
Extreme‐pressure research explores how Earth's mantle solidified
Author(s) -
Schultz Colin
Publication year - 2013
Publication title -
eos, transactions american geophysical union
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.316
H-Index - 86
eISSN - 2324-9250
pISSN - 0096-3941
DOI - 10.1002/2013eo030027
Subject(s) - mantle (geology) , geology , core–mantle boundary , post perovskite , mantle wedge , transition zone , geophysics , mantle convection , planetary differentiation , hotspot (geology) , structure of the earth , geochemistry , earth science , subduction , seismology , tectonics
During the earliest stages of the Earth's formation, the planet's mantle may have taken the form of a giant magma ocean, being fully or partially molten all the way down to the core‐mantle boundary. Though mantle material is predominantly solid today, some scientists suggest that regions of anomalously low seismic wave velocity deep within the mantle, known as ultralow velocity zones (ULVZs), may be indicative of a remnant magma ocean or of partial melting of minerals near the core‐mantle boundary. To understand how the early mantle solidified or whether modern melt could be the source of ULVZs, scientists need to know how various minerals and melts behave under the extreme conditions found near the center of the Earth.