Why globular clusters don't collapse.

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  • #1
Jordi Heguilor
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I asked Bard that question and it responded (among other things) that a) globular clusters are spherical and b) that they are spinning rapidly. Aren't those two things contradictory, as in they should be flattened by centrifugal forces?
 
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If Bard is some sort ofg AI Chatbot, don't believe it.

Globular clusters are not rigid, so they do not rotate like rigid objects. Further, they are pressure supported, which means that the individual stars rotation parameters are fairly random, unlike spirals.
 
  • #3
openai gave a lot more considerations: (bound together by their mutual gravitational attraction.) Gravitational balance, Stellar Velocity Dispersion, mass segregation, tidal effects, a broad distribution of kinetic energies within the cluster, higher energy orbits, Stellar Collisions and re-balancing, mass loss and gravity reduction, dark matter gravitational attraction, high mass-to-light ratio, yet low contamination levels of gas, dust prevent mass clouds that promote collapse. May contain intermediate black holes.

Like rain drops with "like charges", stars repel each other
- while in random kinetic motion
- to contain 10k to 10m stars in a cluster from 3.2 ly across or 100 ly across and up.
- 150m clusters in Milky Way each very dense. Living inside a Globular Cluster
- from Fraser Cain: Publisher Universe Today ...
 
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  • #4
Jordi Heguilor said:
I asked Bard that question and it responded (among other things) that a) globular clusters are spherical and b) that they are spinning rapidly. Aren't those two things contradictory, as in they should be flattened by centrifugal forces?
Welcome to PF, Jordi. :smile:

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1. Why do globular clusters not collapse?

Globular clusters do not collapse because of a phenomenon known as "gravitational binding energy." This refers to the amount of energy that is required to pull the stars in a cluster apart. In globular clusters, the gravitational binding energy is strong enough to counteract the force of gravity pulling the stars towards the center, preventing them from collapsing.

2. How do globular clusters maintain their shape?

Globular clusters maintain their shape through a balance between gravity and the centrifugal force caused by the collective motion of the stars within the cluster. The gravitational force pulls the stars towards the center, while the centrifugal force pushes them away. As long as these forces are balanced, the cluster will maintain its shape.

3. What role do dark matter and black holes play in preventing globular clusters from collapsing?

Dark matter and black holes play a significant role in preventing globular clusters from collapsing. Dark matter, which is invisible and does not interact with light, provides additional gravitational pull that helps to stabilize the cluster. Black holes, which are extremely dense and have strong gravitational pull, also contribute to the overall gravitational binding energy of the cluster.

4. Do all globular clusters have the same lifespan?

No, not all globular clusters have the same lifespan. The lifespan of a globular cluster depends on several factors, such as its mass, density, and distance from the center of its galaxy. Generally, larger and denser clusters have shorter lifespans, while smaller and less dense clusters can survive for billions of years.

5. Can globular clusters eventually collapse?

While globular clusters are stable and long-lasting structures, they can eventually collapse due to a process known as "core collapse." This occurs when the central region of the cluster becomes more densely packed with stars, increasing the gravitational pull and causing the cluster to shrink. However, this process can take billions of years to occur, and some clusters may never experience core collapse.

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