Thermal conductivity measurements of porous dust aggregates: I. Technique, model and first results

Icarus

Volumn 214, Issue 1, 2011, Pages 286-296

  Krause, M ^a   Blum, J ^a   Skorov, Yu V ^a   Trieloff, M ^b  

^a TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

^b UNIVERSITY OF HEIDELBERG   (Germany)

Author keywords

Comets, Dust; Comets, Origin; Origin, Solar System; Planetary formation; Planetesimals; Regoliths

Indexed keywords

EID: 79959557452     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2011.04.024     Document Type: Article

References (48)

1. Bar-Nun A., Laufer D. First experimental studies of large samples of gas-laden amorphous "cometary" ices. Icarus 2003, 161:157-163.
2. Blum J., Schräpler R. Structure and mechanical properties of high-porosity macroscopic agglomerates formed by random ballistic deposition. Phys. Rev. Lett. 2004, 93:115503-1-115503-4.
3. Blum J., Schräpler R., Davidsson B.J.R., Trigo-Rodríguez J.M. The physics of protoplanetesimal dust agglomerates. I. Mechanical properties and relations to primitive bodies in the Solar System. Astrophys. J. 2006, 652:1768-1781.
4. Capria M.T., Coradini A., de Sanctis M.C. A model of the activity of Comet Wild 2. Adv. Space Res. 2002, 29:709-714.
5. Cheng S.C., Vachon R.I. A technique for predicting the thermal conductivity of suspensions, emulsions and porous materials. Int. J. Heat Mass Transfer 1970, 13:537-546.
6. Davidsson B.J.R., Skorov Y.V. On the light-absorbing surface layer of cometary nuclei II. Thermal modeling. Icarus 2002, 159:239-258.
7. Davidsson B.J.R., Gutiérrez P.J., Rickman H. Physical properties of morphological units on Comet 9P/Tempel 1 derived from near-IR Deep Impact spectra. Icarus 2009, 201:335-357.
8. Davis T.A. UMFPACK V4.3, an unsymmetric-pattern multifrontal method with a column pre-ordering strategy. ACM Trans. Math. Softw. 2004, 30:196.
9. Desch S.J. Mass distribution and planet formation in the solar nebula. Astrophys. J. 2007, 671:878-893.
10. Fayette S., Smith D.S., Smith A., Martin C. Influence of grain size on the thermal conductivity of tin oxide ceramics. J. Eur. Ceram. Soc. 2000, 20:297-302.
11. Ghosh A., McSween H.Y. A thermal model for the differentiation of Asteroid 4 Vesta, based on radiogenic heating. Icarus 1998, 134:187-206.
12. Ghosh A., Weidenschilling S.J., McSween H.Y. Importance of the accretion process in asteroid thermal evolution: 6 Hebe as an example. Meteorit. Planet. Sci. 2003, 38:711-724.
13. Ghosh A., Weidenschilling S.J., McSween H.Y., Rubin A. Asteroidal heating and thermal stratification of the asteroidal belt. Meteorites and the Early Solar System II 2006, 555-566. Univ. of Arizona Press, Tucson. D.S. Lauretta, H.Y. McSween (Eds.).
14. Göpel C., Manhes G., Allegre C.J. U-Pb systematics of phosphates from equilibrated ordinary chondrites. Earth Planet. Sci. Lett. 1994, 121:153-171.
15. Groussin O., A'Hearn M.F., Li J., Thomas P.C., Sunshine J.M., Lisse C.M., Meech K.J., Farnham T.L., Feaga L.M., Delamere W.A. Surface temperature of the nucleus of Comet 9P/Tempel 1. Icarus 2007, 187:16-25.
16. Güttler C., Blum J., Zsom A., Ormel C.W., Dullemond C.P. The outcome of protoplanetary dust growth: Pebbles, boulders, or planetesimals?. I. Mapping the zoo of laboratory collision experiments. Astron. Astrophys. 2010, 513:A56.
17. Hevey P.J., Sanders I.S. A model for planetesimal meltdown by 26Al and its implications for meteorite parent bodies. Meteorit. Planet. Sci. 2006, 41:95-106.
18. Huetter E.S., Koemle N.I., Kargl G., Kaufmann E. Determination of the effective thermal conductivity of granular materials under varying pressure conditions. J. Geophys. Res. (Planet) 2008, 113:E12004.
19. Kleine T., Touboul M., van Orman J.A., Bourdon B., Maden C., Mezger K., Halliday A.N. Hf W thermochronometry: Closure temperature and constraints on the accretion and cooling history of the H chondrite parent body. Earth Planet. Sci. Lett. 2008, 270:106-118.
20. Kossacki K.J., Koemle N.I., Kargl G., Steiner G. The influence of grain sintering on the thermoconductivity of porous ice. Planet. Space Sci. 1994, 42:383-389.
21. Kührt E., Keller H.U., Lorenz E. Interpretation of surface temperatures and activity of KOSI samples. Planet. Space Sci. 1995, 43:333-340.
22. Masamune S., Smith J.M. Thermal conductivity of beds of spherical particles. Ind. Eng. Chem. Fund. 1963, 2:136-143.
