Javascript must be enabled to continue!
Magnetite‐sulfide chondrules and nodules in CK carbonaceous chondrites: Implications for the timing of CK oxidation
View through CrossRef
Abstract— CK carbonaceous chondrites contain rare (∼0.1 vol%) magnetite‐sulfide chondrules. These objects range from ∼240 to 500 μm in apparent diameter and have ellipsoidal to spheroidal morphologies, granular textures and concentric layering. They are very similar in size, shape, texture, mineralogy and mineral composition to the magnetite‐sulfide nodules which occur inside mafic silicate chondrules in CK chondrites. It seems likely that the magnetite‐sulfide chondrules constitute the subset of magnetite‐sulfide nodules that escaped as immiscible droplets from their molten silicate chondrule hosts during chondrule formation. The intactness of the magnetite‐sulfide chondrules and nodules implies that oxidation of CK metal occurred before agglomeration; otherwise, the factor of two increase in molar volume associated with the conversion of metallic Fe‐Ni into magnetite would have disrupted the objects and destroyed their concentrically layered textures. Hence, the pervasive silicate darkening of CK chondrites documented previously was caused by the shock mobilization of magnetite and sulfide, not metallic Fe‐Ni and sulfide as in shock‐darkened ordinary chondrites.
Title: Magnetite‐sulfide chondrules and nodules in CK carbonaceous chondrites: Implications for the timing of CK oxidation
Description:
Abstract— CK carbonaceous chondrites contain rare (∼0.
1 vol%) magnetite‐sulfide chondrules.
These objects range from ∼240 to 500 μm in apparent diameter and have ellipsoidal to spheroidal morphologies, granular textures and concentric layering.
They are very similar in size, shape, texture, mineralogy and mineral composition to the magnetite‐sulfide nodules which occur inside mafic silicate chondrules in CK chondrites.
It seems likely that the magnetite‐sulfide chondrules constitute the subset of magnetite‐sulfide nodules that escaped as immiscible droplets from their molten silicate chondrule hosts during chondrule formation.
The intactness of the magnetite‐sulfide chondrules and nodules implies that oxidation of CK metal occurred before agglomeration; otherwise, the factor of two increase in molar volume associated with the conversion of metallic Fe‐Ni into magnetite would have disrupted the objects and destroyed their concentrically layered textures.
Hence, the pervasive silicate darkening of CK chondrites documented previously was caused by the shock mobilization of magnetite and sulfide, not metallic Fe‐Ni and sulfide as in shock‐darkened ordinary chondrites.
Related Results
Clinicopathological Features of Indeterminate Thyroid Nodules: A Single-center Cross-sectional Study
Clinicopathological Features of Indeterminate Thyroid Nodules: A Single-center Cross-sectional Study
Abstract
Introduction
Due to indeterminate cytology, Bethesda III is the most controversial category within the Bethesda System for Reporting Thyroid Cytopathology. This study exam...
Chondrule Formation by the Jovian Sweeping Secular Resonance
Chondrule Formation by the Jovian Sweeping Secular Resonance
Chondritic meteorites, or chondrites, contain some of the oldest and most primitive solids in our solar system. They record the physical conditions at the early phase of the solar ...
Infrared diffuse reflectance spectra of carbonaceous chondrites: Amount of hydrous minerals
Infrared diffuse reflectance spectra of carbonaceous chondrites: Amount of hydrous minerals
Abstract— Infrared diffuse reflectance spectra (2.53–25 μm) of some carbonaceous (C) chondrites were measured. The integrated intensity of the absorption bands near 3 μm caused by ...
Constraints on the ice composition of carbonaceous chondrites from their magnetic mineralogy
Constraints on the ice composition of carbonaceous chondrites from their magnetic mineralogy
Carbonaceous chondrites experienced varying degrees of aqueous alteration on their parent asteroids, which influenced their mineralogies, textures, and bulk chemical and isotopic c...
Chondrules: The canonical and noncanonical views
Chondrules: The canonical and noncanonical views
AbstractMillimeter‐scale rock particles called chondrules are the principal components of the most common meteorites, chondrites. Hence, chondrules were arguably the most abundant ...
Giant Magnetocapacitance in Magnetic Polypyrrole/Magnetite Nanocomposites under Low Magnetic Field
Giant Magnetocapacitance in Magnetic Polypyrrole/Magnetite Nanocomposites under Low Magnetic Field
Electrochemical capacitors have attracted significant attention for their promising potential applications ranging from portable electronic devices to hybrid electrical vehicles an...
Authigenesis at the Urals Massive Sulfide Deposits: Insight from Pyrite Nodules Hosted in Ore Diagenites
Authigenesis at the Urals Massive Sulfide Deposits: Insight from Pyrite Nodules Hosted in Ore Diagenites
The pyrite nodules from ore diagenites of the Urals massive sulfide deposits associated with various background sedimentary rocks are studied using optical and electron microscopy ...
Chromites in Ordinary chondrite fusion crusts
Chromites in Ordinary chondrite fusion crusts
We studied 5 fall Ordinary Chondrites of different groups (H4, H5, LL5, LL6, L3.6) and an Antarctic meteorite (H5), in order to investigate possible compositional differences betwe...

