. This reddish light survives

00:18:53.369 --> 00:18:55.450
the trip through the edges of Earth's atmosphere,

00:18:55.650 --> 00:18:58.369
gets bent into our shadow by refraction, and

00:18:58.369 --> 00:19:00.710
falls squarely onto the moon's surface. So the

00:19:00.710 --> 00:19:02.650
Earth's atmosphere is basically acting like a

00:19:02.650 --> 00:19:05.630
giant cosmic color filter. Pretty much. It tosses

00:19:05.630 --> 00:19:07.650
out the blue light and it bends the reddish light

00:19:07.650 --> 00:19:09.759
from the edges of the Earth. It's projecting

00:19:09.759 --> 00:19:11.940
the collective light of all the world's sunsets

00:19:11.940 --> 00:19:14.059
and sunrises onto the moon at the exact same

00:19:14.059 --> 00:19:16.799
time. That is an incredibly accurate way to describe

00:19:16.799 --> 00:19:19.380
it. A blood moon is quite literally illuminated

00:19:19.380 --> 00:19:22.319
by every sunset and sunrise happening on Earth

00:19:22.319 --> 00:19:24.900
in that specific moment. That is almost poetic.

00:19:25.119 --> 00:19:27.779
It really is. And what makes lunar eclipses so

00:19:27.779 --> 00:19:30.920
accessible is their scale. Earth's shadow is

00:19:30.920 --> 00:19:34.170
massive compared to the moon. Right. So when

00:19:34.170 --> 00:19:36.630
a lunar eclipse happens, you don't have to travel

00:19:36.630 --> 00:19:39.369
to a tiny specific path like you do for a total

00:19:39.369 --> 00:19:42.230
solar eclipse. A lunar eclipse is visible to

00:19:42.230 --> 00:19:45.089
the entire nighttime hemisphere of Earth simultaneously.

00:19:45.849 --> 00:19:48.990
And it lasts for hours, not minutes. You literally

00:19:48.990 --> 00:19:51.049
just walk outside and look up, which actually

00:19:51.049 --> 00:19:53.490
brings us to a really critical safety point here.

00:19:53.589 --> 00:19:55.589
Yes, very important. Looking at a lunar eclipse

00:19:55.589 --> 00:19:58.509
is perfectly safe. Looking at a solar eclipse,

00:19:58.670 --> 00:20:01.710
however, requires understanding a very real biological

00:20:01.710 --> 00:20:04.049
danger. We have to be very direct about this.

00:20:04.269 --> 00:20:07.069
Looking directly at the sun at any point during

00:20:07.069 --> 00:20:09.809
a partial solar eclipse or even during the partial

00:20:09.809 --> 00:20:12.829
phases leading up to and following totality is

00:20:12.829 --> 00:20:15.230
intensely dangerous to your eyesight. Even if

00:20:15.230 --> 00:20:17.670
the sun looks dimmer or a large chunk of it is

00:20:17.670 --> 00:20:20.430
missing? the invisible radiation is still hitting

00:20:20.430 --> 00:20:23.250
your eye. And the scariest part is that you won't

00:20:23.250 --> 00:20:25.750
feel it happening. No, you won't. The retina,

00:20:25.750 --> 00:20:27.630
which is the light -sensitive tissue at the back

00:20:27.630 --> 00:20:29.589
of your eye, has absolutely no pain receptors.

00:20:29.809 --> 00:20:32.230
None. So you just don't feel it burning. Exactly.

00:20:32.289 --> 00:20:34.869
This means you can literally burn permanent blind

00:20:34.869 --> 00:20:37.849
spots into your vision without feeling a single

00:20:37.849 --> 00:20:40.349
thing while the damage is occurring. The damage

00:20:40.349 --> 00:20:42.950
is silent and it is permanent. And regular sunglasses

00:20:42.950 --> 00:20:45.910
don't help, right? Ordinary sunglasses, regardless

00:20:45.910 --> 00:20:48.670
of how dark or how expensive they are, offer

00:20:48.670 --> 00:20:52.069
zero protection against this specific kind of

00:20:52.069 --> 00:20:55.829
solar radiation. So to view a partial solar eclipse

00:20:55.829 --> 00:20:59.369
safely... You must use purpose -built certified

00:20:59.369 --> 00:21:02.150
solar filters, you know, the specific cardboard

00:21:02.150 --> 00:21:04.410
eclipse glasses with international safety ratings.

