Rapid-response characterization of near-Earth asteroid 2024 YR4 during a Torino Scale 3 alert
Maxime Devog\`ele, Olivier R. Hainaut, Marco Micheli, Petr Pravec, Juan Luis Cano, Francisco Oca\~na, Luca Conversi, Nicholas Moskovitz, Julia de Le\'on, Zuri Gray, Mikael Granvik, Grigori Fedorets, Jules Bourdelle de Micas, Simone Ieva, Elisabetta Dotto, Tracie Beuden

TL;DR
This paper reports a rapid observational campaign of asteroid 2024 YR4 during a high-impact risk alert, revealing its physical properties, rotation, and taxonomy to aid planetary defense efforts.
Contribution
It provides the first detailed physical characterization of asteroid 2024 YR4 during a Torino Scale 3 impact alert, emphasizing rapid international response importance.
Findings
Rotation period of approximately 19.46 minutes, classifying it as a fast rotator.
Spectral analysis suggests an Sq or K taxonomic type.
Shallow phase curve slope indicating surface properties.
Abstract
On 27 December 2024, near-Earth object (NEO) 2024 YR was discovered by the ATLAS survey and identified as a virtual impactor. A few weeks later, it eventually reached level 3 on the Torino Scale and was the first and only asteroid to be ever classified at that level. Here we report an intensive observational campaign combining time-series photometry in the visible, broadband visible and near-infrared colors, and low-resolution visible reflectance spectroscopy to assess its physical properties. Fourier analysis of the lightcurves yields a synodic rotation period of min, placing 2024 YR among the fast rotators, even if such rotation is common for objects of similar magnitude. Its visible and near-infrared colors and spectra are most consistent with an Sq or K taxonomic classification, though some ambiguity remains. Finally, its phase curve exhibits a…
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