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Comet Lemmon Illuminates the Night Sky: A Celestial Spectacle for Skywatchers

By Agamveer Singh , 30 October 2025
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Comet C/2025 A6 (Lemmon) has emerged as one of the most captivating astronomical events of 2025, offering skywatchers a rare opportunity to witness a bright green comet with a striking tail. Discovered in January 2025 by the Mount Lemmon Survey in Arizona, this comet has brightened significantly, reaching a visual magnitude of approximately 4.93, making it visible to the naked eye under dark skies. Its closest approach to Earth occurred on October 21, 2025, at a distance of about 89 million kilometers. Currently, Comet Lemmon is best observed in the evening sky, moving through the constellations Boötes and Serpens.

The Journey of Comet Lemmon

Comet Lemmon is a long-period comet with an orbital period of approximately 1,300 years. After its discovery, astronomers observed a significant increase in its brightness, likely due to an outburst of activity on its icy nucleus. As the comet neared the Sun, the heat caused the ices on its surface to sublimate, releasing gas and dust that formed its coma and tail. This process is characteristic of comets as they approach the inner solar system.

Observing Comet Lemmon

For observers in the Northern Hemisphere, Comet Lemmon is visible in the western sky after sunset. In Ludhiana, India, the comet is best viewed approximately 30–40 minutes after sunset. Using binoculars or a small telescope can enhance visibility, allowing observers to see the comet's greenish coma and tail. The comet is currently moving through the constellations Boötes and Serpens, and its position changes nightly, so it's advisable to use a stargazing app or sky chart to locate it.

Significance of the Observation

Comet Lemmon's appearance provides a unique opportunity for both amateur and professional astronomers to study the composition and behavior of long-period comets. Observing such comets helps scientists understand the early solar system's conditions and the materials that contributed to the formation of planets. Additionally, the comet's bright appearance and distinctive green hue, caused by diatomic carbon in its coma, make it a fascinating subject for skywatchers and astrophotographers alike.

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