23. McSween H.Y., Ghosh A., Grimm R.E., Wilson L., Young E.D. Thermal evolution models of asteroids. Asteroids 2002, III:559-571.
24. Merk R., Prialnik D. Early thermal and structural evolution of small bodies in the trans-neptunian zone. Earth Moon Planets 2003, 92:359-374.
25. Merk R., Prialnik D. Combined modeling of thermal evolution and accretion of trans-neptunian objects-Occurrence of high temperatures and liquid water. Icarus 2006, 183:283-295.
26. Merrill, R.B., 1969. Thermal Conduction through an Evacuated Idealized Powder over the Temperature range of 100° to 500°K. NASA Technical Note D-5063.
27. Miyamoto M., Fujii N., Takeda H. Ordinary chondrite parent body: An internal heating model. Proc. Lunar Sci. Conf. 1981, 12B:1145-1152.
28. Parker W.J., Jenkins R.J., Bulter C.P., Abbott G.L. Flash method of determining thermal diffusivity, heat capacity, and thermal conductivity. J. Appl. Phys. 1961, 32:1679-1684.
29. Paton M.D., Kargl G., Ball A.J., Green S.F., Hagermann A., Kömle N.I., Thiel M., Zarnecki J.C. Computer modelling of a penetrator thermal sensor. Adv. Space Res. 2010, 46:337-345.
30. Poppe T. Sintering of highly porous silica-particle samples: Analogues of early Solar System aggregates. Icarus 2003, 164:139-148.
31. Presley M.A., Christensen P.R. Thermal conductivity measurements of particulate materials 1. A review. J. Geophys. Res. 1997, 102:6535-6550.
32. Presley M.A., Christensen P.R. Thermal conductivity measurements of particulate materials 2. Results. J. Geophys. Res. 1997, 102:6551-6566.
33. Prialnik D., Podolak M. Changes in the structure of comet nuclei due to radioactive heating. Space Sci. Rev. 1999, 90:169-178.
34. Prialnik D., Sarid G., Rosenberg E.D., Merk R. Thermal and chemical evolution of comet nuclei and Kuiper Belt objects. Space Sci. Rev. 2008, 138:147-164.
35. Progelhof R.C., Throne J.L., Ruetsch R.R. Methods for predicting the thermal conductivity of composite systems: A review. Polym. Eng. Sci. 1976, 16:615-625.
36. Russell H.W. Principles of heat flow in porous insulators*. J. Am. Ceram. Soc. 1935, 18:1-5.
37. Schaertl W., Sillescu H. Brownian dynamics of polydisperse colloidal hard spheres: Equilibrium structures and random close packings. J. Statist. Phys. 1994, 77:1007-1025.
38. Scott E.R.D. Meteoritical and dynamical constraints on the growth mechanisms and formation times of asteroids and Jupiter. Icarus 2006, 185:72-82.
39. Seiferlin K., Spohn T., Benkhoff J. Cometary ice texture and the thermal evolution of comets. Adv. Space Res. 1995, 15:35-38.
40. Seiferlin K., Kömle N.I., Kargl G., Spohn T. Line heat-source measurements of the thermal conductivity of porous H2O ice, CO2 ice and mineral powders under space conditions. Planet. Space Sci. 1996, 44:691-704.
41. Tipler P. Physics for Scientists and Engineers 1999, W.H. Freeman. fourth ed.
42. Tishkovets V.P., Jockers K. Multiple scattering of light by densely packed random media of spherical particles: Dense media vector radiative transfer equation. J. Quant. Spectrosc. Radiat. Transfer 2006, 101:54-72.
43. Trieloff, M., 2009. Chronology of the Solar System. In: Trümper, J.E. (Ed.), Landolt-Börnstein - Group VI Astronomy and Astrophysics Numerical Data and Functional Relationships in Science and Technology Volume 4B: Solar System, 4.5.
44. Trieloff M., Jessberger E.K., Herrwerth I., Hopp J., Fiéni C., Ghélis M., Bourot-Denise M., Pellas P. Structure and thermal history of the H-chondrite parent asteroid revealed by thermochronometry. Nature 2003, 422:502-506.
45. van Antwerpen W., du Toit C., Rousseau P. A review of correlations to model the packing structure and effective thermal conductivity in packed beds of mono-sized spherical particles. Nucl. Eng. Des. 2010, 240:1803-1818.
46. Weidenschilling S.J. The distribution of mass in the planetary system and solar nebula. Astrophys. Space Sci. 1977, 51:153-158.
47. Wurm, G., Haack, H., 2009. Levitation of dust at the surface of protoplanetary disks. In: Henning, T., Grün, E., Steinacker, J. (Eds.), Astronomical Society of the Pacific Conference Series, pp. 509-519.
48. Zsom A., Ormel C.W., Güttler C., Blum J., Dullemond C.P. The outcome of protoplanetary dust growth: Pebbles, boulders, or planetesimals? II: Introducing the bouncing barrier. Astron. Astrophys. 2010, 513:A57.