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In astronomy, a "radiant" refers to the point in the sky from which meteors in a meteor shower appear to originate. This apparent convergence is similar to how parallel lines seem to meet at a distant point. Meteor showers are named after the constellation containing their radiant. The meteors themselves are small particles, or meteoroids, that burn up upon entering Earth's atmosphere, creating visible streaks of light. These meteoroids often originate from comets, shedding debris along their orbital paths around the Sun. When Earth intersects these streams of debris, we observe a meteor shower. While most showers are associated with comets, some may have other origins.1

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