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Current Map of the Milky Way (or at least a part of it)


Argylas

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I've tried to find a current map of the Milky Way or at least a small part of it, but to no avail. That is why I wanted to ask if someone here has stumbled over something like this.

Let me clarify - I don't mean a map of our galaxy as we observe it right now, as this would only be a collection of snapshots from the past (depending on the distance of each star to us). What I want to find is a map of some part of the galaxy, in which the position of all objects is extrapolated to their current coordinates. I know this requires a very difficult model simulation, but someone somewhere should have done it at least for the local group of stars near our Solar system. As all star orbit the center of the galaxy and have different velocities and orbits, they should be changing their position with regards to our sun. So even a star as close as Procyon (~ 11 light years) should be in a different position with regards to the Solar system 11 years from what we see today.

I know they have done it for the movement of the Andromeda galaxy and have seen that it will collide with the Milky Way in about 4 bln. years. So it should be doable. So if you have come upon something similar to what I am searching for, I would be deeply gratified if you share it with me. :)

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We don't know the motion of all those stars (but perhaps the general arms).

So just rotate the picture by enough. ;)

Else it's only 100,000 light years across. Look at geology as an example, that time-scale is not much, and you might get bigger mountains, smaller rivers or some change in sea level. But most of the interesting locat stuff is unpredictable (collapses, super dam floods, like in the Mediterranean sea etc).

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There's the bulge to fight through, if you want to get to the other side... You can take a look on Hipparcos catalogue and/or Tycho catalogue (from hipparcos satellite). Or wait for Gaia... To map, use spherical coordinate (r, θ, Æ) which θ is galactic latitude (l ; yes, the leter) and Æ is galactic longitude b. r is of course distance. Not sure what program to map through. HII regions should be slightly easier to map (distance is extrapolated from radial velocity assuming some models), but if you want to be accurate get the error bars in.

Regarding rotational speed, galactic rotation isn't keplerian nor rigid body; kind of horrible to graph and to think about as there should be some dark mass but if you think nearby star should zip fast enough, just think how much km you need for a star 1 pc (1 pc is precisely 206265 AU) so you'd notice it already moves half a degree (the width of Moon and Sun); most star velocity is below 100 km/s. Takes you hundreds of years; farther stars would take longer even if the speed is higher.

EDIT : if you wonder is it really slow, the Sun over it's lifetime (until now) has just revolved like 20 or 21 times. Very slow because a galaxy is simply enormous.

Edited by YNM
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