do clarify your question
Generally, the galaxies that are further away will have the larger red shifts.
The ones that are farther from the sun have longer revolutions.
because of the way rock and debris hit them they spin faster
Their orbit is a smaller circle than the ones further out, and as long as they are moving at relatively the same speed they will complete each orbit faster. Check out the planetary orbits link, it gives a really cool description and moving diagram
planets that are closer to the sun usually will have higher density compared to ones further from the sun.
The red shift. A Doppler effect (used in speed trap radar) showing that all (except for a few close ones) galaxies are moving away from us - and the farther away they were the faster they were moving.
my guess is that larger telescopes are stronger than smaller ones. which means they can see farther. .
Irregular ones!
There are billions of other galaxies; perhaps 100 billion or so (1011) in the observable Universe. Some of the closer ones - that can be seen with the naked eye - are M31 (a.k.a. the "Andromeda Galaxy", the Large Magellanic Cloud, and the Small Magellanic Cloud.
I don't believe that is possible to figure out
The closest ones near our galaxy.
The close-in ones move fast, the far-out ones move slower. It's governed by Kepler's third law.
During gel electrophoresis, the smaller particles move faster than the larger ones. The end of the gel where the samples are loaded is called the sample origin. Samples move from the origin toward the opposite electrode according to size. At the end of the run, smaller particles will have migrated farther from the origin and the larger ones will be found closer to the origin
-- "Light Year" for the closer ones -- "Parsec" for the farther ones
Which ones are visible at what time of day does. The galaxies themselves don't.
They look like eclipse ones like s82o.
smaller ones turn faster than larger ones