HUSCAP logo Hokkaido Univ. logo

Hokkaido University Collection of Scholarly and Academic Papers >
Graduate School of Science / Faculty of Science >
Peer-reviewed Journal Articles, etc >

Survivability of presolar oxygen isotopic signature of amorphous silicate dust in the protosolar disk

This item is licensed under: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International

Files in This Item:

The file(s) associated with this item can be obtained from the following URL:https://doi.org/10.1111/maps.13365


Title: Survivability of presolar oxygen isotopic signature of amorphous silicate dust in the protosolar disk
Authors: Yamamoto, Daiki Browse this author
Tachibana, Shogo Browse this author
Kawasaki, Noriyuki Browse this author
Yurimoto, Hisayoshi Browse this author →KAKEN DB
Issue Date: 12-Aug-2019
Publisher: John Wiley & Sons
Journal Title: Meteoritics & Planetary Science
Publisher DOI: 10.1111/maps.13365
Abstract: Oxygen isotope exchange experiments between tens of nanometer-sized amorphous enstatite grains and water vapor were carried out under a condition of protoplanetary disk-like low water vapor pressure in order to investigate the survivability of distinct oxygen isotope signatures of presolar silicate grains in the protosolar disk. Oxygen isotope exchange between amorphous enstatite and water vapor proceeded at 923-1003 K and 0.3 Pa of water vapor through diffusive isotope exchange in the amorphous structure. The rate of diffusive isotope exchange is given by D (m(2) s(-1)) = (5.0 +/- 0.2) x 10(-21) exp[-161.3 +/- 1.7 (kJ mol(-1)) R-1 (1/T-1/1200)]. The activation energy for the diffusive isotope exchange for amorphous enstatite is the same as that for amorphous forsterite within the analytical uncertainties, but the isotope exchange rate is similar to 30 times slower in amorphous enstatite because of the difference in frequency factor of the reaction. The reaction kinetics indicates that 0.1-1 mu m-sized presolar amorphous silicate dust with enstatite and forsterite compositions would avoid oxygen isotope exchange with protosolar disk water vapor only if they were kept at temperatures below similar to 500-650 K within the lifetime of the disk gas.
Rights: https://creativecommons.org/licenses/by-nc-nd/4.0/
Type: article
URI: http://hdl.handle.net/2115/75759
Appears in Collections:理学院・理学研究院 (Graduate School of Science / Faculty of Science) > 雑誌発表論文等 (Peer-reviewed Journal Articles, etc)

Export metadata:

OAI-PMH ( junii2 , jpcoar )

MathJax is now OFF:


 

 - Hokkaido University