28 février 2024 à 1 mars 2024
Institut d'Astrophysique de Paris
Fuseau horaire Europe/Paris

Characterization and comparison of sample returns from the C-type asteroids Ryugu and Bennu

29 févr. 2024, 16:30
15m
Amphithéâtre Henri Mineur (Institut d'Astrophysique de Paris)

Amphithéâtre Henri Mineur

Institut d'Astrophysique de Paris

Institut d'astrophysique de Paris 98 bis Boulevard Arago 75014 PARIS
Oral presentation Session 8

Orateur

Laura Nardelli (IAS)

Description

Primitive asteroids are remnants of the early stage of the Solar System evolution and may have preserved the mineralogical and molecular phases formed during this period.
In 2020, the Hayabusa2 mission of JAXA brought back to Earth, samples from the C-type asteroid Ryugu, a primitive near-Earth object, collected at two different locations and depths. The samples are now preserved and submitted to a first round of analyses at the ISAS Curation center (Sagamihara, Japan) under an ultraclean nitrogen purged chamber to prevent H2O/CO2 contamination. In particular, the MicrOmega instrument, a NIR hyperspectral microscope conceived at IAS, contributes to the characterization of the returned samples (e.g. Pilorget et al. 2022). Recently, the NASA mission OSIRIS-REx also brought back samples from the near-Earth primitive asteroid Bennu (Lauretta et al. 2022). A fraction of these samples will be transferred to ISAS in a Curation Facility similar to that of Ryugu samples, allowing us to characterize, with MicrOmega, the mineralogical and molecular composition of the grains in the same conditions as for Ryugu samples. The comparison between these two asteroids samples using the same instrument under the sames measurements conditions will allow us to better constrain the genericity or specificity of the processes identified.

Day constraints

not Wednesday 28 morning

Astrophysics Field Planetology (including small bodies and exoplanets)

Auteur principal

Documents de présentation

Aucun document.