Astrochemistry

Ethane Clathrate Hydrate Infrared Signatures For Solar System Remote Sensing

By Keith Cowing
astro-ph.EP
March 14, 2021
Filed under
Ethane Clathrate Hydrate Infrared Signatures For Solar System Remote Sensing
Temperature-dependent infrared spectra of the ethane clathrate in the fundamental modes regions. The crystalline pure ethane spectrum of Hudson et al. (2014) recorded at 15K is shown above. The infrared spectrum of an H2O:C2H6 (20:1) ice mixture from the Cosmic Ice Laboratory (Hudson et al., https://science.gsfc.nasa.gov/691/cosmicice/spectra.html), recorded at 20K, is shown above. The ethane:oxirane (7:3) mixed clathrate spectrum from Richardson et al. (1985) recorded at 90K is also shown. It is baseline corrected, and oxirane features are labelled with asterisks for clarity. Tentative assignments of the implied vibrational modes are given (see text for details). Spectra are offset for clarity.

Hydrocarbons such as methane and ethane are present in many solar system objects, including comets, moons and planets.

The interaction of these hydrocarbons with water ice at low temperatures could lead to the formation of inclusion compounds, such as clathrate hydrates (water based host cages trapping hydrocarbons guest molecules), modifying their retention, stability and therefore evolution. The occurrence of {\cor clathrate hydrates} on solar system surfaces could be established by remote sensing of their spectroscopic signatures.

In this study, we measure and analyse ethane clathrate hydrate spectra recorded in the temperature range from 5.3 to 160K, covering most of the temperature range of interest for solar system objects. Specific infrared band signatures are identified for the ethane encaged guest. We provide evidence that ethane clathrate hydrate outcrops can be detected by remote sensing on the surface of planetary bodies.

Emmanuel Dartois, François Langlet

Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Journal reference: Icarus 357 (2021) 114255
DOI: 10.1016/j.icarus.2020.114255
Cite as: arXiv:2103.04928 [astro-ph.EP] (or arXiv:2103.04928v1 [astro-ph.EP] for this version)
Submission history
From: Emmanuel Dartois
[v1] Mon, 8 Mar 2021 17:39:53 UTC (1,127 KB)
https://arxiv.org/abs/2103.04928
Astrobiology, Astrochemistry

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