Solving Redshift Confusion Homework Problem

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The discussion centers on understanding the distinction between redshift caused by Hubble's law and redshift from individual galaxy velocities. The problem requires determining the distance at which the Hubble flow redshift becomes more significant than random peculiar velocities, which are noted to be around 300 km/s. The Hubble constant is provided, and calculations suggest a distance of approximately 1.36 x 10^20 km. Participants emphasize the importance of expressing distance in astronomical units like parsecs or Megaparsecs and highlight the need to convert velocity into redshift (z) for the final answer. Clarifying these concepts will aid in solving the homework problem effectively.
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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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