Organic thermometry for chondritic parent bodies

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Ultrastructural and chemical study of modern and fossil sporoderms by Scanning Transmission X-ray Microscopy (STXM) (2009, unknown): “Alternatively, embedding the samples in elemental sulphurmay provide an alternative solution as it does not affectNEXAFS spectroscopyat the CK edge; however, the procedure is not straightforward to perform (Hugo and Cady, 2004; Lehmann et al., 2005; Cody et al., 2008).”
Chondrites as samples of differentiated planetesimals (2009, background): “The presence 23 of talc and the absence of serpentine indicate peak temperatures of ~300-350°C (Brearley 1 1997, Krot et al. 1995), while organic thermometry and presolar gases in nanodiamonds 2 place an upper limit of <~600 °C (Cody et al. 2008).”
XANES, Raman and XRD study of anthracene-based cokes and saccharose-based chars submitted to high-temperature pyrolysis (2010, background): “[24] Cody G, Alexander C, Yabuta H, Kilcoyne A, Araki T, Ade H, et al.”
Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation (2010, background): “Furthermore, given that Murchison and Orgueil were likely never heated even to ∼150°C (Busemann et al. 2007; Cody et al. 2008) since formation, blocking-temperature relations for magnetite (Pullaiah et al. 1975) and kamacite (Garrick-Bethell and Weiss 2009) indicate that these minerals are unlikely…”