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Rivkin, Andrew S.; Thomas, Cristina A.; Wong, Ian; Rozitis, Benjamin; de León, Julia; Holler, Bryan; Milam, Stefanie N.; Howell, Ellen S.; Hammel, Heidi B.; Arredondo, Anicia; Brucato, John R.; Epifani, Elena M.; Ieva, Simone; La Forgia, Fiorangela; Lucas, Michael P.; Lucchetti, Alice; Pajola, Maurizio; Poggiali, Giovanni; Sunshine, Jessica N. and Trigo-Rodríguez, Josep M.
(2023).
DOI: https://doi.org/10.3847/psj/ad04d8
Abstract
The Didymos binary asteroid was the target of the Double Asteroid Redirection Test (DART) mission, which intentionally impacted Dimorphos, the smaller member of the binary system. We used the Near-Infrared Spectrograph and Mid-Infrared Instrument instruments on JWST to measure the 0.6–5 and 5–20 μm spectra of Didymos approximately two months after the DART impact. These observations confirm that Didymos belongs to the S asteroid class and is most consistent with LL chondrite composition, as was previously determined from its 0.6–2.5 μm reflectance spectrum. Measurements at wavelengths >2.5 μm show Didymos to have thermal properties typical for an S-complex asteroid of its size and to be lacking absorptions deeper than ∼2% due to OH or H2O. Didymos’ mid-infrared emissivity spectrum is within the range of what has been measured on S-complex asteroids observed with the Spitzer Space Telescope and is most consistent with emission from small (<25 μm) surface particles. We conclude that the observed reflectance and physical properties make the Didymos system a good proxy for the type of ordinary chondrite asteroids that cross near-Earth space, and a good representative of likely future impactors.
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