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Why do 36 of Andromeda’s 37 satellite galaxies point toward the Milky Way? This strange alignment presents a serious Andromeda galaxy mystery that defies the Lambda CDM model, the leading theory of cosmology. Discover why this bizarre cosmic imbalance may reveal a deeper dark matter problem in our understanding of the universe. Credit:
Blazars at Galactic North Pole: By NASA/DOE/Fermi LAT Collaboration, https://svs.gsfc.nasa.gov/10505/
NASA Animation Sizes Up the Universe’s Biggest Black Holes: By NASA's Goddard Space Flight Center Conceptual Image Lab, https://svs.gsfc.nasa.gov/14335
Why NASA's Roman Mission Will Study Milky Way's Flickering Lights: By NASA's Goddard Space Flight Center, https://svs.gsfc.nasa.gov/14438/
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Transcript
00:00A vast galactic mystery has recently baffled astronomers.
00:04They've noticed that all but one of Andromeda's 37 satellite galaxies point toward the Milky Way.
00:11It's so extraordinary that it challenges current cosmology and might provide the answer to the dark matter question.
00:18So it happened like this.
00:20One day, scientists looked at those other satellite galaxies that go around Andromeda and spotted a really weird alignment.
00:27Now, we should keep in mind that Andromeda is kind of like our Milky Way's neighbor.
00:32It's huge, about twice as wide as the Milky Way, stretching 200,000 light-years across.
00:38It also has way more stars, around a trillion, compared to our galaxy's mere 250 to 400 billion.
00:47Just like our galaxy, it has a bunch of tiny galaxies called dwarf galaxies spinning around it.
00:52There are 37 of them.
00:54The strange thing is, almost all of those little galaxies are on the same side of Andromeda.
01:01And it's getting even creepier, because it's the side that faces the Milky Way.
01:06Only one galaxy is hanging out on the other side.
01:10Imagine tossing a bunch of marbles around a tree, with nearly every single marble landing on just one side.
01:16That's weird, isn't it?
01:18Scientists say that this discovery doesn't match what they expected at all.
01:22Their usual space models show that stuff like this should be spread out more evenly.
01:27But this isn't even close to even.
01:30It's so lopsided that they can't really explain it yet.
01:33Those models follow the main space theory we use today, called the Lambda Cold Dark Matter model.
01:39According to this theory, the little galaxy should be spread around Andromeda pretty evenly.
01:45Maybe just a bit lopsided.
01:46But in real life, their distribution is way more uneven than the model said it should be.
01:52The scientists have run tons of simulations, and only about 0.3% of them ended up close to what we actually see.
02:00And still, none of them match the real thing exactly.
02:03So, does it show the Lambda CDM model has flaws?
02:07That would be a big deal, because we normally use this model to explain how the universe works.
02:13If the real sky doesn't match what our model says, especially in a place as close and well-known as Andromeda,
02:20it might mean that we're missing something big.
02:24Another strange thing.
02:26Many of Andromeda's satellites seem to lie in a flat plane instead of being randomly distributed in all directions.
02:33This kind of flattened structure has been seen in other big galaxies, too, including our own.
02:38But it's still not well understood.
02:40Maybe this satellite disk is connected to the weird cosmic asymmetry, but no one really knows how.
02:47In any case, the fact that all the tiny galaxies on Andromeda's side line up almost perfectly in the direction of the Milky Way is super weird.
02:57It makes you wonder, could our galaxy be pulling or affecting them?
03:01But the catch is that nothing like this is happening to the Milky Way's own satellites.
03:06Plus, the gravity between our two galaxies doesn't seem strong enough to do that kind of pulling.
03:13The answer might lie in one of the most mysterious things the universe has to offer.
03:18Dark matter.
03:19Let's start from the very beginning.
03:21We'll go all the way back to the early universe, just after the Big Bang.
03:25Now, back then – hey, I wasn't around then, but I'll tell you anyways – matter in the universe was spread out pretty evenly.
03:32But not perfectly even.
03:34In a few spots, there were just slightly higher amounts of matter than in others – tiny clumps.
03:40Those little differences were important, because gravity could latch onto them.
03:44Over time, those denser regions started pulling in more material, slowly growing into the first structures in the universe.
03:52Astronomers believed that dwarf galaxies were the earliest and smallest building blocks of galaxy formation.
