Codes for two-component thermophysical analysis of asteroid (101955) Bennu
Authors/Creators
- 1. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
- 2. Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France
- 3. INAF – Osservatorio Astrofisico di Arcetri, Florence, Italy
Description
The codes in this folder allow fitting abundance of fine regolith and thermal inertia of rocks to the data collected by the OSIRIS-REx Thermal Emission Spectrometer using the method by Cambioni et al. 2019 [1] and analyze the results. The codes supports the findings of the paper: Cambioni, Delbo, Poggiali, Avdellidou, Ryan, Deshapriya, Asphaug, Ballouz, Barucci, Bennett, Bottke, Brucato, Burke, Cloutis, DellaGiustina, Emery, Rozitis, Walsh, Lauretta. "Fine-regolith production on asteroids controlled by rock porosity" (Submitted 2021-03-11).
[1] Cambioni, S., Delbo, M., Ryan, A. J., Furfaro, R. & Asphaug, E. Constraining the thermal properties of planetary surfaces using machine learning: Application to airless bodies. Icarus 325, 16–30 (2019).
Files
codes_and_data_Cambioni_etal.zip
Files
(205.1 MB)
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