High-Pressure Mineral Database

Since September 13, 2011 

by Naotaka TOMIOKA@JAMSTEC & Masaaki MIYAHARA@Hiroshima Univ.

A variety of dense polymorphs of elements, oxides and silicates have been found by laboratory high-pressure experiments. In nature, shocked meteorites are the most important sources of high-pressure minerals in addition to impact crater rocks, inclusions in diamond, mantle xenoliths, and ultrahigh-pressure metamorphic (UHP) rocks. It is not easy to fully characterize such high-pressure minerals because of their very small grain size and low abundance. However, state-of-art techniques such as electron microscopy, synchrotron X-ray diffractometry, and micro-Raman spectroscopy enable the identification of such small crystalline grains. As a result, many of natural high-pressure phases of silicates and oxides have been discovered since 1990's. Textural, crystallographic and chemical characteristics of meteoritic high-pressure minerals provide us not only the clues to understand the impact events of meteorite parent bodies, but also insights on the structure and dynamics of the deep Earth. This website provides a database of the high-pressure minerals in meteorites and also those in terrstrial rocks. 

General references on natural high-pressure minerals: 

Shocked meteorites

Impact craters

Inclusions in diamond

Ultrahigh-pressure metamorphic rocks

Schematic drawing of the formation mechanism of high-pressure minerals in shock-induced melt veins (shock veins) in meteorites. High-pressure minerals form by two types of formation mechanisms (1) solid-state high-pressure transformation of the host-rock minerals, and (2) crystallization of chondritic or monomineralic melt under high pressure in the matrix of shock veins. 

High-pressure minerals approved by IMA

Synthetic high-pressure minerals 

Acknowledgements 

This database was supported by JSPS KAKENHI Grant Numbers 15H03750, 23540558 and contributions from the following people: