journal article·2017-01-01Open access

Thermal conductivity model for powdered materials under vacuum based on experimental studies

N. Sakatani, K. Ogawa, Y. Iijima, M. Arakawa, R. Honda, S. Tanaka

AIP Advances· Volume 7· Issue 1

Abstract

The thermal conductivity of powdered media is characteristically very low in vacuum, and is effectively dependent on many parameters of their constituent particles and packing structure. Understanding of the heat transfer mechanism within powder layers in vacuum and theoretical modeling of their thermal conductivity are of great importance for several scientific and engineering problems. In this paper, we report the results of systematic thermal conductivity measurements of powdered media of varied particle size, porosity, and temperature under vacuum using glass beads as a model material. Based on the obtained experimental data, we investigated the heat transfer mechanism in powdered media in detail, and constructed a new theoretical thermal conductivity model for the vacuum condition. This model enables an absolute thermal conductivity to be calculated for a powder with the input of a set of powder parameters including particle size, porosity, temperature, and compressional stress or gravity, and vice versa. Our model is expected to be a competent tool for several scientific and engineering fields of study related to powders, such as the thermal infrared observation of air-less planetary bodies, thermal evolution of planetesimals, and performance of thermal insulators and heat storage powders.
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Research context

OpenAlex topics: Spacecraft and Cryogenic Technologies · Gas Dynamics and Kinetic Theory · High-pressure geophysics and materials

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Meiji University 1 Department of Physics, School of Science and Technology, , 1-1-1 Higashi-Mita, Tama-ku, Kawasaki, Kanagawa 214-8571, Japan

Kobe University 2 Department of Planetology, Graduate School of Science, , 1-1 Rokkodai-cho, Nada-ku, Kobe, Hyogo 657-8501, Japan

Japan Aerospace Exploration Agency 3 Institute of Space and Astronautical Science, , 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan

Kochi University 4 Department of Information Science, Faculty of Science, , 2-5-1 Akebono-cho, Kochi 780-8520, Japan

Funding

Japan Society for the Promotion of Science

References (44)

Show source-provided references
1. Thermal fatigue as the origin of regolith on small asteroids10.1038/nature13153 ↗
2. Thermal properties of granulated materials10.2514/5.9781600865022.0215.0241 ↗
3. Thermal conductivity measurements of particulate materials: 1. A review10.1029/96JE03302 ↗
4. Thermal conductivity measurements of particulate materials: 2. Results10.1029/96JE03303 ↗
5. Correlation of mechanical and thermal properties of the lunar surface10.1016/0019-1035(69)90020-7 ↗
6. Conductance of packed spheres in vacuum10.1115/1.3450056 ↗
7. Heat conductivity and nature of the lunar surface material
8. Thermal conductivity of packed beds10.1002/aic.690060113 ↗
9. Thermal conduction through an evacuated idealized powder over the temperature range of 100° to 500 °K
10. Thermal conductivity of particulate basalt as a function of density in simulated lunar and martian environments10.1029/JB075i020p04063 ↗
11. Determination of the effective thermal conductivity of granular materials under varying pressure conditions10.1029/2008je003085 ↗
12. Thermal conductivity measurements of porous dust aggregates: I. Technique, model and first results10.1016/j.icarus.2011.04.024 ↗
13. Outgassing of Icy bodies in the solar system - II: Heat transport in dry, porous surface dust layers10.1016/j.icarus.2012.03.013 ↗
14. Experimental study for thermal conductivity structure of lunar surface regolith: Effect of compressional stress10.1016/j.icarus.2012.08.037 ↗
15. Compressional stress effect on thermal conductivity of powdered materials: Measurements and their implication to lunar regolith10.1016/j.icarus.2015.12.012 ↗
16. K. Watson, “I. The thermal conductivity measurements of selected silicate powders in vacuum from 150° - 350 ° K, II. An interpretation of the Moon’s eclipse and lunartion cooling as observed through the Earth’s atmosphere from 8–14 microns,” Ph.D. thesis, Calif. Inst. of Technol., Pasadena, California, 1964.
17. A model of thermal conductivity for planetary soils: 1. theory for unconsolidated soils10.1029/2008JE003308 ↗
18. 1959
19. Approximate expressions for retarded van der waals interaction10.1016/0021-9797(81)90018-7 ↗
20. Surface cleanliness effect on lunar soil shear strength10.1061/(asce)1090-0241(2001)127:4(371) ↗
21. Thermal contact conductance10.1016/0017-9310(69)90011-8 ↗
22. 2000
23. Imaging surface contacts: Power law contact distributions and contact stresses in quartz, calcite, glass and acrylic plastic10.1016/0040-1951(95)00165-4 ↗
24. 2014
25. A study of coordination number in a rondom packed system of monosized sphere particles (in Japanese)10.1252/kakoronbunshu.6.59 ↗
26. 2006
27. 1951
28. Surface energy and the contact of elastic solids10.1098/rspa.1971.0141 ↗
29. 2013
30. Heat-flow experiment
31. Heat-flow experiment
32. Surface brightness temperature at the apollo 17 heat flow site: Thermal conductivity of the upper 15 cm of regolith
33. The lunar reconnaissance orbiter diviner lunar radiometer experiment10.1007/s11214-009-9529-2 ↗
34. Lunar equatorial surface temperatures and regolith properties from the diviner lunar radiometer experiment10.1029/2011je003987 ↗
35. Lunar cold spots: Granular flow features and extensive insulating materials surrounding young craters10.1016/j.icarus.2013.12.017 ↗
36. Thermal infrared imaging experiments of C-type asteroid 162173 Ryugu on Hayabusa210.1007/s11214-016-0286-8 ↗
37. Numerical simulation of dust aggregate collisions. II. Compression and disruption of three-dimensional aggregates in head-on collisions10.1086/529511 ↗
38. Rapid coagulation of porous dust aggregates outside the snow line: A pathway to successful Icy planetesimal formation10.1088/0004-637X/752/2/106 ↗
39. Fluffy dust forms Icy planetesimals by static compression10.1051/0004-6361/201322151 ↗
40. Thermal evolution models of asteroids
41. Thermal evolution and sintering of chondritic planetesimals10.1051/0004-6361/201117177 ↗
42. Differentiation and core formation in accreting planetesimals10.1051/0004-6361/201219157 ↗
43. Thermal conductivity of evacuated perlite at low temperatures as a function of load and load history10.1016/0011-2275(91)90183-W ↗
44. A thermal control system for long-term survival of scientific instruments on lunar surface10.1063/1.4867906 ↗