How our galaxy is formed

How our galaxy is formed

A 2016 study estimated that the universe contains between 2 billion and 2 billion galaxies. Some of these galaxies are similar to ours in the Milky Way, while others are quite different.

When the galaxy is being constructed, it is usually disk-shaped and is called a spiral galaxy because of its spiral arm. The spiral galaxy is a flat, rotating disk with a central cylinder surrounded by winding arms.

Olin Eggen and Donald Lynden Bell Allan (1962) expressed the view that disk galaxies arose from the monolithic collapse of a large gas cloud. Astronomers thought that the force of gravity pulled dust and gas together into a single star, and these stars were then pulled together to form galaxies. It was suggested by Leonard Searle and Robert Zinn [3] that galaxies come from a combination of young ancestors.

Some believe that the size of the galaxy is determined by the number of stars in the universe. Since the 1920s, astronomers have been able to understand the basics of galaxies, or at least galaxies, of massive galaxies and gases and dust similar to those of the Milky Way.

Also, galaxies are formed when large clouds of gas and dust collapse under their gravitational pull, forming stars. One of the gains in recent years is that the small universe has many smaller galaxies that combine to form galaxies. Comments by the Hubble Space Telescope and ground-based instruments show that the first galaxies were not built until a billion years after the Big Bang, which occurred 13 to 14 billion years ago.

The Hubble Space Telescope filmed many such fibers, which preceded modern galaxies. As the atmosphere expands, things go awry, and because of the instability of the gravitational pull, the clouds of lightning fall and form large stars.

Although they make up only a small fraction of the number of visible galaxies, astronomers believe that all the galaxies in the universe are round. Stellar, lens, or circular galaxies are called unconventional galaxies. Extraordinary galaxies, such as the massive and small stems of the Magellan clouds on the sides of our Milky Way, appear to be invisible because of their gravitational pull from other galaxies and have no distinct shapes.

The remaining 3 percent of galaxies in the universe are known as unconventional galaxies. Unusual galaxies may be circular or have arms that rotate, but their shape is not accurately described. The size of some galaxies can be affected, expanded, and distorted.

The above situation seems to define the number of stars in the SA and SB structures, but the bulges of SA and SD galaxies are the same as on the disks of these galaxies. This suggests that bulges are a slow-moving type of galaxy made by the earth's evolutionary process.

The Milky Way halo and other galaxies of SA and SB contain very old stars. The star disks of the burning galaxies are very small, and most of the stars are in trouble.

This suggests that the bulge and halo of spiral galaxies were formed early in the history of the universe by a massive collapse of individual gas clouds.

There is much debate about the precise mechanism of gas accumulation and the accumulation of galaxies, and how this process relates to the structure and strength of galaxies over time. An important part of the debate is whether galaxies like ours, where stars form in the Milky Way, have a natural disk-controlled body structure (Fig. procedures.

The galaxy is a huge galaxy of billions of stars and other objects connected to each other. Many of the stars that make up the galaxy contain dust and air, and this disk appears as dark spots, threads, or silhouettes in starlight. There are a variety of galaxies, including the burning galaxies like ours, the Milky Way, which are rich in dust and star gases in their arms, gaseous galaxies, lens galaxies, and unusual galaxies such as the Magellanic Cloud and the short Sagittarius A *.

The study of the design and evolution of galaxies affects the process of constructing a complex space instead of an equal starting point with the construction of the first galaxies and how the galaxies change over time, a process that produces variations observed in nearby galaxies. Details about astronomers provide important clues as to how our galaxy was built in the future.

To catch on to the formation of small wind farms, see the design of the galaxy simulator. Galaxies are thought to have formed little, and the theory of architecture is the result of the small quantum flexibility behind the Big Bang. The glowing mimic shows what the galaxy looks like in the Milky Way as it transforms from a gas cloud at the beginning of the universe into a beautiful barrier that lasts for a few billion years before spinning in a few minutes.

Thousands of years ago, there was a violent collision between two separate stars that met the tiny galaxy we call Gaia Enceladus. As a result, the tiny galaxy of one-star began to move, forming an existing halo in the Milky Way.

The cluster was formed by a clash between large clusters of galaxies during one of the most powerful events in the universe, the Big Bang. Because the main components of the cluster - the two stars, the gas - and the seemingly dark matter - behaved in a very different way after the collision, scientists have been able to study them extensively.