High School Trying to understand the differences between distant & local galaxies

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Cerenkov
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Hello.

The recent discovery of the galaxy SPT0418-47 has piqued my interest.

https://www.almaobservatory.org/en/images/reconstructed-view-of-spt0418-47/

https://en.wikipedia.org/wiki/SPT0418-47

https://www.eso.org/public/archives/releases/sciencepapers/eso2013/eso2013a.pdf

It's my current understanding that galaxies at this red shift are expected to display very different characteristics (star formation rates, rotation, metallicity, size, etc.) to the mature and highly-evolved galaxies in the local universe. But, it appears that certain characteristics of SPT0418-47 seem to buck this expectation.

It occurs to me that I need to discover more about how galaxies are characterised. Then, knowing this I could look at the characteristics of local galaxies and compare them to those distant ones with a better understanding.

So, this prompts me to ask the following questions.

1.
Is finding out about how galaxies are characterised a good first step in understanding the differences between distant, early galaxies and nearby, evolved ones in the local universe?

2.
If so, could I please be directed to some Basic Level resources (links, websites, blogs, etc.) that will help me achieve this?

3.
If not, could I please be guided to a better option?

4.
In the context of this topic, does the word 'Local' refer to the Local Group of galaxies, to the Virgo or Laniakea Superclusters or to a measurement relating to the redshift (z) ?

Any help given would be very much appreciated.

With thanks,

Cerenkov.
 
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1611345367898.png
Hope it helps but I am not very inteliggent on this matter
 
AndrewWayneHarville said:
View attachment 276676 Hope it helps but I am not very inteliggent on this matter
That has nothing to do with local and distant galaxies. It's referring to our Milky Way galaxy :smile:
 
Many thanks for the help folks. :smile:

I thought this thread had died stillborn.

Looks like I was wrong.

Thanks again.

Cerenkov.
 
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Cerenkov said:
Hello.

The recent discovery of the galaxy SPT0418-47 has piqued my interest.

https://www.almaobservatory.org/en/images/reconstructed-view-of-spt0418-47/

https://en.wikipedia.org/wiki/SPT0418-47

https://www.eso.org/public/archives/releases/sciencepapers/eso2013/eso2013a.pdf

It's my current understanding that galaxies at this red shift are expected to display very different characteristics (star formation rates, rotation, metallicity, size, etc.) to the mature and highly-evolved galaxies in the local universe. But, it appears that certain characteristics of SPT0418-47 seem to buck this expectation.

It occurs to me that I need to discover more about how galaxies are characterised. Then, knowing this I could look at the characteristics of local galaxies and compare them to those distant ones with a better understanding.

So, this prompts me to ask the following questions.

1.
Is finding out about how galaxies are characterised a good first step in understanding the differences between distant, early galaxies and nearby, evolved ones in the local universe?

2.
If so, could I please be directed to some Basic Level resources (links, websites, blogs, etc.) that will help me achieve this?

3.
If not, could I please be guided to a better option?
1) is correct, but the link offered for 2) is not a very good one, yet I don´ t know a better one.

The classification of nearby galaxies is basically into "elliptical" and "spiral" galaxies, with intermediate group of "lenticular"... plus "irregular" galaxies.
Irregular galaxies are common even in local universe - just look up for the Magellanic Clouds. Yet the link only briefly mentions irregular galaxies, and discusses elliptical and spiral galaxies at length.

The problem with SPT0418-47 refers to a guess that young world should have had only irregular galaxies, and no elliptic or spiral galaxies.
Cerenkov said:
4.
In the context of this topic, does the word 'Local' refer to the Local Group of galaxies, to the Virgo or Laniakea Superclusters or to a measurement relating to the redshift (z) ?
To redshift.
 

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