Observing O-type Stars: Easier at 1 or 7 Microm?

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In summary, the extinction of light passing through a partially opaque medium can be calculated using Beer's Law. The intensity of light before and after the medium is denoted by Io and I, respectively, while T represents the optical depth of the medium. The ease of detecting an O-type star embedded in a molecular cloud at either 1 microm or 7 microm depends on the wavelength and absorption properties of the cloud.
  • #1
randa177
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Does anybody have any idea how to solve this problem:

The extinction of light due to its passage through a partially opaque medium is given by Beer’s Law (known by most chemistry students and many physics students, I hope!):

I = Io e^ T

where (Io) is the intensity of the light incident on the medium and (I) is the intensity after exiting the medium. (T) is the “optical depth” of the medium.

Suppose you were observing an O-type star embedded in a molecular cloud and the optical depth at 7 microm was 1. Everything else being equal (detector technology etc.) would it be easier to detect the star at 1 microm or 7 microm?
 
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T depends on the wavelength and on the wavelength-dependent absorption properties of the cloud, so there is no single answer to the question.
 

1. What are O-type stars?

O-type stars are massive and luminous stars that are classified as spectral type O on the Morgan-Keenan system. They are typically found in the spiral arms of galaxies and have high surface temperatures, making them appear blue in color.

2. Why is observing O-type stars important?

O-type stars are important because they are the most massive and luminous stars in the universe. They play a crucial role in the evolution of galaxies and are key indicators of the chemical composition and dynamics of their host galaxies.

3. What does it mean to observe O-type stars at 1 or 7 microm?

Observing O-type stars at 1 or 7 microm refers to using infrared telescopes to study these stars. Infrared light has longer wavelengths than visible light, allowing us to see through the gas and dust that typically surround O-type stars and obtain clearer observations.

4. Is it easier to observe O-type stars at 1 or 7 microm?

It is generally easier to observe O-type stars at 7 microm. This is because at this longer wavelength, the stars emit more infrared radiation, making them easier to detect and study. Additionally, at 1 microm, the stars may be heavily obscured by gas and dust, making it more difficult to obtain clear observations.

5. What can we learn from observing O-type stars at 1 or 7 microm?

Observing O-type stars at 1 or 7 microm can provide valuable insights into their physical properties, such as their temperature, luminosity, and chemical composition. It can also help us better understand the processes involved in their formation and evolution, as well as the impact they have on their surrounding environments.

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