Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Highly siderophile elements in Earth, Mars, the Moon, and asteroids
The highly siderophile elements (HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au) are key tracers of
planetary accretion and differentiation processes due to their affinity for metal relative to …
planetary accretion and differentiation processes due to their affinity for metal relative to …
Meteoritic minerals and their origins
About 435 mineral species have been identified in meteorites including native elements,
metals and metallic alloys, carbides, nitrides and oxynitrides, phosphides, silicides, sulfides …
metals and metallic alloys, carbides, nitrides and oxynitrides, phosphides, silicides, sulfides …
Copper systematics in arc magmas and implications for crust-mantle differentiation
Arc magmas are important building blocks of the continental crust. Because many arc lavas
are oxidized, continent formation is thought to be associated with oxidizing conditions. On …
are oxidized, continent formation is thought to be associated with oxidizing conditions. On …
Systematics and evaluation of meteorite classification
Classification of meteorites is largely based on their mineralogical and petrographic
characteristics and their whole-rock chemical and O-isotopic compositions. According to the …
characteristics and their whole-rock chemical and O-isotopic compositions. According to the …
Origin and age of the earliest Martian crust from meteorite NWA 7533
The ancient cratered terrain of the southern highlands of Mars is thought to hold clues to the
planet's early differentiation,, but until now no meteoritic regolith breccias have been …
planet's early differentiation,, but until now no meteoritic regolith breccias have been …
Young chondrules in CB chondrites from a giant impact in the early Solar System
Chondrules, which are the major constituent of chondritic meteorites, are believed to have
formed during brief, localized, repetitive melting of dust (probably caused by shock waves,) …
formed during brief, localized, repetitive melting of dust (probably caused by shock waves,) …
Enrichment of moderately volatile elements in first-generation planetesimals of the inner Solar System
The depletion of moderately volatile elements (MVEs) in terrestrial planets remains poorly
understood, with explanations including partial nebular condensation and MVE loss during …
understood, with explanations including partial nebular condensation and MVE loss during …
Early core formation in asteroids and late accretion of chondrite parent bodies: Evidence from 182Hf-182W in CAIs, metal-rich chondrites, and iron meteorites
The 182Hf-182W isotopic systematics of Ca-Al-rich inclusions (CAIs), metal-rich chondrites,
and iron meteorites were investigated to constrain the relative timing of accretion of their …
and iron meteorites were investigated to constrain the relative timing of accretion of their …
Partitioning of Ru, Rh, Pd, Re, Ir, and Au between Cr-bearing spinel, olivine, pyroxene and silicate melts
A series of high temperature experiments was undertaken to study partitioning of several
highly siderophile elements (HSE; Ru, Rh, Pd, Re, Os, Ir, Pt and Au) between Cr-rich spinel …
highly siderophile elements (HSE; Ru, Rh, Pd, Re, Os, Ir, Pt and Au) between Cr-rich spinel …
Abundance, distribution, and origin of 60Fe in the solar protoplanetary disk
Meteorites contain relict decay products of short-lived radionuclides that were present in the
protoplanetary disk when asteroids and planets formed. Several studies reported a high …
protoplanetary disk when asteroids and planets formed. Several studies reported a high …