Calculated Diffusivities for Water Isotopologues in Carbon Dioxide, Nitrogen, and the Atmosphere of Mars, and for Methane Isotopologues in Nitrogen Representing the Atmosphere of Titan
Data and Resources
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SHA256 File for Readme fileTEXT
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Readme fileTEXT
Readme file
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SHA256 File for DIffusivity of H2OTEXT
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DIffusivity of H2OBIN
DIffusivity of the H2O molecule in CO2, N2, and the Martian atmosphere
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SHA256 File for Diffusivity of HDOTEXT
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Diffusivity of HDOBIN
DIffusivity of the HDO molecule in CO2, N2, and the Martian atmosphere
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SHA256 File for Diffusivity of H2-17OTEXT
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Diffusivity of H2-17OBIN
Diffusivity of the H2-17O molecule in CO2, N2, and the Martian atmosphere
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SHA256 File for Diffusivity of H2-18OTEXT
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Diffusivity of H2-18OBIN
Diffusivity of the H2-18O molecule in CO2, N2, and the Martian atmosphere
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SHA256 File for Diffusivity of CH4TEXT
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Diffusivity of CH4BIN
Diffusivity of the CH4 molecule in N2 (atmosphere of Titan)
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SHA256 File for Diffusivity of CH3DTEXT
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Diffusivity of CH3DBIN
Diffusivity of the CH3D molecule in N2 (atmosphere of Titan)
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SHA256 File for Diffusivity of 13-CH4TEXT
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Diffusivity of 13-CH4BIN
Diffusivity of the 13-CH4 molecule in N2 (atmosphere of Titan)
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DOI Access for Calculated Diffusivities for...
| Field | Value |
|---|---|
| accessLevel | public |
| bureauCode | {006:55} |
| catalog_@context | https://project-open-data.cio.gov/v1.1/schema/data.json |
| catalog_conformsTo | https://project-open-data.cio.gov/v1.1/schema |
| catalog_describedBy | https://project-open-data.cio.gov/v1.1/schema/catalog.json |
| identifier | ark:/88434/mds2-2351 |
| issued | 2021-01-28 |
| language | {en} |
| license | https://www.nist.gov/open/license |
| modified | 2021-04-19 00:00:00 |
| programCode | {006:045} |
| publisher | National Institute of Standards and Technology |
| resource-type | Dataset |
| source_datajson_identifier | true |
| source_hash | 3fc6726a8d682287917f2460ec4ebd0690065bfd |
| source_schema_version | 1.1 |
| theme | {"Physics:Atomic, molecular, and quantum","Chemistry:Chemical thermodynamics and chemical properties","Chemistry:Theoretical chemistry and modeling"} |
| Groups |
|
| Tags |
|
| isopen | False |
| license_id | other-license-specified |
| license_title | other-license-specified |
| maintainer | Allan H. Harvey |
| maintainer_email | allan.harvey@nist.gov |
| metadata_created | 2025-11-19T14:22:51.515152 |
| metadata_modified | 2025-11-19T14:22:51.515158 |
| notes | Values are computed for the dilute-gas diffusivity of water isotopologues in N2, CO2, and their mixture at a composition representing the atmosphere of Mars, for standard conditions of 101.325 kPa and water mole fraction approaching zero. Values are similarly computed for the diffusivity of methane isotopologues in N2, representing the atmosphere of Titan. Calculations employ state-of-the-art intermolecular potentials and classical trajectory calculations as described in the paper by R. Hellmann and A.H. Harvey, "First-Principles Diffusivity Ratios for Atmospheric Isotope Fractionation on Mars and Titan", published in Journal of Geophysical Research: Planets, 126, e2021JE006857 (2021), https://doi.org/10.1029/2021JE006857. Separate files are given for the diffusivities of H2O, HDO (where D is deuterium), and the 17-O and 18-O substitutions of H2O, and for the diffusivities in N2 of CH4, CH3D, and the 13-C substitution of CH4. |
| num_resources | 17 |
| num_tags | 17 |
| title | Calculated Diffusivities for Water Isotopologues in Carbon Dioxide, Nitrogen, and the Atmosphere of Mars, and for Methane Isotopologues in Nitrogen Representing the Atmosphere of Titan |