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Passionate Eng
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How did we know that our galaxy is spiral?!
A spiral galaxy is a type of galaxy that is characterized by its distinct spiral shape, with a central bulge surrounded by spiral arms. Our own galaxy, the Milky Way, is a spiral galaxy.
The Milky Way is estimated to be about 100,000 light years in diameter, with approximately 200-400 billion stars. It is also surrounded by a halo of dark matter, which extends further out than the visible stars.
Many spiral galaxies, including the Milky Way, have a supermassive black hole at their center. These black holes play a crucial role in the formation and evolution of the galaxy, as they can influence the movement of stars and gas within the galaxy.
Stars form in regions of high gas density within a spiral galaxy, such as in the spiral arms. As gas and dust particles clump together due to gravity, they eventually become dense enough to trigger nuclear fusion and form a star.
It is estimated that the Milky Way will continue to evolve and grow for billions of years. The spiral arms will continue to rotate and stars will continue to form. However, it is also possible that the Milky Way may collide with another galaxy in the future, potentially altering its shape and structure.