Carbonaceous components in the comet Halley dust
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2020, IcarusCitation Excerpt :The IOM consists of a kerogen-like polymer that contains a majority of organic matter in carbonaceous chondrites. The composition of chondritic IOM is not much different from that of non-volatile cometary organic matter (Kissel and Krueger, 1987; Jessberger et al., 1988; Fomenkova et al., 1994; Levasseur-Regourd et al., 2018) that may have a common origin (Alexander, 2011; Alexander et al., 2017). The difference between IOM and analogous cometary organic matter reflects aromatization and decreasing of H/C, N/C and O/C ratios through alteration on parent bodies of chondrites.
Evidence for Ubiquitous Carbon Grain Destruction in Hot Protostellar Envelopes
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