Sekiya, M. (1998) Quasi-equilibrium density distributions of small dust aggregations in the solar nebula, Icarus, 133, 293-309.
Kokubo, E. and Ida, S. (2000) Formation of Protoplanets from Planetesimals in the Solar Nebula, Icarus, 143, 15-27.
Krot, A.N et al. (2009)Origin and chronology of chondritic components: A review, Geochimica et Cosmochimica Acta, 73(17), 4963-4997.
Young E. D. (2001) The hydrology of carbonaceous chondrite parent bodies and the evolution of planet progenitors. Phil. Trans. R. Soc. Lond. A 359, 2095?2110.
Clayton R. N. and Mayeda T. K. (1984) The oxygen isotope record in Murchison and other carbonaceous chondrites. Earth. Planet. Sci. Lett. 67, 151?161.
Guo W. and Eiler J. M. (2007) Temperatures of aqueous alteration and evidence for methane generation on the parent bodies of the CM chondrites. Geochim.Cosmochim. Acta 71, 5565?5575.
Benedix G. K., Leshin L. A., Farquhar J., Jackson T. and Thiemens M. H. (2003) Carbonates in CM2 chondrites: constraints on alteration conditions from oxygen isotopic compositions and petrographic observations. Geochim. Cosmochim. Acta 67, 1577?1588.
地球惑星物理学科四年生を対象とした演習では次の文献を読んでいます。
McKeegan, K.D. and Davis, A.M. (2003) Early Solar System Chronology, session 1.16, p.1-38, in Treatise on Geochemistry (edited by Turekian, K.K. and Holland, H.D.), Elsevier.
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