Keywords: سحابی خورشیدی; Cosmochemistry; Mineralogy; Phosphorus; Solar Nebula;
مقالات ISI سحابی خورشیدی (ترجمه نشده)
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Keywords: سحابی خورشیدی; nucleosynthetic isotope anomalies; molybdenum; solar nebula; iron meteorites; solar system;
Keywords: سحابی خورشیدی; condensation; Ca-, Al-rich inclusions; Ca and Ti isotope fractionation; solar nebula; protoplanetary disk; 50Ti isotopic anomalies;
Keywords: سحابی خورشیدی; Hibonite; Calcium hexaluminate; CA6; CAI; Oxybarometry; Solar nebula; Crystal chemistry; Oxygen fugacity; XANES; FDMNES;
Keywords: سحابی خورشیدی; Refractory Metal Nuggets; Solar Nebula; Solar System; Origin; Meteorites; Carbonaceous chondrites;
Keywords: سحابی خورشیدی; Oxygen isotopes; Achondrites; Laser fluorination; Chondrites; Early Solar System processes; Solar nebula; Mass independent variation;
Keywords: سحابی خورشیدی; Solar Nebula; Cosmochemistry; Origin, Solar System; Planetesimals;
Keywords: سحابی خورشیدی; carbonaceous chondrites; chondrule rims; Solar Nebula; NanoSIMS; circumstellar matter;
Keywords: سحابی خورشیدی; Spinel-hibonite inclusions (SHIBs); CAI; Meteorites; Solar nebula; Oxygen isotopes; Internal isochrons; Aluminum-26; Magnesium isotopes; Titanium isotopes; Calcium isotopes
Keywords: سحابی خورشیدی; Comets, origin; Comets, coma; Origin; Solar System; Solar Nebula;
Keywords: سحابی خورشیدی; Asteroids; Disks; Planetary formation; Solar Nebula;
Keywords: سحابی خورشیدی; chondrules; solar nebula; cosmogenic noble gases; pre-irradiation; galactic cosmic rays; solar cosmic rays
Keywords: سحابی خورشیدی; Disks; Meteorites; Radiative transfer; Solar nebula; Thermal histories;
Keywords: سحابی خورشیدی; Solar nebula; Astrochemistry: water formation; Collapsing cloud core; Solution of MHD equation;
Keywords: سحابی خورشیدی; Collisional physics; Meteorites; Planetesimals; Solar Nebula; Thermal histories
Evidence for accretion of fine-grained rims in a turbulent nebula for CM Murchison
Keywords: سحابی خورشیدی; X-ray CT; chondrules; fine-grained rims; accretionary rims; solar nebula; nebular turbulence;
Crystal growth and disequilibrium distribution of oxygen isotopes in an igneous Ca-Al-rich inclusion from the Allende carbonaceous chondrite
Keywords: سحابی خورشیدی; Oxygen isotopes; Ca-Al-rich inclusions; Solar nebula; Al-Mg systematics; SIMS;
High abundances of presolar grains and 15N-rich organic matter in CO3.0 chondrite Dominion Range 08006
Keywords: سحابی خورشیدی; Carbonaceous chondrites; Early solar system history; NanoSIMS; Nebular processes; Organic matter; Isotopic anomalies; Presolar grains Stardust; Solar Nebula;
A multielement isotopic study of refractory FUN and F CAIs: Mass-dependent and mass-independent isotope effects
Keywords: سحابی خورشیدی; Fractionated and unidentified nuclear (FUN); CAI; Hibonite; Meteorites; Solar nebula; Oxygen isotopes; Aluminum-26; Magnesium isotopes; Titanium isotopes; Calcium isotopes; Mass-dependent fractionation;
Presolar silicates in the matrix and fine-grained rims around chondrules in primitive CO3.0 chondrites: Evidence for pre-accretionary aqueous alteration of the rims in the solar nebula
Keywords: سحابی خورشیدی; Carbonaceous chondrites; Circumstellar grains; Early solar system history; Fine-grained chondrule rims; NanoSIMS; Nebular processes; Pre-accretionary alteration; Presolar grains; Stardust; Solar Nebula;
An experimental study of chondrule formation from chondritic precursors via evaporation and condensation in Knudsen cell: Shock heating model of dust aggregates
Keywords: سحابی خورشیدی; chondrule; condensation and evaporation; chondrite; Knudsen cell; solar nebula; shock wave heating;
Corundum-hibonite inclusions and the environments of high temperature processing in the early Solar System
Keywords: سحابی خورشیدی; Corundum; Hibonite; CAI; Chondrite; Oxygen isotopes; 26Al; Magnesium isotopes; Solar nebula; Condensation;
A long duration of the 16O-rich reservoir in the solar nebula, as recorded in fine-grained refractory inclusions from the least metamorphosed carbonaceous chondrites
Keywords: سحابی خورشیدی; Oxygen isotope; Al-Mg systematics; Refractory inclusion; Solar nebula; SIMS; Acfer 094;
The nature, origin and modification of insoluble organic matter in chondrites, the major source of Earth's C and N
Keywords: سحابی خورشیدی; Meteorites; Chondrites; Comets; Interplanetary dust; Organic matter; Interstellar; Solar nebula; Protoplanetary disk;
Crystallography of refractory metal nuggets in carbonaceous chondrites: A transmission Kikuchi diffraction approach
Keywords: سحابی خورشیدی; Refractory metal nuggets; Solar nebula; Solar System; Origin; Meteorites; Carbonaceous chondrites; Crystallography; Crystallisation; Transmission Kikuchi diffraction;
The ungrouped chondrite El Médano 301 and its comparison with other reduced ordinary chondrites
