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  5. Near-infrared Methanol Bands Probe Energetic Processing of Icy Outer Solar System Objects
 

Near-infrared Methanol Bands Probe Energetic Processing of Icy Outer Solar System Objects

Journal
THE ASTROPHYSICAL JOURNAL LETTERS  
Date Issued
2020
Author(s)
URSO, Riccardo Giovanni  
•
Baklouti, Donia
•
Djouadi, Zahia
•
Pinilla-Alonso, Noemí
•
Brunetto, Rosario
DOI
10.3847/2041-8213/ab8ad9
Abstract
Frozen methanol was detected in the outer solar system on the surfaces of the Centaur 5145 Pholus, the Trans-Neptunian Object (55638) 2002 VE95, and more recently on (486958) Arrokoth. The icy surfaces of these objects are subjected to solar and cosmic ions that modify the physico-chemical properties of their surface. To study the effects of ion bombardment on methanol-rich surfaces, we performed experiments of ion irradiation of H2O:CH3OH mixtures and we monitored the evolution of the methanol near-infrared bands. We observed significant variations of the 2.34/2.27 μm methanol band ratios as a function of the irradiation dose. We then used the Arrokoth and Pholus spectra to test the 2.34/2.27 μm band ratio as a probe of irradiation of methanol-rich surfaces, and we estimated the timescales of processing by solar and cosmic ions. Our results indicate that solar energetic particles are the main drivers of changes in the near-infrared spectra of frozen surfaces in the outer solar system.
Volume
894
Issue
1
Start page
L3
Uri
http://hdl.handle.net/20.500.12386/32726
Url
https://iopscience.iop.org/article/10.3847/2041-8213/ab8ad9
https://api.elsevier.com/content/abstract/scopus_id/85086328583
Issn Identifier
2041-8205
Ads BibCode
2020ApJ...894L...3U
Rights
open.access
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