The effect of salt crust on the thermal conductivity of one sample of fluvial particulate materials under Martian atmospheric pressures

نویسندگان

  • Marsha A. Presley
  • Robert A. Craddock
  • Natalya Zolotova
چکیده

[1] A line-heat source apparatus was used to measure thermal conductivities of a lightly cemented fluvial sediment (salinity = 1.1 g kg ), and the same sample with the cement bonds almost completely disrupted, under low pressure, carbon dioxide atmospheres. The thermal conductivities of the cemented sample were approximately 3 higher, over the range of atmospheric pressures tested, than the thermal conductivities of the same sample after the cement bonds were broken. A thermal conductivity-derived particle size was determined for each sample by comparing these thermal conductivity measurements to previous data that demonstrated the dependence of thermal conductivity on particle size. Actual particle-size distributions were determined via physical separation through brass sieves. When uncemented, 87% of the particles were less than 125 mm in diameter, with 60% of the sample being less than 63 mm in diameter. As much as 35% of the cemented sample was composed of conglomerate particles with diameters greater than 500 mm. The thermal conductivities of the cemented sample were most similar to those of 500-mm glass beads, whereas the thermal conductivities of the uncemented sample were most similar to those of 75-mm glass beads. This study demonstrates that even a small amount of salt cement can significantly increase the thermal conductivity of particulate materials, as predicted by thermal modeling estimates by previous investigators.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Thermal Conductivity Measurements of Natural Eolian and Fluvial

Introduction: The particle size of surficial materials may provide important clues about the history of erosion, transport, and depositional processes that have acted to form the deposit. Particle size may also provide a valuable clue about the genesis of those deposits. On Mars, most of the surface is covered with at least a thin coating of various particulate materials that tend to obscure di...

متن کامل

Thermal Conductivity Studies of Sedimentary Materials from Central Australia and the Implications for Mars

Introduction: In the search for life on Mars, investigating fluvial deposits will be a high priority for future landers. Although there is abundant evidence that fluvial processes worked with great intensity in the past (e.g., outflow channels, valley networks, and modified impact craters), aeolian processes dominate under the current environmental conditions. In fact there is evidence that ext...

متن کامل

AN INVESTIGATION ON EFFECT OF BOND COAT REPLACEMENT ON HOT CORROSION PROPERTIES OF THERMAL BARRIER COATINGS

In the present study NiCrAlY bond coating layer was produced by electroplating against common atmospheric plasma spraying (APS). Both types of the bond coats were applied on IN738LC base metal then, the YSZ (ZrO2-8% Y2O3) thermal barrier top layer was coated by atmospheric plasma spray technique. Hot corrosion is one of the main destructive factors in thermal barrier coatings (TBCs) which come ...

متن کامل

Numerical Investigation of Roofing Materials Effect on Solar Heat Gain in Different External Conditions

In this study, the thermal performance of three kinds of roofs with different heat capacity and thermal conductivity under different external conditions has been investigated using a numerical method. For this purpose, the combined solar radiation, conduction and convection heat transfer were calculated implicitly in terms of a one-dimensional finite difference method. Different high and low so...

متن کامل

Experimental Constraints on the Thermal Structure of the Martian Interior and Martian Magmatism

Introduction: Past space missions to Mars have provided important constraints on the planet's internal density distribution [1,2]. However, the thermal structure of the Martian interior remains highly uncertain. Although theoretical calculations have provided some basic knowledge of the thermal evolution of Mars [e.g., 3-9], the results from these computer simulations are strongly dependent on ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009