Spectrum of hot gas uniformly mixed with dust

In summary: It's important to consider the effects of dust on the light spectrum, as it can cause dimming and a redder appearance. However, more information about the dust would be helpful for a more accurate drawing. Additionally, assuming everything is a sphere can make the drawing easier, but may not give the most precise results.
  • #1
starstruck_
185
8
hey!

EDIT: I didn’t post this in homework help because there aren’t any computational questions, it’s just conceptual

My assignment scenario consists of a star (blackbody) surrounded by an expanding shell of hot gas. I’m given its spectrum and it is a continuous emission spectrum. Emission due to the hot gas and continuous due to the blackbody hidden behind the hot gas.

Now I’m told to assume that dust has been uniformly mixed into the shell of hot gas. I have to draw the spectrum for this scenario. (I’m not sure if I did this right. I’m probably misreading the graph. )I know that blue light is scattered more than red and the light would dim because I’d the dust.

I did drew a continuous spectrum, however I lowered the peak and the blue wavelength (left) side of the spectrum as well as the red wavelength side of the spectrum, however the red side was higher than the blue side.

The darker line is what I drew, and the lighter one is what I was given. I’m almost certain this is incorrect because I don’t really understand what dust does to spectra.
 

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  • #2
Dust particles adsorb (or scatter) wavelengths that are shorter than the diameter of the dust grain. The question should have more information about the dust.

A coffee mug can block visual radiation and 10 cm radiation. 1 m radiation passes it. A sphere of coffee mugs will have a slight anomaly because the handles block extra 3cm radiation. Glass beer mugs would be similar to the coffee mugs but let visual light through. You can get away with assuming everything is a sphere.

starstruck_ said:
hey!

EDIT: I didn’t post this in homework help because there aren’t any computational questions, it’s just conceptual

My assignment scenario consists ...

This is clearly a homework question.
 
  • #3
starstruck_ said:
The darker line is what I drew, and the lighter one is what I was given. I’m almost certain this is incorrect because I don’t really understand what dust does to spectra.

What does your book or lecture notes say about what effect the dust has?
 
  • #4
Drakkith said:
What does your book or lecture notes say about what effect the dust has?

All my lecture notes say is that dust would dim the light and make it appear redder. Due to this, I first drew my spectrum redshifted, confusing colour with the redshift (oops) but then my professor said to think about what happens to light in dust. My lecture notes also say that dust scatters blue light so I drew the whole spectrum with less flux (dimmer) and then made the blue wavelength side of my spectrum smaller than the red wavelength side (or at least I tried to) and have no idea if this was right.

We don’t have a book for the course, just lecture notes.

It doesn’t say the dust was cool so I assumed no absorption spectra.
 
  • #5
stefan r said:
Dust particles adsorb (or scatter) wavelengths that are shorter than the diameter of the dust grain. The question should have more information about the dust.

A coffee mug can block visual radiation and 10 cm radiation. 1 m radiation passes it. A sphere of coffee mugs will have a slight anomaly because the handles block extra 3cm radiation. Glass beer mugs would be similar to the coffee mugs but let visual light through. You can get away with assuming everything is a sphere.
This is clearly a homework question.

There was no other information besides that it was uniformly mixed into the expanding shell of hot gas
 
  • #6
starstruck_ said:
All my lecture notes say is that dust would dim the light and make it appear redder. Due to this, I first drew my spectrum redshifted, confusing colour with the redshift (oops) but then my professor said to think about what happens to light in dust. My lecture notes also say that dust scatters blue light so I drew the whole spectrum with less flux (dimmer) and then made the blue wavelength side of my spectrum smaller than the red wavelength side (or at least I tried to) and have no idea if this was right.

We don’t have a book for the course, just lecture notes.

It doesn’t say the dust was cool so I assumed no absorption spectra.

That looks correct to me, and seems to match up with what your lecture notes say.
 
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1. What is the spectrum of hot gas uniformly mixed with dust?

The spectrum of hot gas uniformly mixed with dust refers to the range of electromagnetic radiation emitted by a mixture of hot gas and dust. This spectrum can include wavelengths from radio waves to X-rays.

2. How is the spectrum of hot gas uniformly mixed with dust produced?

The spectrum of hot gas uniformly mixed with dust is produced when the gas and dust are heated to high temperatures, causing them to emit electromagnetic radiation. This radiation is a result of the atoms and molecules in the gas and dust being excited by the heat.

3. What can we learn from studying the spectrum of hot gas uniformly mixed with dust?

Studying the spectrum of hot gas uniformly mixed with dust can provide valuable information about the composition, density, and temperature of the gas and dust. It can also give insights into the physical processes occurring in the region where the mixture is present.

4. How is the spectrum of hot gas uniformly mixed with dust measured?

The spectrum of hot gas uniformly mixed with dust is typically measured using specialized instruments such as spectrometers, which can detect and analyze the different wavelengths of electromagnetic radiation emitted by the mixture. This data is then used to create a visual representation of the spectrum.

5. What are some examples of where hot gas uniformly mixed with dust can be found?

Hot gas uniformly mixed with dust can be found in various environments, such as the interstellar medium, supernova remnants, and active galactic nuclei. It can also be present in laboratory settings, such as in plasma chambers used for research and experiments.

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