A couple of years ago I started playing a game called Kerbal Space Program (KSP) and my understanding about how orbits actually work increased dramatically. Because of KSP I was looking at a picture of a galaxy with its spiral arms and something struck me as very odd. The stars closer in should orbit the galaxy center faster than the stars farther out and that would smear out these lanes of stars until they were no longer recognizable. Something weird is going on here!

So why do galaxies have arms? What's bunching these stars together like that?

I noticed that the center of galaxies are all smeared out and bulbous like I think that the rest should look like. So what if all that mass rotating around a common center is warping space around it, like the water draining down your sink, and this warping is what catching matter/stars into the lanes.

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    $\begingroup$ Welcome to the astronomy stack exchange and great first question! This was actually an unsolved problem in astronomy for a very long time, so you're not alone in wondering this. $\endgroup$
    – zephyr
    Oct 6, 2016 at 20:10
  • $\begingroup$ I think I recall reading something somewhere a long time ago that the answer lies with the interaction with dark matter and/or dark energy. I could be wrong. Like you, I am very green when it comes to astronomy and astrophysics. I'm just a casual layman with a natural curiosity. I've not even played KSP (although I've seen a few KSP vids on YouTube in the past). I'm sure someone way smarter than me on here can expound on this or debunk me. They might even throw in one of those cool looking, ridiculously complex equations you or I won't have a clue what it means. $\endgroup$
    – iMerchant
    Oct 7, 2016 at 1:56
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    $\begingroup$ Possible duplicate of Why do pictures of the Milky Way look like a spiral? $\endgroup$
    – James K
    Oct 7, 2016 at 5:20
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    $\begingroup$ @zephyr thanks for the point.Doing some research it looks to me that for a keplerian orbit to work as I was assuming all stars in the galaxy would have to be in the sphere of influence of the super massive back hole which they are not. So yes this assumption was the biggest problem. Im going to have to get over that line of thinking. $\endgroup$
    – Hal Clark
    Oct 7, 2016 at 19:16
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    $\begingroup$ Similar question with a nice answer here: astronomy.stackexchange.com/questions/6232/… $\endgroup$
    – userLTK
    Apr 26, 2018 at 6:07

1 Answer 1


The usual explanation of spiral arms involves density waves. Nonuniform motion leads to matter alternately bunching up (boosting star formation) and spreading out. Like cars on a congested road, stars move through regions of greater or lesser density over time. The rotational smearing you anticipate is known as the "winding problem." This Scientific American article offers three explanations by professional astronomers.

  • $\begingroup$ I found that article very very interesting. Thanks for the post. I did not know that I had incidentally stumbled on one of the most interesting ongoing topics in astronomy. $\endgroup$
    – Hal Clark
    Oct 7, 2016 at 18:42
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    $\begingroup$ It's really just gas that bunches up into arms, isn't it? What we see are the young large stars forming there. Most of them go supernova and disappear before they leave the high density regions in the arms. Small stars, which are invisible, are evenly distributed in the galactic disk, not concentrated to arms. Right? $\endgroup$
    – LocalFluff
    Oct 7, 2016 at 23:47
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    $\begingroup$ @LocalFluff -- No, there are density waves in the general population of older stars as well, though they're not as strong as the gas spiral arms. $\endgroup$ Oct 13, 2016 at 20:15

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