TY - JOUR
T1 - Two-step nucleation process of silicate interplanetary dust particles at the vicinity of silicate melt
AU - Kobatake, Hidekazu
AU - Tsukamoto, Katsuo
AU - Satoh, Hisao
PY - 2005/5/15
Y1 - 2005/5/15
N2 - The condensation processes of interplanetary dust particles (IDPs) around a high temperature silicate melt droplet were investigated in situ by a newly developed flash heating technique under microgravity using a drop tube facility. Two-step nucleation process was captured in the vicinity of the MgSiO 3 melt by a CCD camera. The first nucleation was observed at a distance of 7 mm from the vapor source at 0.3 s and the second nucleation was observed 1.4 s after the MgSiO3 melt evaporated. The first nucleated particles were irregularly shaped amorphous silica with a diameter of 100-500 nm. The amorphous enstatite particles with a diameter of 70 nm nucleated 1.1 s later. The observed condensation sequence was silica and then enstatite. The difference of these condensations sequence with the chemical equilibrium was showed through the present experiment. The present in situ observation under microgravity was found to be a very useful technique to judge the nucleation sequence of various phases in very short duration within 3.0 s.
AB - The condensation processes of interplanetary dust particles (IDPs) around a high temperature silicate melt droplet were investigated in situ by a newly developed flash heating technique under microgravity using a drop tube facility. Two-step nucleation process was captured in the vicinity of the MgSiO 3 melt by a CCD camera. The first nucleation was observed at a distance of 7 mm from the vapor source at 0.3 s and the second nucleation was observed 1.4 s after the MgSiO3 melt evaporated. The first nucleated particles were irregularly shaped amorphous silica with a diameter of 100-500 nm. The amorphous enstatite particles with a diameter of 70 nm nucleated 1.1 s later. The observed condensation sequence was silica and then enstatite. The difference of these condensations sequence with the chemical equilibrium was showed through the present experiment. The present in situ observation under microgravity was found to be a very useful technique to judge the nucleation sequence of various phases in very short duration within 3.0 s.
KW - A1. Chemical composition
KW - A1. Nucleation
KW - A2. Microgravity conditions
KW - B2. Interplanetary gas and dust
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U2 - 10.1016/j.jcrysgro.2005.01.105
DO - 10.1016/j.jcrysgro.2005.01.105
M3 - Article
AN - SCOPUS:17744375167
SN - 0022-0248
VL - 279
SP - 186
EP - 194
JO - Journal of Crystal Growth
JF - Journal of Crystal Growth
IS - 1-2
ER -