An equation of state of CO for use in planetary modeling

M. Podolak; A. Levi; A. Vazan; U. Malamud

doi:10.1016/j.icarus.2023.115424

An equation of state of CO for use in planetary modeling

M. Podolak, A. Levi, A. Vazan, U. Malamud

Tel Aviv University, Open University of Israel, Technion - Israel Institute of Technology

Research output: Contribution to journal › Article › peer-review

Abstract

Although carbon monoxide (CO) is an abundant molecule and may have great importance for planetary interiors, measurements of its properties are difficult due to its extreme volatility. We calculate the equation of state for CO over a range of temperature and density that is applicable to the conditions in planetary interiors. Previous experimental and theoretical studies cover only a limited temperature–density range. Our calculations match these early results well, but now cover the full range of relevance. The method of calculation is based on the general-purpose quotidian equation of state described by More et al. (1988), which is here used in order to generate a freely downloadable look-up table to be used by the community.

Original language	English
Article number	115424
Journal	Icarus
Volume	394
DOIs	https://doi.org/10.1016/j.icarus.2023.115424
State	Published - Apr 2023

Keywords

Carbon monoxide
Equation of state
Planetary interiors

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1016/j.icarus.2023.115424

Cite this

@article{030c6e4ee4874c7aaa118bbcc8a53b21,

title = "An equation of state of CO for use in planetary modeling",

abstract = "Although carbon monoxide (CO) is an abundant molecule and may have great importance for planetary interiors, measurements of its properties are difficult due to its extreme volatility. We calculate the equation of state for CO over a range of temperature and density that is applicable to the conditions in planetary interiors. Previous experimental and theoretical studies cover only a limited temperature–density range. Our calculations match these early results well, but now cover the full range of relevance. The method of calculation is based on the general-purpose quotidian equation of state described by More et al. (1988), which is here used in order to generate a freely downloadable look-up table to be used by the community.",

keywords = "Carbon monoxide, Equation of state, Planetary interiors",

author = "M. Podolak and A. Levi and A. Vazan and U. Malamud",

note = "Publisher Copyright: {\textcopyright} 2023 Elsevier Inc.",

year = "2023",

month = apr,

doi = "10.1016/j.icarus.2023.115424",

language = "الإنجليزيّة",

volume = "394",

journal = "Icarus",

issn = "0019-1035",

publisher = "Academic Press Inc.",

}

TY - JOUR

T1 - An equation of state of CO for use in planetary modeling

AU - Podolak, M.

AU - Levi, A.

AU - Vazan, A.

AU - Malamud, U.

PY - 2023/4

Y1 - 2023/4

N2 - Although carbon monoxide (CO) is an abundant molecule and may have great importance for planetary interiors, measurements of its properties are difficult due to its extreme volatility. We calculate the equation of state for CO over a range of temperature and density that is applicable to the conditions in planetary interiors. Previous experimental and theoretical studies cover only a limited temperature–density range. Our calculations match these early results well, but now cover the full range of relevance. The method of calculation is based on the general-purpose quotidian equation of state described by More et al. (1988), which is here used in order to generate a freely downloadable look-up table to be used by the community.

AB - Although carbon monoxide (CO) is an abundant molecule and may have great importance for planetary interiors, measurements of its properties are difficult due to its extreme volatility. We calculate the equation of state for CO over a range of temperature and density that is applicable to the conditions in planetary interiors. Previous experimental and theoretical studies cover only a limited temperature–density range. Our calculations match these early results well, but now cover the full range of relevance. The method of calculation is based on the general-purpose quotidian equation of state described by More et al. (1988), which is here used in order to generate a freely downloadable look-up table to be used by the community.

KW - Carbon monoxide

KW - Equation of state

KW - Planetary interiors

UR - http://www.scopus.com/inward/record.url?scp=85145857054&partnerID=8YFLogxK

U2 - 10.1016/j.icarus.2023.115424

DO - 10.1016/j.icarus.2023.115424

M3 - مقالة

SN - 0019-1035

VL - 394

JO - Icarus

JF - Icarus

M1 - 115424

ER -

An equation of state of CO for use in planetary modeling

Abstract

Keywords

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this