Astromony Q: Red Shift of 500nm Wavelength Line in Hydra Galaxy

  • Thread starter Thread starter asdf1
  • Start date Start date
Click For Summary

Homework Help Overview

The discussion revolves around a question in astronomy regarding the redshift of a spectral line emitted by a distant galaxy in the constellation Hydra, which is receding from Earth at a significant velocity. The specific focus is on determining the shift of a green spectral line with a wavelength of 500nm.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the application of the relativistic Doppler effect to calculate the redshift. There is a mention of the relevant formula and the definition of variables involved, such as the velocity of the galaxy and the source wavelength.

Discussion Status

The conversation is ongoing, with some participants providing insights into the reasoning behind using the Doppler effect. There is an acknowledgment of a spelling correction, indicating a collaborative atmosphere, but no consensus or resolution has been reached yet.

Contextual Notes

Participants are navigating the complexities of the relativistic Doppler effect and its application to the problem, with some assumptions about the definitions and parameters involved in the calculations being discussed.

asdf1
Messages
734
Reaction score
0
There's an astromony question that I'm stuck on~
" A distant galaxy in the constellation Hydra is receding from the Earth at 6.12*10^7 m/s. By how much is a green spectral line of wavelength 500nm (1nm=10^(-9) )emitted by this galaxy shifted toward the red end of the spectrum?
 
Physics news on Phys.org
what knowledge do you have?
 
asdf1 said:
There's an astromony question that I'm stuck on~
" A distant galaxy in the constellation Hydra is receding from the Earth at 6.12*10^7 m/s. By how much is a green spectral line of wavelength 500nm (1nm=10^(-9) )emitted by this galaxy shifted toward the red end of the spectrum?

Just use the relativistic doppler effect:

[tex]\nu_{obs}/\nu_{source} = \sqrt{\frac{1+\beta}{1-\beta}}[/tex]

where [itex]\beta = v/c = .204[/itex] and [itex]\nu_{source} = c/\lambda_{source}[/itex]

AM
 
How did you think of to use the Doppler effect?
 
Probably because the question is about the Doppler effect (well, it's about red shift, which is to do with the Doppler effect). Also, you mean "astronomy", not "astromony".
 
I see~
Thanks for correcting my spelling mistake!
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
2K
Replies
1
Views
3K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 7 ·
Replies
7
Views
4K
Replies
10
Views
4K
  • · Replies 6 ·
Replies
6
Views
7K
  • · Replies 2 ·
Replies
2
Views
3K