A body intermediate to stars and galaxies

In summary, the largest star and smallest galaxy formed from primordial materials are no longer observable, with the largest star lasting only about 100 million years before exploding. However, enormous primordial stars are thought to have been abundant and played a role in galaxy formation. Other larger objects were not able to form due to the isothermal collapse of protogalactic clouds, leading to fragmentation and the formation of stars.
  • #1
Loren Booda
3,125
4
Out of the primordial hydrogen, what were the largest star and smallest galaxy that eventually formed?
 
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  • #2
Who can say? According to the BB model, the largest star formed from primordial materials (it is assumed that the BB created more than just Hydrogen, by the way) is LONG since gone, and the smallest galaxy ( if it still exists) is undetectable due to low luminosity.
 
  • #3
Enormous primordial stars [>200 solar masses] are thought to have been very abundant. Large numbers of early supernova are needed to explain reionization, primordial metallicity and create the black hole seeds responsible for quasars. These behemoths would only last around 100 million years before detonating. The earliest large structures were probably globular clusters. They apparently play a role in galaxy formation.
 
  • #4
Apart from these big primordial population III stars, I do not see how larger objects could actually have formed. Immediately after decoupling, the Jeans mass is about 105 solar masses (the mass of globular clusters, as Chronos mentioned). This structures will be the first protogalactic clouds, which will merge and cluster. However, the formation of a massive body (assuming you had that in mind) on such a scale is actually not possible, since it takes place isothermal collapse of the cloud, which leads the Jeans mass to decrease (density increase), and produces fragmentation into smaller clouds. When the cooling of the cloud is not longer possible, the temperature does not longer remain constant and this process is stopped, leading to the formation of stars.
 
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1. What is a body intermediate to stars and galaxies?

A body intermediate to stars and galaxies is a celestial object that falls between the size and mass of a star and a galaxy. It is smaller than a galaxy, but larger than a star, and often has its own system of orbiting bodies.

2. How are bodies intermediate to stars and galaxies formed?

These bodies are typically formed through the collapse of a large molecular cloud. As the cloud collapses, smaller clumps break off and form into stars, while the larger clumps form into intermediate bodies.

3. What are some examples of bodies intermediate to stars and galaxies?

Some examples include globular clusters, dwarf galaxies, and brown dwarfs. These objects have a range of sizes and masses, but all fall between the size and mass of a star and a galaxy.

4. What is the significance of studying bodies intermediate to stars and galaxies?

Studying these objects can provide valuable insights into the formation and evolution of galaxies. They can also help us understand the processes that lead to the formation of stars and planets.

5. How do scientists observe bodies intermediate to stars and galaxies?

Scientists use a variety of tools, such as telescopes and satellites, to observe these objects. They also study the light emitted by these bodies to gather information about their composition and characteristics.

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