03:58Think of them like Lego bricks – tiny pieces that were later pulled together by gravity to build larger galaxies over billions of years.
04:06Now, when we talk about matter, we mean two different things.
04:11Normal matter, the kind we can see and touch, including atoms, gas, stars, planets, and everything around us.
04:17And dark matter, the invisible kind.
04:20It doesn't give off any light, doesn't absorb it, and doesn't interact with normal matter in the usual ways.
04:26The only reason we know it exists is because of its gravitational pull.
04:31There's also a lot more of it than normal matter.
04:34Scientists think that roughly 85% of all matter in the universe is dark matter.
04:40At the same time, we've never directly detected a dark matter particle.
04:44But we know dark matter is there because it bends light, it holds galaxies together,
04:49they spin too fast to stay intact otherwise, and it shapes the structure of the universe,
04:54allowing us to map its influence on larger scales.
04:57While normal matter can clump together, crash, heat up, cool down, and eventually form stars and galaxies,
05:05dark matter can't do any of that.
05:07It doesn't bump into itself or radiate heat.
05:10But it can still form big, invisible clumps, which we call dark matter halos.
05:15In the early stages of the universe, the halos acted like gravity wells.
05:19They pulled in normal matter, which sank into the centers of those halos and formed the first galaxies.
05:26So, galaxies like the Milky Way or Andromeda might be sitting inside enormous blobs of dark matter that we just can't see.
05:34So, cosmic asymmetry explained?
05:37Eh, not yet.
05:38Scientists are sure that dwarf galaxies are some of the most dark matter-dominated objects in the universe.
05:43In many cases, over 99% of their mass is likely to be dark matter.
05:49That means they give us a unique chance to study dark matter without all the messy gas and stars that exist in larger galaxies.
05:57Researchers use dwarf galaxies to figure out how dark matter clumps together,
06:01or whether there are alternative theories of dark matter, like warm or self-interacting dark matter.
06:06At the moment, the main theory is that dark matter behaves like a cold, clumpy, and slow-moving fluid.
06:14At the same time, it might not be totally cold.
06:18Maybe it has other properties.
06:19Maybe it interacts with itself or with normal matter in subtle ways we haven't discovered yet.
06:25If that's true, it could help explain why satellite galaxies form in strange patterns, like the ones around Andromeda.
06:32In other words, the Lambda-CDM model might indeed have flaws.
06:37According to it, thousands of dwarf galaxies should be orbiting around larger galaxies like the Milky Way and Andromeda.
06:44But we only see a few dozen.
06:47This is known as the missing satellites problem.
06:50There are other puzzles, too.
06:52For example, Lambda-CDM predicts that dark matter halos should be the densest at the center,
06:57but many dwarf galaxies seem to have cores of their own.
07:01Plus, dwarf satellites around galaxies like Andromeda and the Milky Way seem to lie in thin, co-rotating planes.
07:09And it's something extremely rare in Lambda-CDM simulations.
07:13And finally, some simulated dark matter halos are so massive that they should form bright dwarf galaxies.
07:19But we don't see them.
07:22No wonder astronomers are so interested in dwarf galaxies and the explanation of cosmic asymmetry.
07:27For that, we need more precise measurements of their motions and structures
07:32and simulations that add more realistic physics, like stellar feedback, turbulence, and so on.
07:38Plus, we gotta search for new dwarf galaxies in the local group and beyond,
07:43using better telescopes and deeper surveys.
07:46Now, getting back to Andromeda's weirdly positioned satellites.
07:49If the dark matter theory doesn't work out, there's another possibility that involves large-scale interactions between galaxies.
07:57It could be an old collision or near-miss that shape the current distribution of satellites.
08:03For example, some scientists think a smaller galaxy, Messier 32, might have collided with Andromeda long ago, stirring things up.
08:12Scientists have seen some lopsided shapes in other galaxies before.
08:16But none is weird as what's going on around Andromeda.
08:20Usually, the little galaxies around big ones spread out pretty evenly or are just a bit off.
08:26That makes scientists think Andromeda might be a super-special case.
08:30They say we need to keep looking, using better telescopes to crack the Andromeda galaxy mystery.
08:36And, perhaps, after figuring out the truth, we'll also come closer to solving the dark matter problem.
08:47That's it for today.
08:49So, hey, if you pacified your curiosity, then give the video a like and share it with your friends.
08:54Or, if you want more, just click on these videos and stay on the bright side!

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