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Strange Green Glow Discovered in Interstellar Comet 3I/ATLAS

by Rachel Kim – Technology Editor

Interstellar Comet 3I/ATLAS Displays Unusual green Glow, Challenging Existing Cometary science

NAMIBIA – Images captured by astrophotographers Gerald Rhemann and ⁣Michael Jäger in namibia ⁢reveal that interstellar comet 3I/ATLAS is now exhibiting a vibrant blue-green gas coma and a developing tail, sparking ​a scientific ⁣puzzle over its unusual composition. The‍ observations, made during the ‌total lunar eclipse on the night of September ⁤7, 2025, show a coma ⁤measuring 2.5 arcminutes across and ‍a ⁢visible tail as of September 9.

This⁤ isn’t the first indication that 3I/ATLAS is unlike any comet previously studied. Observations‍ from the James Webb‌ Space⁢ Telescope (JWST) have already​ revealed​ a peculiar ‍chemical makeup, with‍ larger-than-usual proportions ​of carbon dioxide. Further analysis has also detected the presence of ⁢nickel and cyanogen, but these elements don’t explain the observed green fluorescence.

Comets typically display their glow as ices ⁣sublimate into a gas atmosphere – or coma ⁤- when approaching the Sun,with molecules fluorescing when stimulated by solar​ radiation. However, the molecule responsible for the ⁤green ‍glow in most comets, diatomic‍ carbon (C2), has not been detected in 3I/ATLAS. This absence ‍is especially perplexing⁢ given the early detection of‌ cyanogen.

A recent preprint led by astronomer Luis Salazar Manzano of the university of Michigan,‍ Ann Arbor, suggests a strong depletion of ⁣carbon-chain molecules, including both C2 and C3. “Our​ upper limit⁣ on the C2-to-CN ratio,” the researchers‌ write, ⁤”places 3I/ATLAS among the ⁣most carbon-chain depleted comets known.”

The mystery surrounding⁢ 3I/ATLAS deepens as scientists await its closest approach to earth ⁤in December, hoping to gather more data and unravel the secrets of this interstellar visitor. The comet’s unique⁤ composition offers‌ a rare opportunity to ⁣study materials from beyond our solar system and‌ perhaps refine our understanding⁢ of cometary formation and evolution.

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