Movement of Galaxies in relation to each other

In summary, the universe started with a "Big Bang" about 14 thousand million years ago and has been expanding ever since. There is no centre to the expansion; it is the same everywhere. Edwin Hubble's discovery that the farther galaxies are from us, the faster they are receding suggests that we are at the centre of the universe, but in fact if the universe is expanding uniformly according to Hubble's law, it will appear to do so from any vantage point. The universe also has a local gravitational effect on neighboring galaxies. As we know all matter in a galaxy is moving in rotation, the movement of galaxies or even clusters of galaxies to each other is due to the expanding universe. There is also rotational movement between neighboring galaxies.
  • #1
GiZeHy
15
0
hi folks, maybe somebody can help me with this:

According to the standard theories of cosmology, the universe started with a "Big Bang" about 14 thousand million years ago and has been expanding ever since. Yet there is no centre to the expansion; it is the same everywhere. The Big Bang should not be visualised as an ordinary explosion. The universe is not expanding out from a centre into space; rather, the whole universe is expanding and it is doing so equally at all places, as far as we can tell.

In 1929 Edwin Hubble announced that he had measured the speed of galaxies at different distances from us, and had discovered that the farther they were, the faster they were receding. This might suggest that we are at the centre of the expanding universe, but in fact if the universe is expanding uniformly according to Hubble's law, then it will appear to do so from any vantage point.

As we know all matter in a galaxy is moving in rotation. But how is the movement of galaxies or even clusters of galaxies to each other? Is there any rotational movement between neighboring galaxies in addition to the expanding?
 
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  • #2
Please, somebody can answer this question!

As we know all matter in a galaxy is moving in rotation. But how is the movement of galaxies or even clusters of galaxies to each other? Is there any rotational movement between neighboring galaxies in addition to the expanding?
 
  • #3
Although overall the galaxies are all moving away from each other - as Hubble's law says.
They do have a local gravitational effect on each other, and nearby galaxies are sometimes moving toward each other.

The milky way and a few other local galaxies are all moving in a particular direction - known as the great attractor.
 
  • #4
Zolaxy said:
Please, somebody can answer this question!

As we know all matter in a galaxy is moving in rotation. But how is the movement of galaxies or even clusters of galaxies to each other? Is there any rotational movement between neighboring galaxies in addition to the expanding?



Our own Milky Way Galaxy has many satellite galaxies which orbit it.
The closest is the Sagittarius Dwarf Galaxy. Prior to its discovery the most familiar ones were the Large and Small; Magellanic Clouds. Here is a list of Milky Way Satellite Galaxies. The ones with question marks are suspected of being satellites but not as yet fully confirmed.

Excerpt:


I Canis Major Dwarf .
II Sagittarius Dwarf .
III LMC .
IV SMC .
V Ursa Major II Dwarf .
VI Ursa Minor Dwarf .
VII Draco Dwarf .
VIII Sculptor Dwarf Galaxy .
IX Sextans Dwarf.
X Carina Dwarf .
XI Ursa Major I Dwarf .
XII Fornax Dwarf .
XIII Leo II .
XIV Leo I .
? Leo IV.
? Boötes .
? Boötes II.
? Boötes III .
? Coma Berenices .
? Segue 2 0.07 35 dG D 2007
? Canes Venatici .
? Canes Venatici II .
? Hercules .
? Pisces II .
.

http://en.wikipedia.org/wiki/List_of_Milky_Way's_satellite_galaxies
 
  • #5
But how is the movement of galaxies or even clusters of galaxies to each other?

There IS movement but I've never read a summary/synopsis of such movement...likely it's rather random.

Is there any rotational movement between neighboring galaxies in addition to the expanding?

Yes, in general. Our own Milky Way galaxy and the nearby Andromedia galaxy are moving toward a general rotatioonal "collision"...but few stars or planets will actually collide as all galaxies are 99% space...gravitational attraction will shift the orbits of most mass in both galaxies...
I've seen computer simulations of galactic collisions but don't have any references...

Here is one type of movement: http://en.wikipedia.org/wiki/Virgo-centric_flow

and some discussion of collisions here:

http://en.wikipedia.org/wiki/Galactic_collision
 

FAQ: Movement of Galaxies in relation to each other

How do galaxies move in relation to each other?

Galaxies move in a variety of ways, depending on their location and the forces acting upon them. On a large scale, galaxies are moving away from each other due to the expansion of the universe. However, within galaxy clusters, gravity can cause galaxies to orbit around a central point. Additionally, galaxies can collide and merge, altering their movement patterns.

What causes the movement of galaxies?

The movement of galaxies is primarily driven by the force of gravity. The mass of the galaxies and the distance between them determine the strength of the gravitational pull. In some cases, other forces such as dark matter may also play a role in the movement of galaxies.

How do scientists study the movement of galaxies?

Scientists use a variety of tools and techniques to study the movement of galaxies. These include telescopes, which can observe the positions and velocities of galaxies over time, as well as computer simulations that can model the movement of galaxies based on known physical laws.

What can the movement of galaxies tell us about the universe?

The movement of galaxies can provide valuable insights into the structure and evolution of the universe. By studying the patterns of movement, scientists can better understand the distribution of matter and the effects of gravity on large scales. This can also offer clues about the history and future of the universe.

Can galaxies move closer together?

Yes, galaxies can move closer together through a process called gravitational attraction. If two galaxies are close enough and have a favorable trajectory, they can merge to form a larger, more massive galaxy. This is a slow process that can take millions of years to occur.

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