Polarimetry and albedo of the Near-Earth Asteroid 2025 FA22
J.-P. Rivet, S. Bagnulo, P. Bendjoya, G. Borisov, A. Cellino, M. Devog\`ele, Z. Gray, S. Ieva, L. Kolokolova, Y. G. Kwon, A. Berdyugin, S. V. Berdyugina, L. Boulanger, E. Dotto, P. Fatka, E. Frank, M. Lazzarin, V. Piirola, P. Pravec, and the NEOPOPs team

TL;DR
This study presents spectropolarimetric observations of asteroid 2025 FA22 during its close approach, providing insights into its albedo, composition, and classification, demonstrating polarimetry's role in planetary defense.
Contribution
First detailed spectropolarimetric analysis of NEA 2025 FA22, constraining its albedo and taxonomic class, and highlighting polarimetry's utility in rapid asteroid characterization.
Findings
Estimated albedo of 0.17 ± 0.04 in V band.
Most consistent with M-type asteroid classification.
Dense phase-polarization curve coverage during close approach.
Abstract
We report spectropolarimetric and broadband polarimetric observations of the near-Earth asteroid 2025 FA22 during its close approach of 18 September 2025 (about two Moon distances). With a diameter estimated between 130 and 290 m, 2025 FA22 is among the largest NEAs observable at such proximity, prompting an International AsteroidWarning Network (IAWN) rapid-response campaign. Although early orbital solutions indicated a possible impact in 2089, further follow-up astrometric observations ruled out collision hazard. The favourable geometry of this close encounter enabled a dense coverage of the positive part of the phase-polarisation curve, from the high polarisation domain (high phase angles), nearly to the inversion angle where the linear polarisation fraction vanishes. The spectropolarimetric observations provided the wavelength dependence of the polarisation fraction. Using empirical…
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