Galaxies are vast systems of stars, gas, dust, and dark matter held together by gravity. There are estimated to be billions of galaxies in the universe, each containing anywhere from a few hundred billion to a few trillion stars. The shape and structure of galaxies can vary, with some being spiral-shaped like our Milky Way, while others are more elliptical or irregular in shape. Galaxies are believed to have formed through a combination of gravitational attraction and the cooling and condensing of gas and dust in the early universe. They continue to evolve over time through a variety of processes, such as mergers, collisions, and the formation of new stars. The study of galaxies and their properties is a major area of research in astrophysics and cosmology.
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