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It might be odd to get your head around, but galaxies can and do collide.
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But far from an wild party of death, galaxies collisions yield hotbeds for new star formation,
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leading astronomers to suspect that this not-so-violent event is actually a driving factor behind galactic evolution.
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The big question here is how can galaxies collide and not just destroy everything?
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It helps to think about what a galaxy really is.
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Every galaxy is made up of some 100 billion stars with planets orbiting their host stars,
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but those stars are really far apart.
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Take the Milky Way for example.
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We're about here on the edge of a spiral arm called Orion Spur.
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It looks crowded in our little neighborhood, but our nearest neighbor Alpha Centuri A, is actually 4.3 light years away.
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So galaxies might full of stars, but those stars are really far apart, meaning the likelihood of two hitting is pretty low.
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But that doesn't mean nothing happens, because there is stuff in those vast distances.
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The “space” between stars is actually full of gas and dust.
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Within these regions are dense pockets of interstellar material, called molecular clouds,
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that collapse under their own mass and gravity, forming protostars and eventually new stars.
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When galaxies collide, it's this material — the interstellar gas and dust — that
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interacts gravitationally with some neat results.
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In a collision, one galaxy can rip material from another, disrupting star formation and
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adding more material to its own molecular clouds.
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A direct collision between these gases can also result in shockwaves reverberating through
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both galaxies, triggering new regions of star formation where there wasn't any before.
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Aside from generating new pockets of star formation, both close passes and full-on collisions
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cause gravitational interactions begetting interesting changes, causing spiral arms, tidal tails, and even rings.
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Two spiral galaxies could merge and form an elliptical galaxy with more active star formation than either had before.
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But it's not like this happens overnight… not that there's a “night” where galaxies are concerned.
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This process can take millions of years.
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Which is a good thing because our own Milky Way is on a crash course with the Andromeda galaxy, but we've got a good 4 billion years…
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That should be enough time to live my best life.
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If you want more cosmic science in your feed be sure to subscribe to Seeker.
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And if you want to know what happens when galaxies die, Trace has more on that right here.
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You know what'd be awesome?
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If after the Andromeda collision our sky lit up with tons of newly forming stars!