00:21:04.589 --> 00:21:06.950
Yes. Or you go back to where we started this

00:21:06.950 --> 00:21:09.869
deep dive, indirect viewing. You make a pinhole

00:21:09.869 --> 00:21:11.890
projector with a piece of card and you safely

00:21:11.890 --> 00:21:14.769
watch the projection on the ground, just like

00:21:14.769 --> 00:21:18.289
the leaves do. There is one and only one genuine

00:21:18.289 --> 00:21:20.470
exception to this rule. And that's totality.

00:21:20.630 --> 00:21:25.190
Yes. The brief window of 100 % totality. Only

00:21:25.190 --> 00:21:28.250
when the sun's bright disk is completely, totally

00:21:28.250 --> 00:21:31.190
covered by the moon does it become safe and truly

00:21:31.190 --> 00:21:33.849
spectacular to look directly at the Carina with

00:21:33.849 --> 00:21:35.869
the naked eye. But you have to be absolutely

00:21:35.869 --> 00:21:39.210
certain totality has begun. Exactly. And the

00:21:39.210 --> 00:21:41.549
second that diamond ring flashes and the sun

00:21:41.549 --> 00:21:44.769
starts to reappear, the protective filters must

00:21:44.769 --> 00:21:47.680
go straight back on. It requires care, but the

00:21:47.680 --> 00:21:49.900
payoff of seeing the corona is apparently just

00:21:49.900 --> 00:21:53.279
life -changing. It's unparalleled. So, as we

00:21:53.279 --> 00:21:55.180
wrap up our journey through the shadows today,

00:21:55.319 --> 00:21:57.640
I want to bring you back to that warm afternoon.

00:21:57.859 --> 00:22:00.859
Put yourself back under that leafy tree. Right

00:22:00.859 --> 00:22:02.900
back where we started. The next time you find

00:22:02.900 --> 00:22:05.299
yourself standing under a canopy on an ordinary

00:22:05.299 --> 00:22:08.599
sunny afternoon, remember what is actually happening.

00:22:09.200 --> 00:22:12.099
Every single gap in the leaves above you is quietly

00:22:12.099 --> 00:22:15.299
acting as a camera, faithfully tracing the truth

00:22:15.299 --> 00:22:17.599
of the cosmos right onto the ground at your feet,

00:22:17.700 --> 00:22:19.880
whether anything unusual is happening up there

00:22:19.880 --> 00:22:23.059
or not. It is a quiet, ongoing record of our

00:22:23.059 --> 00:22:26.480
solar system's mechanics. But, you know, understanding

00:22:26.480 --> 00:22:29.579
these incredibly precise mechanics opens up one

00:22:29.579 --> 00:22:32.539
final, fascinating reality to think about. Oh,

00:22:32.619 --> 00:22:34.619
what's that? We talked earlier about how the

00:22:34.619 --> 00:22:36.259
moon is gradually moving away from the Earth,

00:22:36.339 --> 00:22:38.299
right? Right, the slow drift. Because of that

00:22:38.299 --> 00:22:41.759
drift, We know that one day, millions of years

00:22:41.759 --> 00:22:44.279
from now, the moon will be too far away to ever

00:22:44.279 --> 00:22:47.559
fully cover the sun's disk. Total eclipses will

00:22:47.559 --> 00:22:50.859
simply cease to exist on Earth. Wow. Future beings

00:22:50.859 --> 00:22:53.740
will only ever see partial or annular eclipses,

00:22:53.740 --> 00:22:55.960
never a total one. That's sort of heartbreaking,

00:22:56.099 --> 00:22:58.599
but also amazing. It really is. And it invites

00:22:58.599 --> 00:23:01.829
a pretty profound question. What other temporary

00:23:01.829 --> 00:23:04.970
cosmic masterpieces are we just taking for granted

00:23:04.970 --> 00:23:07.970
right now, simply because our tiny slice of human

00:23:07.970 --> 00:23:10.269
history happened to align perfectly with the

00:23:10.269 --> 00:23:12.269
clockwork of the universe? Something to mull

00:23:12.269 --> 00:23:13.769
over the next time you're standing in the shade.
