A second planetesimal collision in the Fomalhaut system

The nearby star Fomalhaut is orbited by a compact source, Fomalhaut b, which has previously been interpreted as either a dust-enshrouded exoplanet or a dust cloud generated by the collision of two planetesimals. Such collisions are rarely observed, but their debris can appear in direct imaging. We report Hubble Space Telescope observations that show the appearance in 2023 of a second point source around Fomalhaut, resembling the appearance of Fomalhaut b 20 years earlier. We interpret this additional source as a dust cloud produced by a recent impact between two planetesimals. The positions and motion of two impact-generated dust clouds over 20 years provide constraints on the collisional dynamics in the debris belt.

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Publication Details

Journal
Science
Published
2025-12-18
DOI
https://doi.org/10.1126/science.adu6266
Citations
2
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
2.31
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article

A second planetesimal collision in the Fomalhaut system

Maxwell A. Millar‐Blanchaer, Robert J. De Rosa, Grant M. Kennedy, Thomas M. Esposito et al.
2 citations
Science
Stellar, planetary, and galactic studies
2.31
article

A second planetesimal collision in the Fomalhaut system

Maxwell A. Millar‐Blanchaer, Robert J. De Rosa, Grant M. Kennedy, Thomas M. Esposito, Paul Kalas, Bin Ren, M. C. Wyatt, Maximilian Sommer, Michael P. Fitzgerald, Jason Wang
article en
2 citations

Abstract

The nearby star Fomalhaut is orbited by a compact source, Fomalhaut b, which has previously been interpreted as either a dust-enshrouded exoplanet or a dust cloud generated by the collision of two planetesimals. Such collisions are rarely observed, but their debris can appear in direct imaging. We report Hubble Space Telescope observations that show the appearance in 2023 of a second point source around Fomalhaut, resembling the appearance of Fomalhaut b 20 years earlier. We interpret this additional source as a dust cloud produced by a recent impact between two planetesimals. The positions and motion of two impact-generated dust clouds over 20 years provide constraints on the collisional dynamics in the debris belt.

ScienceVol. 391(6783)
Northwestern University (US), University of California, Santa Barbara (US), University of California, Los Angeles (US), Xiamen University (CN), Malaghan Institute of Medical Research (NZ), Université Côte d'Azur (FR), University of Cambridge (GB), University of Warwick (GB), Max Planck Institute for Astronomy (DE), Observatoire de la Côte d’Azur (FR), European Southern Observatory (CL), Search for Extraterrestrial Intelligence (US), Foundation for Research and Technology Hellas (GR), University of California, Berkeley (US)
Openalex Percentile: Top 9%
Stellar, planetary, and galactic studies
2.31
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