# Density of stars near the center of the Milky Way

At night, I can look up and see the Milky Way across the sky. My question is, supposing our solar system was, instead of way out on an 'arm' of the galaxy, if we were near the galactic center. Would the night sky be much brighter?? If so, how close would we have to be to never have darkness of night??

Thanks!

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this might be better answered on the "physics" stack exchange – Dale Oct 2 '11 at 4:17
@Joe This question is astronomy! Would You expect a physicist to know about star/dust density in the center? – Georg Oct 3 '11 at 11:20
I just got through an episode of science.discovery.com/convergence/cosmos/cosmos.html were one of the scientists talked about if you were on a planet closer to the middle it would basically be daylight all the time from all the stars. If you are actually close to the galactic center you would get sucked into a black hole! – polynomial Oct 5 '11 at 0:19

In the solar neighborhood, the stellar density is about one star per cubic parsec (one parsec is 3.26 light-years). At the Galactic core, around 100 parsecs from the Galactic center, the stellar density has risen to 100 per cubic parsec, crowded together because of gravity.

So we'd see about 100 times as many stars as we see now, and the nearest star would most likely be less than 1 light-year away (compared to 4.3 light-years for Alpha Centauri).

This Wikipedia article says the stellar density near the Sun is only 0.14 stars per cubic parsec; it doesn't give a figure for the Galactic core. (If somebody has more information, please comment or edit.)

According to this Wikipedia article, the total integrated magnitude of the night sky as seen from Earth is -6.5. Making that 100 times as bright produces a total magnitude of -11.5 (5 magnitudes is a factor of 100 in brightness). The maximum brightness of the full Moon is -12.92.

So even with 100 times as many stars in the sky, the total brightness would be substantially less than that of a full moon.

(This assumes that the average brightness of the core stars is similar to the average brightness out here in the Galactic suburbs.)

The stars might be more dense close to the center, but I don't think you'd really want to be closer than 100 parsecs.

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Thanks so much! Unfortunately, your first link is currently broken. Is there a paper somewhere that would help me generate a 3D plot of the density of stars in the Milky Way? – theJollySin Feb 26 '13 at 6:58
@theJollySin: Not really. I've updated my answer with a link to a Wikipedia article that gives different figures. – Keith Thompson Feb 26 '13 at 15:53

Okay the notion that the sky would be 100 times brighter because there are 100 more stars within a cubic parsec is ludicrous. First it would discount the 100x 100 more stars that would lie within the next parsecs distance from us. More importantly it discounts the far closer proximity of the stars within our Parsec. With 100 stars within our particular cubic parsec odds are one would be just outside of our solar envelope... heck one very possibly would be closer than Planet 9!

Could you imagine if Betelgeuse was a solar month away! The answer is in the galactic bulge you would never need a flashlight but bring SPF1,000,000 !

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