Yes,
The Big Bang theory says all galaxies are moving outward and the universe is also expanding due to the explosion.
The radiation left over from the big bang, known as the cosmic microwave background radiation, has not dissipated to the far ends of the universe because it is constantly expanding and cooling as the universe expands. This radiation is spread uniformly throughout space, and although it has cooled significantly since the big bang, it can still be detected in all directions.
Stars spread out in the universe due to the expansion of space over time. As the universe expands, the distance between stars increases, leading to their distribution across vast distances. This expansion also causes galaxies to move away from each other.
Cosmic Microwave Background Radiation is electromagnetic radiation left over from the events of the Big Bang. This radiation causes a very slight increase in the universe's temperature; the coldest areas of the universe will be only about 2 degrees kelvin (2 degrees above absolute zero). It is not spread in a perfectly uniform pattern, though the differences in density are very slight.
There are billions of stars in the universe, far more than just 27. Stars are spread across galaxies, and each galaxy can contain billions or even trillions of stars. The universe is vast and expansive, with countless stars yet to be discovered.
It means they are distributed equally after some time. This is the phenomena of diffusion.
There is no singular star in the center of the universe. Our universe is vast and does not have a center. Stars are spread throughout the universe in galaxies, and our sun is just one of the billions of stars in the Milky Way galaxy.
Although we can't calculate the exact no galaxies in the universe , because of the vast distance the universe is spread over, The most accepted assumptions holds that there are approximately 100 Billion galaxies in the universe.
Edwin Hubble proved that there are other galaxies spread throughout the universe, and that these galaxies move away from each other as the universe expands. He further found that the galaxies in the outermost areas of the universe move faster that those nearer the middle, a feature in his Hubble's Law.
our Universe is telling us that you are bad at Astronomy.
suspension
A mixture with two or more substances spread evenly throughout is called a homogeneous mixture. This means that the different substances are uniformly distributed at a molecular level, resulting in a consistent composition throughout the mixture.
The universe emits the most cosmic microwave background radiation, which is thermal radiation left over from the Big Bang. This radiation is spread uniformly in all directions throughout space and has a temperature of about 2.7 Kelvin.
The radiation left over from the big bang, known as the cosmic microwave background radiation, has not dissipated to the far ends of the universe because it is constantly expanding and cooling as the universe expands. This radiation is spread uniformly throughout space, and although it has cooled significantly since the big bang, it can still be detected in all directions.
The big bang theory states that the galaxies in the universe are continuously moving away from each other due to the expansion of space. This expansion suggests that the universe began from a hot, dense state approximately 13.8 billion years ago.
Stars spread out in the universe due to the expansion of space over time. As the universe expands, the distance between stars increases, leading to their distribution across vast distances. This expansion also causes galaxies to move away from each other.
Cosmic Microwave Background Radiation is electromagnetic radiation left over from the events of the Big Bang. This radiation causes a very slight increase in the universe's temperature; the coldest areas of the universe will be only about 2 degrees kelvin (2 degrees above absolute zero). It is not spread in a perfectly uniform pattern, though the differences in density are very slight.
A homogeneous mixture has substances that are uniformly spread out. This means that the components of the mixture are evenly distributed at a molecular level, resulting in a uniform appearance throughout the mixture. Examples include solutions like saltwater and air.