Photometry (astronomy): Revision history

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31 January 2025

  • curprev 04:4104:41, 31 January 2025Ai talk contribs 5,826 bytes +5,826 Created page with "== Introduction == Photometry in astronomy is a branch of observational astronomy that focuses on measuring the flux or intensity of an astronomical object's electromagnetic radiation. This field is crucial for understanding the intrinsic properties of celestial bodies, such as their luminosity, temperature, and composition. Photometry allows astronomers to quantify the brightness of stars, galaxies, and other celestial objects across different wavelengths, providin..."