Celestial hemisphere:  Northern  ·  Constellation: Serpens (Ser)  ·  Contains:  5 Ser  ·  IC 4537  ·  M 5  ·  NGC 5904  ·  The star 5Ser
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Messier 5, Alex Woronow
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Messier 5

Getting plate-solving status, please wait...
Messier 5, Alex Woronow
Powered byPixInsight

Messier 5

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Description

Messier 5

OTA: TAO 150 (f/7.3)

Camera: FLI - ML16200 (1.13 arcseconds/pixel)

Observatory: Deep Sky West, Chile

EXPOSURES:

Red: 27 x 600 sec.

Blue: 12 x 600

Green: 14 x 600

L: 23 x 600

Total exposure 12 hours

Image Width: ~52 arcminutes

Processed by Alex Woronow (2020) using PixInsight, Skylum, SWT

Globular clusters predominantly host old stars. Messier 5 is among the oldest known globular clusters in the Milky Way. GC’s tend to have very little associated gas and dust and, therefore, very no significant active star-formation. It is thought that all the stars in a given GC were born at approximately the same time, and, therefore have about the same ages. Because massive stars burn their fuels fastest, they have long since depleted their fuels and vanished in supernovae explosions. The remaining stars are mostly low-mass and old. M 5 has a few stars younger than the 12 billion-year age of the cluster, probably born from the debris of the supernovae or through star-star collisions. These stars are labeled as “blue stragglers.” All totaled, M 5 has over 100,000 stars--perhaps even 6 times this minimum number.

Globular clusters generally occur outside of the main disk of a galaxy, in a halo around it. These dense, spherical star associations probably formed in areas of abnormally elevated gas densities. However, considerably uncertainty surrounds how GC’s arise--strangely, the more massive a galaxy’s central black hole, the more globular clusters the galaxy tends to have. Is it a correlation or a cause-and-effect?

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Messier 5, Alex Woronow