Celestial hemisphere:  Northern  ·  Constellation: Coma Berenices (Com)  ·  Contains:  HD114762  ·  HD114881  ·  M 53  ·  NGC 5024  ·  NGC 5053
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M53 & NGC 5053 RGB, Randy Lindstrom
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M53 & NGC 5053 RGB

Getting plate-solving status, please wait...
M53 & NGC 5053 RGB, Randy Lindstrom
Powered byPixInsight

M53 & NGC 5053 RGB

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Description

German astronomer, Johann Elert Bode discovered M53 in 1775. This 220 light year diameter ball of stars (in the upper right) is 60,000 light-years away, one of the most distant globular clusters from Earth within our galaxy.

Globular clusters are much older and larger than open clusters, such as NGC 5053 (to the lower left) so they are generally expected to contain more elderly, red stars and fewer young, blue stars. But Messier 53 has a surprising number of a type of star called blue stragglers. Blue stragglers appear to be brighter and more youthful than they should be. These unusual objects are probably formed by close encounters, possibly collisions, between stars in the crowded centers of globular clusters like M53.

A tidal bridge-like structure appears to connect M53 with its diffuse neighbor NGC 5053 about 6000 light years away. It suggests the pair may have interacted in the past — a possibly unique occurrence within the Milky Way as there are no other known binary clusters within the galaxy.

Sources: Wikipedia, Universe Today

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M53 & NGC 5053 RGB, Randy Lindstrom

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