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Astronomical surveys

Astronomical surveys are systematic efforts to map and study celestial objects and phenomena across the universe. Astronomers use advanced telescopes and instruments to capture detailed images and data about stars, galaxies, planets, and other cosmic features. These surveys help scientists catalog celestial bodies, analyze their properties, and understand the universe's structure and evolution. By collecting vast amounts of information, astronomical surveys contribute to our knowledge of fundamental questions about the cosmos, such as the nature of dark matter, the expansion of the universe, and the formation of galaxies.

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    Astronomical surveys are systematic observations of the night sky aimed at cataloging celestial objects and phenomena. These surveys use telescopes equipped with cameras and detectors to capture images and data across different wavelengths, such as visible light, infrared, and radio. By surveying large areas of the sky, astronomers can identify stars, galaxies, asteroids, and other cosmic features. The information gathered helps scientists understand the universe's structure, origins, and evolution while also discovering new objects and gaining insights into cosmic events. Notable surveys include the Sloan Digital Sky Survey and the Hubble Space Telescope observations.