Keywords: سحابی خورشیدی; Ordinary chondrite; Enstatite chondrite; Reduced chondrite; Solar nebula; Reduction;
A new mechanism for chondrule formation: Radiative heating by hot planetesimals
Keywords: سحابی خورشیدی; Cosmochemistry; Meteorites; Solar Nebula;
Dust photophoretic transport around a T Tauri star: Implications for comets composition
Keywords: سحابی خورشیدی; Comets, composition; Comets, dust; Comets, origin; Solar Nebula;
Microstructural constraints on complex thermal histories of refractory CAI-like objects in an amoeboid olivine aggregate from the ALHA77307 CO3.0 chondrite
Keywords: سحابی خورشیدی; Amoeboid olivine aggregates (AOAs); Refractory phases; TiO2 nanoparticles; Condensation; Solar nebula; Transport;
A link between oxygen, calcium and titanium isotopes in 26Al-poor hibonite-rich CAIs from Murchison and implications for the heterogeneity of dust reservoirs in the solar nebula
Keywords: سحابی خورشیدی; Platy hibonite crystals (PLACs); CAI; Meteorites; Solar nebula; Oxygen isotopes; Titanium isotopes; Calcium isotopes; Aluminum-26;
Semarkona: Lessons for chondrule and chondrite formation
Keywords: سحابی خورشیدی; Asteroids; Asteroids, composition; Disks; Planetary formation; Solar Nebula;
Formation of analogs of cometary nitrogen-rich refractory organics from thermal degradation of tholin and HCN polymer
Keywords: سحابی خورشیدی; Cosmochemistry; Organic chemistry; Solar Nebula; Comets; Interplanetary dust;
Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation
Keywords: سحابی خورشیدی; Mo isotopes; meteorites; solar nebula; core formation; Moon; Mars;
The quasi-universality of chondrule size as a constraint for chondrule formation models
Keywords: سحابی خورشیدی; Meteorites; Solar nebula; Cosmochemistry; Disk; Accretion;
Water formation in early solar nebula: I. Quasi-stationary cloud core
Keywords: سحابی خورشیدی; Solar nebula; Hydrostatic gas sphere; Interstellar dust; Astrochemistry: water formation;
The 15N-enrichment in dark clouds and Solar System objects
Keywords: سحابی خورشیدی; Cosmochemistry; Solar nebula; Meteorites; Origin, Solar System; Radio observations;
The D/H ratio of water in the solar nebula during its formation and evolution
Keywords: سحابی خورشیدی; Cosmochemistry; Comets, Composition; Origin, Solar System; Solar nebula;
p-Process 180W anomalies in iron meteorites: Nucleosynthetic versus non-nucleosynthetic origins
Keywords: سحابی خورشیدی; p-process; 180W; solar nebula; protoplanetary disk; nucleosynthetic anomalies; iron meteorites;
Water transport in protoplanetary disks and the hydrogen isotopic composition of chondrites
Keywords: سحابی خورشیدی; Meteorites; Solar nebula; Cosmochemistry; Disks; Comets
Free collisions in a microgravity many-particle experiment - II: The collision dynamics of dust-coated chondrules
Keywords: سحابی خورشیدی; Experimental techniques; Planetary formation; Solar nebula; Planetesimals; Meteorites;
Formation of chondrules in magnetic winds blowing through the proto-asteroid belt
Keywords: سحابی خورشیدی; chondrule formation; solar nebula; protostellar winds
LETTERSCosmochemical consequences of particle trajectories during FU Orionis outbursts by the early Sun
Keywords: سحابی خورشیدی; solar nebula; short-lived radioactivities; oxygen isotopes; refractory inclusions; chronometry; accretion disks;
Origin of isotopic heterogeneity in the solar nebula by thermal processing and mixing of nebular dust
Keywords: سحابی خورشیدی; Mo isotopes; W isotopes; nucleosynthesis; meteorites; solar nebula
First-principles investigation of equilibrium isotopic fractionation of O- and Si-isotopes between refractory solids and gases in the solar nebula
Keywords: سحابی خورشیدی; isotopic fractionation; ab initio calculations; solar nebula;
On the aerodynamic redistribution of chondrite components in protoplanetary disks
Keywords: سحابی خورشیدی; Meteorites; Solar nebula; Cosmochemistry; Disks;
Refractory Metal Nuggets - Formation of the first condensates in the Solar Nebula
Keywords: سحابی خورشیدی; Accretion; Solar Nebula; Origin, Solar System; Meteorites; Magnetic fields;
UV photolysis, organic molecules in young disks, and the origin of meteoritic amino acids
Keywords: سحابی خورشیدی; Organic chemistry; Origin, Solar System; Solar nebula; Meteorites
The thermal structure and the location of the snow line in the protosolar nebula: Axisymmetric models with full 3-D radiative transfer
Keywords: سحابی خورشیدی; Accretion; Solar nebula; Radiative transfer; Planetary formation;
Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth
Keywords: سحابی خورشیدی; Mo isotopes; nucleosynthesis; meteorites; solar nebula; Earth composition
Origin of the differences in refractory-lithophile-element abundances among chondrite groups
Keywords: سحابی خورشیدی; Meteorites; Solar nebula; Cosmochemistry; Disks