Credit & Copyright: Malcolm Park  
(North York Astronomical Association)  
  
  
Explanation:
Separated by about 14 degrees  
(28 Full Moons) in planet Earth's sky,  
spiral galaxies M31 at left, and M33 are both large members of  
the Local  
Group, along with our own Milky Way galaxy.  
  
This narrow- and wide-angle,  
multi-camera  
composite finds details of spiral structure  
in both, while the massive neighboring galaxies seem to be balanced  
in starry fields either side of  
bright Mirach, beta star in  
the constellation Andromeda.  
  
Mirach is just 200 light-years from the Sun.  
  
But M31, the Andromeda Galaxy,  
is really 2.5 million light-years distant and  
M33, the Triangulum Galaxy, is also about  
3 million light years away.  
  
Although they look far apart,   
M31 and M33 are engaged in a gravitational struggle.  
  
In fact, radio astronomers have  
found indications of  
a bridge of neutral hydrogen gas that could connect the two,  
evidence of a closer encounter in the past.  
  
Based on measurements, gravitational  
simulations currently  
predict that the Milky Way, M31, and M33  
will all undergo mutual close encounters and potentially  
mergers, billions of years  
in the future.  
  
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Публикации с ключевыми словами:
M 31 - M 33
 Публикации со словами: M 31 - M 33  | |
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