Identification of isotopically primitive interplanetary dust particles: A NanoSIMS isotopic imaging study

By C. Floss, F. Stadermann, J. P. Bradley, R. Z, Dai, S. Bajt, G. Graham, A. S. Lea. 2006

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NanoSIMS: Technical Aspects and Applications in Cosmochemistry and Biological Geochemistry (2013, unknown): “Highest abundances are usually observed in primitive IDPs, which have average presolar silicate concentrations of ~ 400 lg g (Floss et al. 2006) and up to the weight per cent level in individual particles (Busemann et al.”
Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection (2009, background): “The bulk δ13C values between −9 and −51‰ are in the typical range observed previously in IDPs (Messenger et al., 2003b; Floss et al., 2006).”
Characterization of Presolar Silicate and Oxide Grains in Primitive Carbonaceous Chondrites (2007, background): “Floss et al. (2006) report a presolar silicate abundance of 375 ppm in isotopically primitive IDPs.”
Aluminum-, Calcium- and Titanium-rich Oxide Stardust in Ordinary Chondrite Meteorites (2008, background): “…of manymore presolar spinel grains (Zinner et al. 2003) and, more significantly, the discovery and characterization of presolar silicate minerals (Floss et al. 2006; Messenger et al. 2003; Mostefaoui & Hoppe 2004; Nagashima et al. 2004; Nguyen et al. 2007; Nguyen& Zinner 2004; Vollmer et al.…”