Machine learning clustering of meteor observations produces a new hardness classification H_class that refines traditional Kb models using more parameters and reveals compositional structure in meteoroid populations.
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A Haser model tracking the fading of icy grain albedo by sublimation explains the exponential surface brightness profiles and photometry of comet 3I/ATLAS, with total ice scattering cross-section peaking at 3-4 au.
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A Machine Learning Approach to Meteor Classification
Machine learning clustering of meteor observations produces a new hardness classification H_class that refines traditional Kb models using more parameters and reveals compositional structure in meteoroid populations.
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A Physical Model for the Ice Coma of the Interstellar, Hyperactive Comet 3I/ATLAS
A Haser model tracking the fading of icy grain albedo by sublimation explains the exponential surface brightness profiles and photometry of comet 3I/ATLAS, with total ice scattering cross-section peaking at 3-4 au.