Written by: Chami Amarasinghe
Edited by: Kate Giffin and Austin Shannon
For a hundred years now, evidence for invisible matter has been piling up (1). Eighty-five percent of the mass in our cosmic neighborhood is transparent (2). We are completely awash in this invisible substance, dark matter. It far outweighs the stars, planets, asteroids, gas, dust, and us (3). The evidence lies plainly in the night sky. Stars and galaxies are accelerated by the gravity of dark matter (4, 5). Light emitted from distant objects bends in its presence (6). But, despite its ubiquity, nearly nothing is known about the fundamental particles that make up dark matter (7). How heavy are they? Why are they so prevalent? If they are everywhere and interact with the atoms of our world, could we detect them as Earth travels through space? Dark matter particles have long been searched for in experiments but none have been found (8). The devices built to detect them are the most sensitive ears we have opened to the skies, and they continue to grow in size and complexity as scientists continue their search (9). Discovering the nature of dark matter would upturn our understanding of the universe, but history warns of dead ends. It is not predetermined that dark matter particles will be discovered (10).
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