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An astronomical observation team at the Qattamia Observatory, affiliated with the National Institute for Astronomical Research, successfully observed and captured images of the periodic comet 220P/McNaught on August 12, 2026. The comet showed a noticeable increase in brightness and activity, aimed at studying the development of its coma and tail. The comet is classified as a short-period comet, with an orbital period of approximately 5.5 years. It made a close approach to the Sun on June 14, 2026, at a distance of 1.56 astronomical units, during which sudden outbursts of activity were observed throughout 2026. This observation is part of efforts to study the astronomical processes associated with comets and to understand the evolution of primitive bodies that contribute to the formation of the solar system. The observations were conducted using a 1.88-meter telescope, providing vital data on changes in the comet's coma, tail structure, and activity variations.
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