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Our galaxy is made up of 90% dark matter (matter that cannot be seen) and 10% bright matter (matter that can be seen with the naked eye). Simulations of the Milky Way's spinning have shown an invisible halo.

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In exploring the composition and dynamics of our galaxy, scientists have found fascinating insights into the dark and bright components that shape the Milky Way. About 90% of the galaxy is made up of dark matter, a mysterious substance that does not emit, absorb, or reflect light, and thus cannot be seen with the naked eye. The remaining 10% consists of bright matter, which includes stars, planets, gases, and other celestial objects that are detectable through various means of astronomical observation.

Dark matter, despite being invisible, plays a crucial role in the galaxy. Its presence is inferred from gravitational effects on visible matter and the structure of the universe. Without dark matter, the stars in the galaxy would move in very different patterns. The evidence for dark matter comes from observations such as those involving the rotational speeds of galaxies. In a galaxy like the Milky Way, stars at the outer edge rotate at the same speed as those near the center, which defies the laws of physics as we understand them based purely on the visible mass present.

Advanced simulations and models have shown that the Milky Way is enveloped in an enormous, invisible halo of dark matter. This halo extends much farther into space than the visible part of the galaxy, and it has a profound influence on the galaxy's structure and evolution. The gravitational pull of this dark matter halo helps to hold the galaxy together and prevents the stars from flying apart as they rotate at high speeds.

Understanding the exact nature of dark matter remains one of the foremost challenges in modern astrophysics. Various experiments aim to detect dark matter particles directly, but so far, none have succeeded. Theories about what dark matter might be range from weakly interacting massive particles (WIMPs) to more exotic possibilities like primordial black holes or new forms of matter altogether unseen.

The ongoing study of dark matter is not just academic. It has profound implications for understanding the entire universe, from the smallest scales to the largest cosmic structures. By continuing to study how galaxies like the Milky Way spin and hold together, astronomers piece together the puzzle of the cosmos, where dark matter plays an indispensable role. This mysterious component, though invisible, molds the visible universe in profound and enduring ways, challenging our perceptions and pushing the boundaries of known physics.