日本地球惑星科学連合2015年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT03] Structure and dynamics of Earth and Planetary deep interiors

2015年5月25日(月) 14:15 〜 16:00 106 (1F)

コンビーナ:*芳野 極(岡山大学地球物質科学研究センター)、田中 聡(海洋研究開発機構 地球深部ダイナミクス研究分野)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、John Hernlund(Earth-Life Science Institute, Tokyo Institute of Technology)、座長:趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、Konstantin Litasov(V.S. Sobolev Institute of Geology and Mineralogy SB RAS)

14:45 〜 15:00

[SIT03-03] Defect chemistry and diffusion in hydrous forsterite

*Hongzhan FEI1Tomoo KATSURA2 (1.Institute for Study of the Earth Interior, Okayama University, Misasa, Tottori, 682-0193, Japan、2.Bayerisches Geoinstitut, University of Bayreuth, 95447, Bayreuth, Germany)

キーワード:defect chemistry, self-diffusion coefficient, silicon, oxygen, water content, forsterite

The mass transport of olivine, which reflects the flow in the Earth's upper mantle, is controlled by the diffusion of structural elements. On the other hand, the diffusivity of an ion in the crystal is dominated by the motion of point defects of the corresponding sites. It is thus necessary to know the diffusivities of elements in olivine in the view of defect chemistry so as to investigate the behaviors in the upper mantle conditions.
Fei et al. (2013, 2014) systematically measured silicon and oxygen self-diffusion coefficients (DSi and DO, respectively) in iron-free forsterite as functions of water contents, showing that DSiCH2O0.32(7), DOCH2O0.05(6). These water-content exponents are much smaller than that expected on the basis of the assumption that self-diffusion coefficient of a chemical species is simply proportional to its defect density. Therefore, a new defect chemistry model is required to explain the above relationships.
Silicon diffusion:
The DSi should be proportional to the density of silicon defects, namely, DSi[VSi'''']. On the other hand, Si4+ is tightly surrounded by four-coordinated O2-, and therefore, migration of Si4+ should be enhanced if a surrounding O2- is missing. We can expect that a certain proportion of VSi'''' is associated with VO•• due to their excess charges with the opposite signs. As a result, Si migration is probably dominated by VO••-associated VSi''''. DSi is thus also proportional to [VO••] and we have,
DSi [VSi''''] × [VO••].
Under the charge neutrality condition of [(OH)O•] = 2[VMg''] in hydrous forsterite, we have [VSi''''] (fH2O)2/3 and [VO••] (fH2O)-1/3. Therefore,
DSi [VSi''''] ×[VO••] (fH2O)1/3,
which agrees well with the experimental results: DSi (CH2O)0.32(7) (Fei et al., 2013).
Oxygen diffusion:
In hydrous olivine/forsterite, hydrogen exists as hydroxyl, (OH)-. Oxygen ions could diffuse either by hopping of O2- without H+ or by hopping of O in (OH)-. Because H+-associated O has a lower Coulomb force due to the excess charge by H+, the hopping probability of (OH)- should be higher than that of O2-. Thus, the O diffusion should be dominated by O2- of (OH)-. As a result, we have,
DO [VO] × ([O2-]hopping + [(OH)-]hopping) ≈ [VO••] × [(OH)-]hopping.
There are mainly three types of (OH)- in hydrous olivine/forsterite: (a) (OH)O• associated with VMg''; (b) (OH)O• associated with VSi''''; (c) (OH)O• un-associated with any cation vacancies. The un-associated (OH)O• should have much higher mobility than VSi'''' or VMg'' associated ones due to the Coulomb force and therefore the O diffusion is probably dominated by un-associated (OH)O•. Thus,
DO [VO••] × [(OH)-]hopping ≈ [VO••] × [(OH)O•]un-associated.
Under the charge neutrality condition of [(OH)O•] = 2[VMg''], we have [VO••] (fH2O)-1/3 and [(OH)O•]un-associated (fH2O)1/3. Therefore,
DO [VO••] × [(OH)O•]un-associated (fH2O)0.
This model suggests that DO is independent from CH2O, which agrees well with the experimental results, DO CH2O0.05(6) (Fei et al., 2014).

Fei et al. (2013), Nature 498, 213-215.
Fei et al. (2014), JGR 119, 7598-7606.