Presolar silicate grains: Abundances, isotopic and elemental compositions, and the effects of secondary processing
C Floss, P Haenecour - Geochemical Journal, 2016 - jstage.jst.go.jp
Close to a thousand presolar silicate grains have been identified since their initial discovery
in interplanetary dust particles (IDPs) just over ten years ago. Studies have shown that …
in interplanetary dust particles (IDPs) just over ten years ago. Studies have shown that …
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 …
To investigate the origin of fine-grained rims around chondrules (FGRs), we compared
presolar grain abundances, elemental compositions and mineralogies in fine-grained …
presolar grain abundances, elemental compositions and mineralogies in fine-grained …
Stardust investigation into the CR chondrite Grove Mountain 021710
We report the presolar grain inventory of the CR chondrite Grove Mountain 021710. A total
of 35 C-anomalous grains (∼ 236 ppm) and 112 O-anomalous grains (∼ 189 ppm) were …
of 35 C-anomalous grains (∼ 236 ppm) and 112 O-anomalous grains (∼ 189 ppm) were …
First laboratory observation of silica grains from core collapse supernovae
We report the discovery of two supernova silica (SiO 2) grains in the primitive carbonaceous
chondrites LaPaZ 031117 and Grove Mountains 021710. Only five presolar silica grains …
chondrites LaPaZ 031117 and Grove Mountains 021710. Only five presolar silica grains …
[PDF][PDF] Supernova Grains Identified in the Lab
EBYM CRUZ, S VIGNIERI - Ibis, 2013 - researchgate.net
Presolar grains are tiny mineral and/or amorphous grains (from a few nanometers to several
micrometers in diameter) that formed in stellar outflows or supernova ejecta, survived the …
micrometers in diameter) that formed in stellar outflows or supernova ejecta, survived the …