Hydroxylated Mg-rich Amorphous Silicates: A New Component of the 3.2 μ m Absorption Band of Comet 67P/Churyumov–Gerasimenko

Autor: Mennella, V., Ciarniello, M., Raponi, A., Capaccioni, F., Filacchione, G., Suhasaria, T., Popa, C., Kappel, D., Moroz, L., Vinogradoff, V., Pommerol, A., Rousseau, Batiste, Istiqomah, I., Quirico, E, Beck, P, Bockelée-Morvan, D., Carlson, R., Pilorget, C.

Publikováno v: The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 897 (2), pp.L37. ⟨10.3847/2041-8213/ab919e⟩
The Astrophysical journal letters, 2020, 897 (2), pp.L37. ⟨10.3847/2041-8213/ab919e⟩

International audience; The VIRTIS imaging spectrometer on board Rosetta has shown that the nucleus surface of comet 67P/ Churyumov-Gerasimenko (67P/CG) is characterized by a broad absorption band at around 3.2 μm. The feature is ubiquitous across t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae5371e5e743b5dd07e3f9f8630e621d
https://hal.archives-ouvertes.fr/hal-02996616