In our galaxy, the Milky Way, it is estimated that there are approximately 100 billion to 400 billion stars. The exact number is challenging to determine precisely due to the vast size and complexity of the galaxy, as well as the limitations of our observation methods. These stars vary in size, age, and characteristics, including their own solar systems, which may have planets orbiting them.
Our Sun, also known as Sol, is just one of these many stars within the Milky Way. It is located in the outer part of the galaxy, about 27,000 light-years away from the galactic center. The Sun is an average-sized star, classified as a G-type main-sequence star, and it serves as the primary source of light and energy for our solar system.
So, while it is difficult to provide an exact count, the estimated range of stars in the Milky Way suggests that there are millions upon millions of stars similar to our Sun throughout the galaxy.