An analytic sky-motion formula applied to synthetic interstellar object populations indicates that high velocities, particularly for dim objects, may cause many to go undetected, implying a larger galactic population than currently observed.
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Rubin Observatory delivers the earliest large-telescope astrometry and grizy photometry of interstellar comet 3I/ATLAS, including colors and a dust-to-nucleus cross-section ratio lower limit.
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Sky-Plane Velocity Distributions of Interstellar Objects and Implications for Their Detection
An analytic sky-motion formula applied to synthetic interstellar object populations indicates that high velocities, particularly for dim objects, may cause many to go undetected, implying a larger galactic population than currently observed.
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NSF-DOE Vera C. Rubin Observatory Observations of Interstellar Comet 3I/ATLAS (C/2025 N1)
Rubin Observatory delivers the earliest large-telescope astrometry and grizy photometry of interstellar comet 3I/ATLAS, including colors and a dust-to-nucleus cross-section ratio lower limit.