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| Scientific Frontline / Stock image |
The universe, in its vastness, is largely composed of matter that does not shine. For centuries, the discipline of astronomy was fundamentally limited to the study of luminous objects: stars that fuse hydrogen into helium, gas clouds excited by radiation, and galaxies that act as islands of light in the cosmic dark. This reliance on electromagnetic radiation—photons—as the primary messenger of cosmic information created a significant selection bias. It rendered the "dark sector" of the Milky Way, including brown dwarfs, black holes, old white dwarfs, and free-floating planetary-mass objects, effectively invisible to standard census techniques. To map the true mass distribution of our galaxy, astronomers required a method that did not rely on the emission of light but rather on the one force that pervades all matter: gravity.



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