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New images of 3I/ATLAS just dropped, and they’re raising fresh questions. A newly released NEOSSat contour map shows a compact inner structure with persistent sunward features that don’t smear out the way we’d expect from a diffuse coma. The core remains tight, suggesting an organized source region rather than random dust release. Independent amateur observations now back this up. New Seestar S50 captures from multiple observers show the same faint elongation and brightness concentration across different exposure lengths. Despite different equipment, locations, and processing, the structure holds. Additional imaging and video from Italy, captured during the object’s recent close approach, shows 3I/ATLAS moving rapidly against background stars while maintaining a coherent central glow. The motion is fast. The morphology is stable. That combination is what makes this object worth watching closely. Nothing here relies on a single telescope, a single filter, or a single observer. The pattern is repeating — and that’s the part that matters. We’ll keep following the data as new observations come in. 📚 Sources: • NEOSSat observations and contour map: D. D. Balam (DAO/NRC), C. E. Spratt, D. W. E. Green (CBAT), P. Langill (RAO/University of Calgary), Omar Elmi, Jack Williams, Canadian Space Agency • Amateur Seestar S50 images by Con Stoitsis • Imaging and perigee video by Mario Feraco (MPC L85, Italy) • Orbital context and alignment analysis: Stefan Burns • Lunar impact flash detection: Armagh Observatory and Planetarium What do you think is driving this structure? Drop your thoughts below. If you want more clear, evidence-based updates on 3I/ATLAS and other space events, hit like and subscribe. #3IATLAS #interstellarobject #astronomy #spacenews #spaceunfiltered