Undergrad Factor of how much linear size scale has changed

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The discussion focuses on calculating the change in the linear size scale of the Universe based on redshift (z). The formula for linear size scale is given as 1 / (1 + z), where 'now' corresponds to z=0 and a scale factor of a=1. To find the factor of change, one must calculate the size scale at the time of emission using the initial redshift. The linear size scale itself represents the factor by which the universe's size has changed over time. The conversation clarifies that the question is straightforward, contrary to initial assumptions.
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Question: By what factor has the linear size-scale of the Universe changed between when the light was emitted from the galaxy and now?

The question gives the red shift z and I have the equation linear size scale = 1 / 1 + z and I know how to calculate the linear size scale. But I'm a little confused as to what the question is saying. It is asking about the factor of how much the linear size scale has changed right? So if I just give the linear size scale, the answer won't be fully correct. So I'm assuming to calculate the factor, I would need to find the initial red shift z and calculate the exponent which will give me the new linear size scale that I calculated previously? Thanks for your help.
 
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I don't quite understand what you are asking. By definition, 'now' means z=0 and the scale factor a = 1. So when you calculate the size scale a = 1/(1+z) at the time of emission that tells you the factor by which the size scale has changed from then to now. If you are 6 feet tall today and were 3 feet tall when you were 8 years old, you were 0.5X as tall then as you are now.
 
Ok I understand. The linear size scale itself is the factor by which the size of the universe changed. I thought the question is more complex than what it really is asking. Thanks.
 
UC Berkely, December 16, 2025 https://news.berkeley.edu/2025/12/16/whats-powering-these-mysterious-bright-blue-cosmic-flashes-astronomers-find-a-clue/ AT 2024wpp, a luminous fast blue optical transient, or LFBOT, is the bright blue spot at the upper right edge of its host galaxy, which is 1.1 billion light-years from Earth in (or near) a galaxy far, far away. Such objects are very bright (obiously) and very energetic. The article indicates that AT 2024wpp had a peak luminosity of 2-4 x...

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