Asteroid families are the remnant fragments of asteroids broken apart by collisions. There are only a few known Main Belt (MB) asteroid families with ages greater than 2 Gyr (Brož et al., 2013; Spoto et al., 2015). Estimates based on the family producing collision rate suggest that the lack of > 2 Gyr-old families may be due to a selection bias...
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May 30, 2018 (v1)PublicationUploaded on: December 4, 2022
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January 21, 2018 (v1)Journal article
International audience
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2018 (v1)Journal article
The debiased absolute-magnitude and orbit distributions as well as source regions for near-Earth objects (NEOs) provide a fundamental frame of reference for studies of individual NEOs and more complex population-level questions. We present a new four-dimensional model of the NEO population that describes debiased steady-state distributions of...
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February 2016 (v1)Journal article
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September 1, 2020 (v1)Journal article
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Uploaded on: December 4, 2022