Nearby galaxies won't show much of a redshift, because they aren't moving away very quickly - or at all. For example, the Andromeda Galaxy, M31, is actually getting closer - and will collide with the Milky Way in about 3 billion years.
Distance at cosmological scales is typically measured using the redshift of light from distant galaxies. This redshift is caused by the expansion of the universe, with more distant galaxies exhibiting higher redshifts. By measuring the redshift of galaxies, astronomers can calculate the distance based on the way that light is stretched as the universe expands.
Probably, but impossible to tell as we are only just seeing planets within our own galaxy.
Spiral galaxies have a clearly defined disk component characterized by spiral arms, while lenticular galaxies have a disk without prominent spiral arms. Irregular galaxies may also have a disk component, but it is usually less organized than in spiral galaxies.
As light from other galaxies travels through space to reach Earth, it can be affected by various factors, including the expansion of the universe, which causes redshift, making the light appear more stretched and shifting it toward the red end of the spectrum. Additionally, the light may interact with interstellar dust and gas, which can scatter or absorb some wavelengths, altering the observed colors. Gravitational lensing can also occur, where massive objects bend the light, magnifying or distorting the image of the distant galaxy. Ultimately, the light we observe provides valuable information about the universe's structure and the galaxies' properties.
Very lens-shaped elliptical galaxies have a high amount of reddish stars. Hence both their shape (the "spiral arms" have pulled inward over time) and the color of the stars implies they are very old galaxies. Spherical galaxies - I'm not up enough on that topic, so I will leave that part of the answer to another.
Distance at cosmological scales is typically measured using the redshift of light from distant galaxies. This redshift is caused by the expansion of the universe, with more distant galaxies exhibiting higher redshifts. By measuring the redshift of galaxies, astronomers can calculate the distance based on the way that light is stretched as the universe expands.
Most galaxies generally move away from each other due to the expansion of the universe, a phenomenon observed through the redshift of light from distant galaxies. This movement is described by Hubble's Law, which states that the recessional velocity of a galaxy is proportional to its distance from us. However, within galaxy clusters, gravitational interactions can cause galaxies to move closer together, and some may even collide or merge. Overall, the large-scale motion of galaxies is predominantly influenced by the expansion of space itself.
one kind is lenticular galaxies
That has nothing to do with the "type"; it is how far they are away from Earth. Due to the general expansion of the Universe, galaxies that are far way from us systematically move away from us - the farther away, the faster. It is only nearby galaxies which may happen to move towards us.
The Big Bang is a type of beginning of the Universe. It wasn't exactly an explosion in the traditional sense, and it may or may not have been the actual beginning.We know about the Big Bang, among other things, because of the redshift of distant galaxies (the only reasonable explanation is that galaxies are moving away from us); because the element distribution in the Universe closely matches what is expected from a Big Bang; and because the cosmic microwave background radiation, likewise, closely matches the expectations.
They (scientists) think there are hundreds of thousands of galaxies because the universe is limitless so there may be billions of galaxies!
Galaxies may have any of four general shapes. Elliptical galaxies show little or no structure and vary in general shape from moderately flat and round or oval to spherical. Spiral galaxies have a small, bright central region, or nucleus, and arms that come out of the nucleus and wind around, trailing off like a giant pinwheel. In barred spiral galaxies, the arms extend sideways in a short straight line before turning off into the spiral shape. Both kinds of spiral systems are flat. Irregular galaxies are usually rather small and do not have a symmetrical shape.
Probably, but impossible to tell as we are only just seeing planets within our own galaxy.
About the only thing that can surround galaxies is other galaxies. Since many galaxies appear to lie in approximate lines, one thing that influences galaxy formation may be "superstrings," but these have yet to be directly detected.
Here is what i belive to be the correct awnser. If you belive in the big bang theory then you swould know the universe started from the middle and started expanding out so the closest galaxie is moving away with us but distant galaxies are also moving away from us now i dont know about how they move or what speed they move at or if theres a differnce it is possible considering some galaxies formed billions of years after our a slowley catching up with as so i belive it varies now i hope this answer your question people may edit this in future and make it easyer to understand.
Spiral galaxies have a clearly defined disk component characterized by spiral arms, while lenticular galaxies have a disk without prominent spiral arms. Irregular galaxies may also have a disk component, but it is usually less organized than in spiral galaxies.
As light from other galaxies travels through space to reach Earth, it can be affected by various factors, including the expansion of the universe, which causes redshift, making the light appear more stretched and shifting it toward the red end of the spectrum. Additionally, the light may interact with interstellar dust and gas, which can scatter or absorb some wavelengths, altering the observed colors. Gravitational lensing can also occur, where massive objects bend the light, magnifying or distorting the image of the distant galaxy. Ultimately, the light we observe provides valuable information about the universe's structure and the galaxies' properties.