WEBVTT

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Howdy Star Gazers and welcome to Star Trails.

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My name is Drew and I'll be your guide to the

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night sky for the week of October the 19th through

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the 25th. The calendar says late October and

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the heavens agree. Crisp air, long nights, and

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a new moon make this one of the best observing

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weeks of the year. And since Halloween creeps

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ever closer, we're continuing our eerie tour

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of the cosmos with a visit to a place both beautiful

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and haunting, the Cosmic Graveyard, where dead

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stars still whisper across time. Whether you're

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tuning in from the backyard, the balcony, or

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just your imagination, I'm glad you're here.

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So, find a cozy spot, let your eyes adjust, and

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let's see what the sky holds for us this week.

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The moon disappears this week, reaching its new

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phase on Tuesday, October 21st. That means a

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stretch of wonderfully dark skies from Sunday

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through Friday, perfect for galaxies, nebula,

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and meteor watching. And speaking of meteors,

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the Orionids peak Monday night into Tuesday morning.

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These swift streaks are the dust of Halley's

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Comet, burning up as Earth plows through the

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debris field. With no moonlight to wash them

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out, you could catch 10 to 20 per hour under

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good conditions. Face southeast after midnight,

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lie back, and enjoy one of autumn's finest shows.

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Now for the planets. Saturn glows in the southeast

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after dusk, nestled in Aquarius. It's still bright

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and steady, and its moon Titan is visible in

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modest telescopes. Jupiter rises around midnight

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in Gemini, climbing higher each morning. Watch

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for its shifting cloud belts and dancing moons.

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Mars and Mercury linger low in the western twilight,

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challenging but not impossible with binoculars

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and a flat horizon. As the constellations wheel

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overhead, Pegasus and the Great Square mark the

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heart of the autumn sky. Follow the chain of

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stars east to Andromeda, and you'll find the

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glowing oval of M31, our neighboring galaxy,

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easily seen in binoculars. Below that, seek out

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M33, the Triangulum Galaxy, a faint but graceful

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swirl of starlight. Farther west, Perseus rises

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with a glittering double cluster, while Cassiopeia's

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W shape rides high, tracing the Milky Way's rich

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star fields. Down south near Saturn, swing your

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scope toward M2 in Aquarius, a fine globular

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cluster. And if you have a nebula filter, check

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out the Helix Nebula, a ghostly ring of gas that

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lives up to its nickname, the Eye of God. Stay

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up past midnight and you'll see Taurus climb

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the eastern sky, bringing the Hyades and the

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Pleiades, the first messengers of winter. Before

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we get into the second half of the show, I wanted

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to respond to an excellent listener question,

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and it's one that's been on my mind also. The

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listener writes, I'm seeing the same artist's

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depiction of a black hole everywhere lately,

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notably as the logo for the AI service Grok,

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which appears all over Twitter or X, but also

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in movies like Interstellar. Is this really what

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a black hole looks like? Thanks for that question,

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and if you follow any space news, you probably

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know exactly what the listener is referring to.

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That striking, impossible -looking figure that

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sort of resembles a ringed planet, maybe if designed

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by MC Escher. It's sort of a glowing lopsided

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ring with a dark center, and it's been plastered

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across science videos, documentaries, space agency

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posters, and yes, the logo for the ex -owned

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AI service, Grok. It looks almost too perfect,

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like some digital artist cooked it up after a

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late -night sci -fi binge. In case you've never

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seen one of these depictions, I'll include a

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link to such an image in the show notes. Well,

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here's the twist. That image is rooted in the

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actual physics of how black holes warp light.

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What looks like a sleek bit of graphic design

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is possibly a very accurate visualization. Let's

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unpack it. At the center of that image is a dark

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patch. It isn't the black hole itself, because

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you can't actually see a black hole. Think of

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it as the shadow of a black hole. When light

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from hot gas passes near the event horizon, the

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black hole's gravity bends those paths. Photons

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that get too close are trapped forever, creating

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a dark silhouette slightly larger than the event

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horizon. That's what we're looking at when we

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see that central void. Surrounding it is the

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bright thin ring. That's made of photons that

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have orbited the black hole before escaping toward

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us. Think of light caught in a cosmic racetrack

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looping around at breakneck speed, then slingshotting

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off to hit our telescopes. This is called the

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photon ring, and its existence is a direct consequence

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of Einstein's general relativity. But the part

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that really gives the image its distinctive shape

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is the crescent, the brighter arc on one side

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of the ring. That asymmetry is due to a relativistic

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effect called Doppler boosting. Contrary to what

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we might think, black holes don't just suck in

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matter from every direction. In almost all cosmic

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environments, the gas around them has some spin.

