Title of article :
Micrometer-sized ice particles for planetary-science experiments – I. Preparation, critical rolling friction force, and specific surface energy
Author/Authors :
Gundlach، نويسنده , , B. and Kilias، نويسنده , , S. and Beitz، نويسنده , , E. and Blum، نويسنده , , J.، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2011
Abstract :
Coagulation models assume a higher sticking threshold for micrometer-sized ice particles than for micrometer-sized silicate particles. However, in contrast to silicates, laboratory investigations of the collision properties of micrometer-sized ice particles (in particular, of the most abundant H2O-ice) have not been conducted yet. Thus, we used two different experimental methods to produce micrometer-sized H2O-ice particles, i.e. by spraying H2O droplets into liquid nitrogen and by spraying H2O droplets into a cold nitrogen atmosphere. The mean particle radii of the ice particles produced with these experimental methods are (1.49 ± 0.79) μm and (1.45 ± 0.65) μm. Ice aggregates composed of the micrometer-sized ice particles are highly porous (volume filling factor: ϕ = 0.11 ± 0.01) or rather compact (volume filling factor: ϕ = 0.72 ± 0.04), depending on the method of production. Furthermore, the critical rolling friction force of FRoll,ice = (114.8 ± 23.8) × 10−10 N was measured for micrometer-sized ice particles, which exceeds the critical rolling friction force of micrometer-sized SiO2 particles ( F Roll , SiO 2 = ( 12.1 ± 3.6 ) × 10 - 10 N ) . This result implies that the adhesive bonding between micrometer-sized ice particles is stronger than the bonding strength between SiO2 particles. An estimation of the specific surface energy of micrometer-sized ice particles, derived from the measured critical rolling friction forces and the surface energy of micrometer-sized SiO2 particles, results in γice = 0.190 J m−2.
Keywords :
comets , origin , Nucleus , ICES , mechanical properties , Interplanetary dust , solar system