Distribution of radial velocities in a gas

In summary, the lecturer discussed a gas with particles that have a random direction of absolute velocity v. When observing this gas from a far distance, only the radial velocities of the particles can be seen, resulting in a distribution of velocities in the range of [-v,v]. The question of what this observed distribution would be, with the most prominent velocity, was raised. The lecturer claimed that it would be a uniform curve, but this was stated quickly and without explanation. It was proposed that all particles have the same velocity v, forming a sphere, and when viewed from far away, one coordinate can be chosen as the observed direction. The surface area as a function of this coordinate can be determined using a formula.
  • #1
Arnoldas
2
0
The lecturer did not explain this for some reason.

Assuming that we have a gass where all the particles have a certain absolute velocity v. Directions of v vector are random though, giving velocity vector a uniform direction distribution. That means that a velocity vector of any random particle has equal probability to point in any direction. But what if we observe this gas from a very far distance ( like atmosphere of a star): we can then only observe the radial velocities of particles. That means that we would observe all velocities in the interval [-v,v]. But the question is what would be the distribution that we would observe (particles per velocity curve)? for example which velocity would be most prominent? Would it also be a uniform curve?-thats what lecturer claimed in haste.
 
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  • #2
All have the same velocity v? Then their velocity vectors form a sphere, and "seen from far away" you can pick one coordinate as your "observed direction". Then you just have to find the surface area as function of this coordinate, which is a formula you can look up (or derive yourself).
 
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What is the distribution of radial velocities in a gas?

The distribution of radial velocities in a gas refers to the spread of velocities of gas particles moving towards or away from a central point, such as a star or galaxy. This distribution is typically described by a Gaussian or Maxwell-Boltzmann distribution.

How is the distribution of radial velocities measured?

The distribution of radial velocities is measured using spectroscopy, specifically the Doppler effect. By analyzing the shifts in the wavelengths of spectral lines, scientists can determine the velocities of gas particles along the line of sight.

What factors can affect the distribution of radial velocities in a gas?

The distribution of radial velocities in a gas can be affected by various factors such as temperature, pressure, and the presence of other nearby objects. These factors can influence the speeds and directions of gas particles, leading to changes in the distribution.

Why is the distribution of radial velocities important in astrophysics?

The distribution of radial velocities plays a crucial role in understanding the dynamics of celestial objects, such as stars and galaxies. It provides insight into their formation, evolution, and interactions with other objects in the universe.

Can the distribution of radial velocities be used to detect exoplanets?

Yes, the distribution of radial velocities can be used to detect exoplanets orbiting a star. As a planet orbits its star, it causes a slight wobble, resulting in periodic changes in the star's radial velocity. By measuring these changes, scientists can infer the presence and properties of an exoplanet.

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