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Protocol for Measuring the Thermal Properties of a Supercooled Synthetic Sand-water-gas-methane Hydrate Sample
Published on: March 21, 2016
Spectroscopic Measurements of Methane Solid-Gas Equilibrium Clapeyron Curve between 40 and 77 K
Patrice Cacciani1, Peter Čermák1, Cédric Pardanaud2
1Laboratoire de Physique des Lasers, Atomes et Molécules , Université de Lille, CNRS, UMR 8523 , 59655 Villeneuve d'Ascq , France.
Researchers measured methane's solid-gas equilibrium curve using infrared spectroscopy. This study determined the vapor pressure and sublimation enthalpy of methane between 40-77 K.
Area of Science:
- Thermodynamics and Spectroscopy
- Planetary Science and Astrochemistry
Background:
- Methane (CH4) is a key molecule in planetary atmospheres and interstellar ices.
- Accurate thermodynamic data, particularly the solid-gas equilibrium, is crucial for modeling these environments.
- Previous measurements of methane's vapor pressure have limitations in temperature range and accuracy.
Purpose of the Study:
- To experimentally determine the Clapeyron solid-gas equilibrium curve for methane.
- To accurately measure methane's vapor pressure and sublimation enthalpy across a wide temperature range (40-77 K).
- To validate experimental results using two distinct optical setups and compare with existing literature data.
Main Methods:
- Utilized infrared gas-phase absorption spectroscopy to probe methane.
- Employed two cryogenically cooled experimental setups: a Fourier transform infrared spectrometer and a tunable laser source with a Herriott cell.
- Recorded methane absorption features from 40 K to 77 K.
Main Results:
- Derived the methane vapor pressure curve: ln(p/Pa) = -(1191.92 ± 8.92)/(T/K) + (22.49 ± 0.16) in the 40-77 K range.
- Calculated a sublimation enthalpy of 9910 ± 75 J mol⁻¹.
- Extended knowledge of methane saturation pressure by two orders of magnitude down to 40 K.
Conclusions:
- The derived vapor pressure relation provides a reliable thermodynamic dataset for methane.
- The experimental results align well with literature values and thermodynamic models.
- This study enhances our understanding of methane's behavior in low-temperature environments relevant to astrochemistry and planetary science.
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