What Factors Influence the Density of a Hydrogen Cloud in Space?

In summary: The pressure is balanced by the gravitational force, so that's why the density decreases as you go outward from the center. You can use the ideal gas law to relate pressure, density, and temperature. In summary, the density of a hydrogen cloud in space depends on the mass of the cloud and the distance from the center. The free-fall time of a particle in this cloud is independent of its distance from the center, but this only holds true for a cloud with constant density. In reality, the density decreases as you move outward from the center due to the balance between pressure and gravity. To determine the density of hydrogen, one must take into account the external pressure and use the ideal gas law.
  • #1
BOAS
552
19
Hi,

I wanted to ask, what does the density of a hydrogen cloud in space depend upon?

That might be a silly question given the definition of density, but here's the context;

Considering a particle at rest within a molecular cloud at radius [itex]r[/itex] from the centre, I have shown that the acceleration this particle feels is approximately [itex]a \approx \frac{Gm}{r^{2}} \approx \frac{4 \pi G \rho r}{3}[/itex] (from mass being density x volume).

Using the equations of motion for constant acceleration I have determined that the 'free fall' time of this particle is independent of [itex]r[/itex] and can be approximated by [itex]t \approx \frac{1}{\sqrt{G \rho}}[/itex].

Two questions;

Why is this time independent of the particles distance from the center?

How do you determine the density of hydrogen when the external pressure is presumably close to zero?

Thanks!
 
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  • #2
Thanks for the post! Sorry you aren't generating responses at the moment. Do you have any further information, come to any new conclusions or is it possible to reword the post?
 
  • #3
The free-fall time is only constant for constant density. You can get this from Kepler's 3rd law t2~r3/m.(the square of the orbital period is proportional to the cube of the radius divided by the enclosed mass). Since for a constant density m~r3, this means that t=const.

A cloud with constant density would be gravitationally unstable though, In hydrodynamic equilibrium, the cloud density decreases like 1/r2. In that case, m~r (not ~r3), so that t2~r3/m ~ r2 i.e. t~r
 
  • #4
BOAS said:
Why is this time independent of the particles distance from the center?
Because at larger r, there is more mass that is pulling the particle inward, so the force is greater in a way that ends up being proportional to r-- just like a simple harmonic oscillator (for which the time is also independent of r).
How do you determine the density of hydrogen when the external pressure is presumably close to zero?
You need to use the external pressure-- the pressure in the interstellar medium is not zero.
 
  • #5


Hello,

Thank you for your questions about the density of a hydrogen cloud in space. The density of a hydrogen cloud depends on various factors such as the initial conditions of the cloud, its temperature, and the surrounding environment. The initial conditions of the cloud, including its mass and size, will determine the overall density. The temperature of the cloud can also affect its density, as hotter clouds tend to have lower densities. Additionally, the surrounding environment, such as the presence of other nearby clouds or the influence of a nearby star, can also impact the density of the hydrogen cloud.

To address your first question, the free fall time of a particle within a molecular cloud is independent of its distance from the center because of the nature of gravitational acceleration. According to Newton's law of gravitation, the force of gravity between two objects is inversely proportional to the square of the distance between them. This means that as the particle moves closer to the center of the cloud, the force of gravity increases, but at the same time, the distance squared decreases. These two effects cancel each other out, resulting in a constant acceleration and therefore a constant free fall time.

As for your second question, the density of hydrogen in a cloud can be determined using various methods, such as spectroscopy or measuring the cloud's mass and volume. However, in the context of your equation, the density is determined by the external pressure, which is likely close to zero in a hydrogen cloud in space. This is because the pressure within a cloud is primarily due to the weight of the gas above it, and in space, there is no significant weight or pressure from the surrounding environment. Therefore, the density of a hydrogen cloud in space is primarily determined by its own mass and volume.

I hope this helps answer your questions about the density of a hydrogen cloud in space. If you have any further inquiries, please do not hesitate to ask.

Best regards,
 

Related to What Factors Influence the Density of a Hydrogen Cloud in Space?

1. What is the density of a hydrogen cloud?

The density of a hydrogen cloud can vary greatly depending on its size and location, but on average it is estimated to be around 10,000 hydrogen atoms per cubic centimeter.

2. How is the density of a hydrogen cloud measured?

The density of a hydrogen cloud is typically measured using spectroscopic techniques, where the light emitted or absorbed by the cloud is analyzed to determine the number of hydrogen atoms present per unit volume.

3. What factors can affect the density of a hydrogen cloud?

The density of a hydrogen cloud can be influenced by various factors such as temperature, pressure, and the presence of other elements or molecules. Gravitational forces can also play a role in shaping the density of a cloud.

4. Can the density of a hydrogen cloud change over time?

Yes, the density of a hydrogen cloud can change over time as the cloud evolves and interacts with its surroundings. Factors such as gas flows, stellar activity, and mergers with other clouds can all impact the density of a hydrogen cloud.

5. What is the significance of studying the density of hydrogen clouds?

Studying the density of hydrogen clouds can provide valuable insights into the formation and evolution of galaxies, stars, and planets. It can also help us better understand the physical processes that occur within these structures, such as star formation and chemical enrichment.

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