Why Do Globular Clusters Maintain Their Shape Over Billions of Years?

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SUMMARY

Globular clusters, among the oldest structures in the galactic halo, have maintained their shape over approximately 10 billion years due to the predominance of lower mass stars, which do not undergo supernova explosions. Instead of being destroyed, these clusters experience a process called "core collapse," where the central region becomes denser while the outer parts become less dense. This process occurs over a timescale significantly longer than the age of the clusters, allowing them to retain their spherical shape, which is the minimum energy configuration for gravitationally bound systems.

PREREQUISITES
  • Understanding of stellar evolution, particularly the life cycles of massive and low-mass stars.
  • Familiarity with gravitational dynamics and the concept of energy configurations in astrophysics.
  • Knowledge of core collapse phenomena in globular clusters.
  • Basic comprehension of the structure and formation of the Milky Way galaxy.
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  • Research the life cycle of stars, focusing on the differences between massive stars and low-mass stars.
  • Explore the mechanics of gravitational dynamics and how they influence the shape of celestial bodies.
  • Investigate the process of core collapse in globular clusters and its implications for stellar evolution.
  • Study the formation and evolution of the Milky Way galaxy to understand the context of globular clusters.
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in the dynamics of stellar clusters and the evolution of the Milky Way galaxy will benefit from this discussion.

Eridanus1
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they are the oldest things in the galactic halo, having formed near the birth of the milky way. So with all the 10 odd billions of years of existence, i think they all should have gone supernova and destroyed the shape of the cluster.

So how do they stay gloubular in their shape?
 
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(1) Only large stars explode as a supernova. Less massive stars like our sun and smaller do not do this (e.g., our sun will swell to a red giant, becoming a "planetary nebula" and then shrink to a white dwarf). Large stars are also short-lived. So, such ancient star clusters contain lots of lower mass (longer lived) stars.

(2) It's not much of a "shape" to begin with. It's a collection of stars held by each other's gravity (like a mini-galaxy). The shape is constantly changing anyway.
 
Eridanus1 said:
they are the oldest things in the galactic halo, having formed near the birth of the milky way. So with all the 10 odd billions of years of existence, i think they all should have gone supernova and destroyed the shape of the cluster.

As was already said, this is not an issue. However, globular clusters do undergo a process known as "core collapse", in which the central part gets ever denser with time and the outer parts get less dense. The end result of this process is that the cluster dissipates, but for most globular clusters, this timescale for it is much longer than 10 billion years.


So how do they stay gloubular in their shape?

It turns out that for a group of objects moving under the influence of gravity, the minimum energy configuration (and, therefore, the preferred one) is spherical...unless it has a significant amount of rotation, then it goes to a disk.
 

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