Search results for "Parent body"

showing 3 items of 3 documents

PIANCALDOLI METEORITE: CHEMISTRY, MINERALOGY AND PETROLOGY

1976

The fall occurred near Piancaldoli, Florence, Italy, at 19.14 U.T. on the 10th August 1968. The fireball broke up in the atmosphere producing a cloud like a balloon. The trajectory and the terminal point were calculated, leading to the recovery of three small meteoritic fragments, found on the roof of a house. Chemical analysis gave the following results: SiO2 40.80; TiO2 0.15; Al2O3 2. 70; Cr2O3 0.47; FeO 17.20; MnO 0.07; MgO 25.18; CaO 1.95; Na2O 0.64; K2O 0.07; P2O5 0.20; NiS 0.93; FeS 6.24; Fe° 2.40; Ni° 0.40; Co 0.05; sum 99.45. In the lithic portion of the meteorite the following minerals were found: both clino and orthopyroxenes (En = 76 to 98%), olivines (Fo = 66 to 98%), troilite, …

GeochemistryMineralogyengineering.materialTroiliteParent bodyKamaciteSchreibersiteMeteoriteChondriteengineeringGeneral Earth and Planetary SciencesPyrrhotiteGeologyGeneral Environmental ScienceOrdinary chondriteMeteoritics
researchProduct

Cosmic-ray exposure ages of pallasites

2015

We analyzed cosmogenic nuclides in metal and/or silicate (primarily olivine) separated from the main-group pallasites Admire, Ahumada, Albin, Brahin, Brenham, Esquel, Finmarken, Glorieta Mountain, Huckitta, Imilac, Krasnojarsk, Marjalahti, Molong, Seymchan, South Bend, Springwater, and Thiel Mountains and from Eagle Station. The metal separates contained an olivine fraction which although small, <1 wt% in most cases, nonetheless contributes significantly to the budgets of some nuclides (e.g., up to 35% for Ne-21 and Al-26). A correction for olivine is therefore essential and was made using model calculations and/or empirical relations for the production rates of cosmogenic nuclides in iron …

RadionuclideOlivineMeteoroidGeochemistryMineralogyengineering.materialSilicateParent bodychemistry.chemical_compoundGeophysicschemistryMeteoriteSpace and Planetary ScienceengineeringNuclideCosmogenic nuclideGeologyMeteoritics &amp; Planetary Science
researchProduct

Origin of SiO2-rich components in ordinary chondrites

2006

Abstract Silica-rich objects are common minor components in ordinary chondrites (OC), occurring as fragments and as chondrules. Their typical paragenesis is orthopyroxene + SiO 2 (with bulk SiO 2 >65 wt%) and occasionally with additional olivine and/or spinel. Individual silica-rich components (SRC) have previously been studied in various types of OCs, although there is only one comprehensive study of these objects by Brigham et al. [Brigham, C.A., Murrell, M.T., Yabuki, H., Ouyang, Z., El Goresy, A., 1986. Silica-bearing chondrules and clasts in ordinary chondrites. Geochim. Cosmochim. Acta 50, 1655–1666]. Several different explanations of how SRCs formed have been published. The main ques…

TridymiteOlivineGeochemistry and PetrologyChondriteengineeringMineralogyChondrulePyroxeneengineering.materialFormation and evolution of the Solar SystemCristobaliteGeologyParent bodyGeochimica et Cosmochimica Acta
researchProduct