How Does Hubble's Law Calculate Redshift for Distant Galaxies?

In summary: So if you could find an object that was receding from us at a rate greater than the speed of light, you could use the expansion of space to calculate its distance and speed.
  • #1
SN1987a
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0
How would one use hubble's law to find the redshift of a galaxy[itex] 10^10[/itex] light years away? (in other words [itex] 3*10^9 pc[/itex])

All I know however is the version of hubble's where [itex] v=H_o d[/itex], with [itex] H_o=71 \frac{m}{s*pc}[/itex], which tells me that [itex] v= 2.2*10^11 m/s[/itex]. But this violates the second principle of special relativity!

How do I get around this problem?
 
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  • #2
  • #3
Yeah, but km/sMpc is the same as m/spc, is it not? So that doesn't change my problem a whole lot.
 
  • #4
well if you plug in the numbers you will find that you should get a reasonable answer. And no they aren't the same. m/skpc would be the same as km/sMpc.
 
  • #5
SN1987a said:
How would one use hubble's law to find the redshift of a galaxy[itex] 10^10[/itex] light years away? (in other words [itex] 3*10^9 pc[/itex])

Well, big man is right about your value of Hubble's constant, but one really shouldn't use Hubble's law to find the distance or speed of an object at 3 Gpc. Hubble's Law is just a first order approximation approximation to whatever cosmological model describes the universe that we live in. This approximation is only valid if the object's recession speed is much less than the speed of light (for your purposes, this corresponds to redshifts <~ 0.1).

Even when you put in the correct value of Hubble's constant, you'll get v ~ 0.7c, so Hubble's Law will give a pretty inaccurate result. However, if this is a homework assignment and you've just learned basic cosmology, I suspect that your teacher wants you to use Hubble's Law anyway.

By the way, objects can recede from us at rates greater than the speed of light. This is because the object isn't moving through space, the space itself is expanding. The expansion of space is not restricted by the speed of light.
 

Related to How Does Hubble's Law Calculate Redshift for Distant Galaxies?

1. What is Hubble's law?

Hubble's law, also known as the Hubble-Lemaître law, is a fundamental relationship in cosmology that describes the expansion of the universe. It states that the further a galaxy is from us, the faster it is moving away from us.

2. How is Hubble's law related to redshift?

Redshift is a phenomenon that occurs when light from an object is stretched as it travels through expanding space. Hubble's law is related to redshift because the amount of redshift observed in the light from a distant galaxy is directly proportional to its distance from Earth, as described by the law.

3. What is the significance of Hubble's constant?

Hubble's constant, denoted by the symbol "H", is a numerical value that represents the rate at which the universe is expanding. It is a crucial parameter in many models of the universe and is used to estimate the age and size of the universe.

4. How does Hubble's law provide evidence for the Big Bang theory?

Hubble's law provides evidence for the Big Bang theory because it supports the idea that the universe is expanding from a single point in space, as predicted by the theory. The linear relationship between the distance and velocity of galaxies, as described by the law, is consistent with the idea of an expanding universe.

5. Can Hubble's law be used to measure the age of the universe?

Yes, Hubble's law can be used to estimate the age of the universe by using the inverse of the Hubble constant. This value, known as the Hubble time, is equal to the age of the universe if the expansion rate has been constant throughout its history. However, recent research suggests that the Hubble time may not accurately represent the true age of the universe due to the effects of dark energy on the expansion rate.

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