Astronomy Reflection nebula Question

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SUMMARY

The spectrum of a reflection nebula primarily exhibits a continuous spectrum similar to that of the illuminating star, rather than distinct absorption or emission lines. This occurs because the light is scattered and reflected by fine grains of dust within the nebula, which do not absorb specific wavelengths of light. The absence of spectral lines indicates that the light has not interacted significantly with the dust particles, maintaining the characteristics of the original starlight.

PREREQUISITES
  • Understanding of reflection nebulae and their properties
  • Knowledge of light scattering and reflection principles
  • Familiarity with stellar spectra and spectral lines
  • Basic concepts of astrophysics related to nebulae
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  • Research the properties of reflection nebulae and their formation
  • Study the differences between absorption and emission spectra
  • Explore the role of dust in astrophysical environments
  • Learn about the techniques used to analyze stellar spectra
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Astronomy students, astrophysicists, and educators interested in the properties of nebulae and stellar light interactions.

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Homework Statement



1. If you looked at the spectrum of a reflection nebula, would you see absorption lines, emission lines, or no lines? Explain your answer. As part of your explanation, describe how the spectrum demonstrates that the light was reflected from nearby stars.


Homework Equations



Quoted from my book:

"Reflection nebula- caused by fine grains of dust in a lower concentration than that found in dark nebulae. The light we see coming from the nebula is starlight that has been scattered and reflected by these dust grains."


The Attempt at a Solution



If the light is being reflected, does that mean there will be no spectral lines? I'm so lost on this one please help!
 
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Think of it as measuring the spectrum of Sun light reflected off a white surface, it will still produce a mostly continuous spectrum. When the light travels through the nebula cloud is when you get absorption lines.

Joe
 

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