The formation of stars is a natural process that occurs when a cloud of gas and dust collapses under its own gravity. As the cloud becomes denser and hotter, nuclear fusion reactions begin, resulting in the birth of a new star.
The formation of stars is an ongoing process in the universe, and there is a continuous supply of gas and dust in galaxies that can form new stars. However, the rate of star formation can vary depending on the availability of materials and other factors.
The type of star being formed at this rate would depend on the characteristics of the gas and dust clouds that are collapsing. Generally, these new stars would be young and relatively small, such as red dwarfs or brown dwarfs.
The distance of these newly formed stars would depend on the location of the gas and dust clouds in the galaxy. Some may be relatively close to us, while others may be much farther away in other parts of the universe.
The formation of stars is a crucial process in the universe, as they are responsible for creating and distributing heavy elements, which are essential for the formation of planets and life. The continuous formation of stars also contributes to the expansion and evolution of the universe.