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Thanks to the conservation of angular momentum,

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that gas can't just fall straight in. It forms

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a flat, spinning accretion disk. Over time, turbulence

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and magnetic forces shuffle angular momentum

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outward, letting material slowly spiral inward

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and heat up. This disk is what lights up so brightly

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that we can actually see the black hole's surroundings,

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even though the hole itself remains invisible.

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The gas in the accretion disk is whipping around

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the black hole at a significant fraction of the

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speed of light. On the side rotating towards

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us, the light is intensified. On the opposite

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side, it's dimmed. The result is that glowing

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curve you see. In 2019, the Event Horizon Telescope

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gave us the first real image of a black hole's

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shadow in the galaxy M87, and it looked a lot

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like these simulation images. A glowing asymmetric

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ring around a dark center. So far, it's our best

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glimpse at gravity in its purest, most extreme

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form. In a moment, we'll leave the living sky

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behind and step into a darker realm, a place

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where suns have burned out, galaxies devour one

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another, and time itself decays to silence. We're

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headed into the cosmic graveyard. That's coming

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up after the break. Stay with us. Welcome back.

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Tonight we walk among the tombstones of the universe.

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Our destination is not a place, but a condition.

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The cold and quiet aftermath of creation itself.

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This is the Cosmic Graveyard. When you look up,

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the stars seem eternal. But many of those pinpoints

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are already dead, their light still traveling

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towards us, tricking our eyes with the glow of

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long -expired suns. The universe is a cemetery

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of extinguished stars and broken galaxies, a

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realm where everything bright must one day fade.

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First, let's take a look at white dwarves, the

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embers of suns. Stars like our sun end their

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lives gently. They swell into red giants, shed

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their outer layers, and leave behind a dense

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core about the size of Earth. That remaining

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ember is a white dwarf, a glowing cinder cooling

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slowly for billions of years. Someday, each will

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fade to invisibility. becoming a black dwarf,

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though the universe isn't old enough for any

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to exist yet. They are the quiet ashes of creation.

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Then there are neutron stars, the undead pulsars.

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Massive stars die violently. Their cores collapse

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in a flash, crushing protons and electrons into

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neutrons. The resulting neutron star packs the

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sun's mass into a sphere just a dozen miles wide.

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A teaspoon of that matter outweighs a mountain.

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Some spin rapidly, beaming radio pulses into

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space. We call them pulsars, rotating corpses

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that tick like cosmic clocks. When first discovered

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they were nicknamed LGM 1 for little green men

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But these aren't signals from aliens. They're

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the heartbeats of dead stars that refuse to stop

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Then there are black holes Graves with no bottom

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for the heaviest stars gravity wins completely

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their cores collapse beyond recovery forming

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black holes, regions where not even light can

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escape. They devour nearby stars, twist time

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and shape entire galaxies. They're tombs without

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headstones, yet they also sculpt the cosmos.

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But even black holes will not endure forever.

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Physicist Stephen Hawking showed that black holes

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leak energy. tiny sparks of radiation. And that

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means given enough time, even these ultimate

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graves will evaporate into nothing. Even galaxies

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can die, and they cannibalize each other. Galaxies

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themselves expire through consumption. Big ones

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devour small ones, scattering stellar remains

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across the cosmos. Our own Milky Way is guilty.

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Right now, it's consuming the Sagittarius dwarf

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galaxy. It's stars smeared across the sky like

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ashes scattered by a cosmic wind. And in about

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four billion years, Andromeda will collide with

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us. Two spirals locked together, merging into

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a single bloated relic. Even in death, gravity

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hungers. The far future brings the great dimming.

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Eventually, star birth ceases, the last red dwarfs

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fade, the galaxies darken, and black holes evaporate.

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The cosmos cools toward absolute zero, the heat

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death of everything. It's a state of perfect

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equilibrium where no energy remains to power

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change, light, or life. Just the last photons

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drifting through infinite darkness. If the stars

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spoke to you this week or if a question's been

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on your mind, I'd love to hear it. Visit StarTrails

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.Show where you can contact me and explore past

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episodes. Be sure to follow Star Trails on Blue

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Sky and YouTube. Links are in the show notes.

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Until we meet again beneath the stars, clear

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skies everyone.
