elib
DLR-Header
DLR-Logo -> http://www.dlr.de
DLR Portal Home | Impressum | Datenschutz | Kontakt | English
Schriftgröße: [-] Text [+]

Thermal Properties of the Mojave Mars Regolith Simulant in Mars-Like Atmospheric Conditions

Nagihara, S. und Ngo, Peter und Grott, Matthias (2022) Thermal Properties of the Mojave Mars Regolith Simulant in Mars-Like Atmospheric Conditions. International Journal of Thermophysics, 43 (98). Springer. doi: 10.1007/s10765-022-03023-y. ISSN 0195-928X.

[img] PDF - Nur DLR-intern zugänglich - Verlagsversion (veröffentlichte Fassung)
2MB

Offizielle URL: https://link.springer.com/article/10.1007/s10765-022-03023-y

Kurzfassung

On Mars, thermal conductivity of regolith may vary with atmospheric conditions. When atmospheric pressure rises, the regolith’s pore gas pressure also increases, and that results in greater thermal conductivity, and vice versa. Atmospheric temperature fluctuation may also influence thermal properties of the regolith. In recent robotic Mars-landing missions, in-situ measurements of regolith thermal properties and heat flow have been attempted. The challenges for the in-situ measurements on these missions is that they may be able to capture only a snapshot of the regolith properties while they would continuously fluctuate with the atmospheric conditions. To support these in-situ measurement efforts, we attempted to characterize the possible annual variation of thermal properties of Mars regolith due to seasonal pore gas pressure and temperature fluctuations, using the Mojave Mars simulant (MMS) in Mars-like atmospheric conditions. Two batches of samples with differing densities (1540 kg·m−3 and 1660 kg·m−3) were placed in a thermal vacuum chamber, one at a time, filled with CO2 gas, and their thermal conductivity was measured by the hotwire and the dual-probe heat pulse (DPHP) methods. Their specific heat was measured by the DPHP method. Because these two methods were originally developed for Earth’s soils that have much greater thermal conductivity than the regolith on Mars, we modified their standard data reductions schemes, aided by finite-element thermal modeling of the individual measurement experiments. We found that thermal conductivity of MMS increased by~20 % from 600 Pa to 1000 Pa, the range of atmospheric pressure observed by the current and the previous Mars missions. We also found that specific heat of MMS increased by ~16 % from~− 30 °C (243 K) to 30 °C (303 K). Thermal diffusivity, which is the primary control factor of the thermal skin depth, could vary by 20 % to 25 % in the range of CO2 pressures and temperatures the MMS samples were tested .

elib-URL des Eintrags:https://elib.dlr.de/186334/
Dokumentart:Zeitschriftenbeitrag
Titel:Thermal Properties of the Mojave Mars Regolith Simulant in Mars-Like Atmospheric Conditions
Autoren:
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID-iDORCID Put Code
Nagihara, S.Texas Tech Univ.NICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Ngo, PeterHoneybee Robotics, Altadena, CA 91001, USANICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Grott, MatthiasMatthias.Grott (at) dlr.dehttps://orcid.org/0000-0002-8613-7096NICHT SPEZIFIZIERT
Datum:3 Mai 2022
Erschienen in:International Journal of Thermophysics
Referierte Publikation:Ja
Open Access:Nein
Gold Open Access:Nein
In SCOPUS:Ja
In ISI Web of Science:Ja
Band:43
DOI:10.1007/s10765-022-03023-y
Verlag:Springer
ISSN:0195-928X
Status:veröffentlicht
Stichwörter:Mars Regolith Wärmeleitfähigkeit Geophysik
HGF - Forschungsbereich:Luftfahrt, Raumfahrt und Verkehr
HGF - Programm:Raumfahrt
HGF - Programmthema:Erforschung des Weltraums
DLR - Schwerpunkt:Raumfahrt
DLR - Forschungsgebiet:R EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):R - Projekt InSight - HP3
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetare Sensorsysteme
Hinterlegt von: Grott, Dr.rer.nat. Matthias
Hinterlegt am:17 Mai 2022 09:29
Letzte Änderung:20 Okt 2023 07:30

Nur für Mitarbeiter des Archivs: Kontrollseite des Eintrags

Blättern
Suchen
Hilfe & Kontakt
Informationen
electronic library verwendet EPrints 3.3.12
Gestaltung Webseite und Datenbank: Copyright © Deutsches Zentrum für Luft- und Raumfahrt (DLR). Alle Rechte vorbehalten.