Solving Redshift Confusion Homework Problem

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SUMMARY

The discussion centers on understanding the distinction between Hubble's law redshift and peculiar velocities in the context of galaxy movements. The Hubble constant is specified as 2.18 x 10-18 s-1, leading to a calculated distance of 1.36 x 1020 km where Hubble's redshift dominates. Participants emphasize the importance of using astronomical units such as parsecs or Megaparsecs instead of kilometers for clarity. Additionally, the conversion from velocity to redshift (z) is highlighted as a necessary step in the problem-solving process.

PREREQUISITES
  • Understanding of Hubble's Law and its equation V = h0 * D
  • Knowledge of redshift calculations using the formula V/c = Δλ/λ
  • Familiarity with the concept of peculiar velocities in astrophysics
  • Ability to convert units between kilometers, parsecs, and Megaparsecs
NEXT STEPS
  • Research the implications of Hubble's Law on cosmic expansion
  • Learn about the calculation of redshift (z) from velocity measurements
  • Explore the significance of peculiar velocities in galaxy dynamics
  • Study unit conversions in astronomy, focusing on parsecs and Megaparsecs
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in the dynamics of galaxies and the expansion of the universe will benefit from this discussion.

MoAli
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Homework Statement


I encountred a question that says : Assume that gravitational interactions between galaxies in groups lead to random galaxy velocities of 300 km/s At what distance would the redshift predicted by Hubble's law dominate over that produced by individual velocities? and what is the redshift at that distance?
I don't understand what's the difference between the 2 redshifts mentioned here, so I am confused on how to approach this

Homework Equations


V= h_0 * D
where D is the distance and the Hubble constant is 2.18*10^-18 s^-1

V /c = Δλ/λ

The Attempt at a Solution


I tried substituting in the numbers and got D= 1.36*10^20 km and v/c=0.001. [/B]
 
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I think you did it right. There is a smoothly increasing velocity moving away from us faster and faster as the distance increases (the "Hubble flow"), and superimposed on this is a random set of what are called "peculiar velocities". You are asked to determine how far away you need to look before the smooth Hubble velocities begin to dominate. A couple of comments: (1) I would put the distance in units more used by astronomers, like parsecs or Megaparsecs in stead of km, and (2) you gave a velocity, but you were asked for the redshift z.
 

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