TY - JOUR
T1 - Thermal Conductivity and Compressional Velocity of Methane at High Pressure
T2 - Insights Into Thermal Transport Properties of Icy Planet Interiors
AU - Meyer, Dylan W.
AU - Hsieh, Wen Pin
AU - Hsu, Han
AU - Kuo, Ching Yi
AU - Lin, Jung Fu
N1 - Publisher Copyright:
© 2022. American Geophysical Union. All Rights Reserved.
PY - 2022/3
Y1 - 2022/3
N2 - Methane is a primary component of the “ice” layers in icy bodies whose thermal transport properties and velocity-density profiles are essential to understanding their unique geodynamic and physiochemical phenomena. We present experimental measurements of methane's thermal conductivity and compressional velocity to 25.1 and 45.1 GPa, respectively, at room temperature, and theoretical calculations of its equation of state, velocity, and heat capacity up to 100 GPa and 1200 K. Overall, these properties change smoothly with pressure and are generally unaffected by the imposed atomic structure; though we observe a discrete spike in conductivity near the I-A phase boundary. We cross-plot the thermal conductivity and compressional velocity with density for the primary “ice” constituents (methane, water, and ammonia) and find that methane and water are the upper and lower bounds, respectively, of conductivity and velocity in these systems. These physical properties provide critical insights that advance the modeling of thermo-chemical structures and dynamics within icy bodies.
AB - Methane is a primary component of the “ice” layers in icy bodies whose thermal transport properties and velocity-density profiles are essential to understanding their unique geodynamic and physiochemical phenomena. We present experimental measurements of methane's thermal conductivity and compressional velocity to 25.1 and 45.1 GPa, respectively, at room temperature, and theoretical calculations of its equation of state, velocity, and heat capacity up to 100 GPa and 1200 K. Overall, these properties change smoothly with pressure and are generally unaffected by the imposed atomic structure; though we observe a discrete spike in conductivity near the I-A phase boundary. We cross-plot the thermal conductivity and compressional velocity with density for the primary “ice” constituents (methane, water, and ammonia) and find that methane and water are the upper and lower bounds, respectively, of conductivity and velocity in these systems. These physical properties provide critical insights that advance the modeling of thermo-chemical structures and dynamics within icy bodies.
KW - compressional velocity
KW - icy planets
KW - solid methane
KW - thermal conductivity
UR - http://www.scopus.com/inward/record.url?scp=85127231574&partnerID=8YFLogxK
U2 - 10.1029/2021JE007059
DO - 10.1029/2021JE007059
M3 - 期刊論文
AN - SCOPUS:85127231574
SN - 2169-9097
VL - 127
JO - Journal of Geophysical Research: Planets
JF - Journal of Geophysical Research: Planets
IS - 3
M1 - e2021JE007059
ER -