Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Local Group
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
== Future == The galaxies of the Local Group are likely to merge together under their own mutual gravitational attractions over a timescale of [[Timeline of the far future|tens of billions of years]] into a single elliptical galaxy, with the [[Andromeda–Milky Way collision|coalescence of Andromeda and the Milky Way]] being the predominant event in this process.<ref>{{cite journal | author= Fred C. Adams | author2= Gregory Laughlin | title=A dying universe: the long-term fate and evolution of astrophysical objects | journal=Reviews of Modern Physics | date=1997 | volume=69 | issue=2 | pages=337–372 | bibcode=1997RvMP...69..337A | doi=10.1103/RevModPhys.69.337 | arxiv=astro-ph/9701131 | s2cid= 12173790 }}</ref> [[File:Andromeda and Milky Way collision.ogv|thumb|upright=1.5|A [[NASA]] conception of the collision using [[computer-generated imagery]]]]
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)