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March 13, 2023 (v1)Conference paperUploaded on: November 25, 2023
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January 2023 (v1)Journal article
Context. Observational and instrumental difficulties observing small bodies below 0.5 μm make this wavelength range poorly studied compared with the visible and near-infrared. Furthermore, the suitability of many commonly used solar analogues, essential in the computation of asteroid reflectances, is usually assessed only in visible...
Uploaded on: February 22, 2023 -
September 21, 2020 (v1)Journal article
When rubble-pile asteroid 2008 TC3 impacted Earth on October 7, 2008, the recovered rockfragments indicated that such asteroids can contain exogenic material [1,2]. However,spacecraft missions to date have only observed exogenous contamination on large,monolithic asteroids that are impervious to collisional disruption [3, 4]. Here we report...
Uploaded on: December 4, 2022 -
April 2019 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
October 8, 2020 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2023 (v1)Journal article
Context. Quaoar is a classical trans-Neptunian object (TNO) with an area-equivalent diameter of 1100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultations observed between 2018 and 2021, an inhomogeneous ring (Q1R, i.e., Quaoar's first ring) has been detected around this body. Aims: A new stellar...
Uploaded on: March 3, 2024 -
2024 (v1)Journal article
International audience
Uploaded on: October 9, 2024