Interstellar Dust: Extinction & Photon Ratio

In summary, the conversation discusses the density of interstellar dust in the galaxy and how it varies along the vertical direction. The given equation shows that the density decreases as the distance from the plane of the galaxy increases. The task is to find the extinction to an object in the galactic center, 8 kpc away, and the ratio of the number of photons before and after the extinction. The net extinction perpendicular to the galactic plane is given as 0.4 magnitudes. The symbols (phi) and (psi) represent (o) and (k) respectively.
  • #1
randa177
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1

Homework Statement



Suppose that the density of interstellar dust is uniform along the direction of the plane of the galaxy, but that its vertical density is given approximately by

[tex]\rho[/tex] = [tex]\rho[/tex] [tex]\o[/tex] exp - ( z / 0.15 )^2

where z is the distance from the plane of our galaxy in kpc. If the net extinction perpendicular to the galactic plane is 0.4 magnitudes (i.e. integrated from the mid-plane to infinity), find the extinction to an object in the galactic center, 8 kc away (and where z=0), and the ratio of the number of photons before and after the extinction


Homework Equations



Please see attachment

The Attempt at a Solution



I am very confused, no clue!
 

Attachments

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  • #2
Here the (phi) symbol stands for (o)
 

1. What is interstellar dust and how does it affect light?

Interstellar dust refers to the small particles, typically less than 1 micrometer in size, that exist in the space between stars. These particles can absorb, scatter, and reflect light, leading to a phenomenon known as extinction, where the intensity of light decreases as it travels through the dust. This can impact our ability to observe and study distant objects in space.

2. How does the extinction of light due to interstellar dust vary across different wavelengths?

The amount of extinction caused by interstellar dust depends on the wavelength of light. Shorter wavelengths, such as ultraviolet and blue light, are more easily scattered and absorbed by dust particles, resulting in a greater amount of extinction compared to longer wavelengths like infrared. This is known as the "extinction curve" and is an important factor to consider when studying objects in space.

3. What causes the variation in the ratio of photon counts from distant objects?

The number of photons, or particles of light, received from distant objects can vary due to the effects of interstellar dust. As light travels through the dust, some photons may be scattered or absorbed, leading to a decrease in the overall number of photons received. This can also result in a change in the color or spectrum of the light, making it appear different from its original source.

4. How do scientists study interstellar dust and its effects on light?

Scientists use a variety of methods to study interstellar dust and its impact on light. One common approach is to analyze the spectrum of light from distant objects, which can reveal the presence of certain elements that are known to exist in interstellar dust. Other techniques include using computer models and simulations to understand the behavior of dust particles and their effects on light.

5. What are the implications of interstellar dust on our understanding of the universe?

The presence of interstellar dust can have significant implications for our understanding of the universe. It can affect our ability to observe and study distant objects, leading to potential biases in our data and interpretations. Additionally, the composition and behavior of interstellar dust can provide valuable insights into the formation and evolution of galaxies and other structures in the universe.

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