Spectroscopy and the doppler effect

Click For Summary
SUMMARY

The discussion centers on the concept of redshift in spectroscopy, specifically how to determine if an object is redshifted by comparing its spectrum to a laboratory standard. Participants clarify that the comparison involves analyzing emission lines from both the distant object and a local hydrogen spectrum, allowing for the calculation of the Doppler shift and relative velocity. The key takeaway is that two different spectra are used: one from the object and one from a lab standard, rather than two spectra of the same moving object.

PREREQUISITES
  • Understanding of spectroscopy principles
  • Familiarity with redshift and Doppler effect concepts
  • Knowledge of emission lines and their significance in spectral analysis
  • Basic grasp of hydrogen spectral lines and their laboratory measurements
NEXT STEPS
  • Research the process of measuring redshift in astronomical objects
  • Learn about the Doppler effect in relation to light and sound
  • Explore spectral analysis techniques used in astrophysics
  • Study the characteristics of hydrogen emission lines and their applications
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in understanding the principles of spectroscopy and the Doppler effect in celestial observations.

The Subject
Messages
32
Reaction score
0
So the prof shows us how to tell if an object is red shifted, by comparing two spectra (i assume of the same object). The emission lines had similar gaps but were shifted right, therefore moving away from us.

How can you obtain two different spectra of the same object if it's constantly moving away from us? Wouldn't it only produce one red shifted spectra?

My understanding isn't clear.
 
Astronomy news on Phys.org
Hi Subject:

The red-shift is based on comparing the spectrum of a distant object with a spectrum that could be measured in a local laboratory. The line(s) that one compares are those that are present in both spectra. It is not necessary to compare all lines. For example., a spectrum from a distant star will likely include lines from hydrogen atoms. The pattern (ratios of wavelengths) of lines are recognizable as being from hydrogen. Their wavelengths can then be compared with those corresponding to lines from local hydrogen.

Hope this helps.

Regards,
Buzz
 
  • Like
Likes   Reactions: The Subject and |Glitch|
Here is an example of what Buzz Bloom was talking about:

33xy3ur.jpg
 
  • Like
Likes   Reactions: The Subject
They wouldn't be different spectra of the same object. One would be of the object and the other would be of a lab standard. You would then look at the lines of, say hydrogen, in both the object's spectra and the lab standard to measure the redshift. You can then calculate the Doppler shift and relative velocity.
 
  • Like
Likes   Reactions: The Subject
That explains a lot actually! Thanks
 

Similar threads

  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 13 ·
Replies
13
Views
3K
Replies
8
Views
5K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 7 ·
Replies
7
Views
4K
  • · Replies 14 ·
Replies
14
Views
4K
Replies
2
Views
3K