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Published April 2024 | Supplemental Material
Journal Article Open

Metasomatic alteration of coarse-grained igneous calcium-aluminum-rich inclusions from CK3 carbonaceous chondrites

  • 1. ROR icon University of Hawaii at Manoa
  • 2. ROR icon Colby College
  • 3. ROR icon Harvard University
  • 4. ROR icon California Institute of Technology
  • 5. ROR icon Senckenberg Nature Research Society

Abstract

We report on the primary and secondary mineralogies of three coarse‐grained igneous calcium‐aluminum‐rich inclusions (CAIs) (Compact Type A [CTA], Type B [B], and forsterite‐bearing type B [FoB]) from the Northwest Africa (NWA) 5343 (CK3.7) and NWA 4964 (CK3.8) carbonaceous chondrites, compare them with the mineralogy of igneous CAIs from the Allende (CV3.6) chondrite, and discuss the nature of the alteration processes that affected the CK and CV CAIs. The primary mineralogy and mineral chemistry of the CK3 CAIs studied are similar to those from Allende; however, primary melilite and anorthite are nearly completely absent. Although the secondary minerals identified in CK CAIs (Al‐diopside, andradite, Cl‐apatite, clintonite, forsterite, ferroan olivine, Fe,Ni‐sulfides, grossular, ilmenite, magnetite, plagioclase, spinel, titanite, and wadalite) occur also in the Allende CAIs, there are several important differences: (i) In addition to melilite and anorthite, which are nearly completely replaced by secondary minerals, the alteration of CK CAIs also affected high‐Ti pyroxenes (fassaite and grossmanite) characterized by high Ti3+/Ti4+ ratio and spinel. These pyroxenes are corroded and crosscut by veins of Fe‐ and Ti‐bearing grossular, Fe‐bearing Al,Ti‐diopside, titanite, and ilmenite. Spinel is corroded by Fe‐bearing Al‐diopside and grossular. (ii) The secondary mineral assemblages of grossular + monticellite and grossular + wollastonite, commonly observed in the Allende CAIs, are absent; the Fe‐bearing grossular + Fe‐bearing Al‐diopside ± Fe,Mg‐spinel, Fe‐bearing grossular + Fe,Mg‐olivine ± Fe,Mg‐spinel, and Ca,Na‐plagioclase + Fe‐bearing Al‐diopside + Fe‐bearing grossular assemblages are present instead. These mineral assemblages are often crosscut by veins of Fe‐bearing Al‐diopside, Fe,Mg‐olivine, Fe,Mg‐spinel, and Ca,Na‐plagioclase. The coarse‐grained secondary grossular and Al‐diopside often show multilayered chemical zoning with distinct compositional boundaries between the layers; the abundances of Fe and Ti typically increase toward the grain edges. (iv) Sodium‐rich secondary minerals, nepheline and sodalite, commonly observed in the peripheral portions of the Allende CAIs, are absent; Ca,Na‐plagioclase is present instead. We conclude that coarse‐grained igneous CAIs from CK3.7–3.8 s and Allende experienced an open‐system multistage metasomatic alteration in the presence of an aqueous solution–infiltration metasomatism. This process resulted in localized mobilization of all major rock‐forming elements: Si, Ca, Al, Ti, Mg, Fe, Mn, Na, K, and Cl. The metasomatic alteration of CK CAIs is more advanced and occurred under higher temperature and higher oxygen fugacity than that of the Allende CAIs.

Copyright and License

c2023 The Meteoritical Society.

Acknowledgement

This work supported by the Emerging Worlds NASA grant 80NSSC23K0253 (ANK, PI) and DOE-NNSA grant #DE-NA0004084 (S.B. Jacobsen, PI) is dedicated to our friend and colleague Dr. Edward R. D. Scott whose remarkably broad scientific interest included refractory inclusions, chondrules, chondritic matrices, irons, asteroidal and planetary achondrites, shock and thermal metamorphism, aqueous and metasomatic alteration, collisional evolution of asteroid belt, radial transport of solids in the protoplanetary disk, oxygen and nucleosynthetic isotopic anomalies, and many others. ANK will always remember stimulating discussions with Ed. We thank Dr. T. J. Fagan and two anonymous reviewers for their detailed comments and suggestions which helped to improve the manuscript. Editorial handling by Dr. A. J. Brearley is highly appreciated.

Supplemental Material

  • Figure EA1. Backscattered electron images of the CTA CAI #1 from NWA 4964 (CK3.8).
  • Figure EA2. Backscattered electron images of rhönite grains #1 (a, b, h), #2 (c, d), and #3 (e, f, g).
  • Figure EA3. Backscattered electron images of the Type B1 CAI #2 from NWA 5343 (CK3.7).
  • Figure EA4. Backscattered electron images of the FoB CAI #3 from NWA 5343 (CK3.7).

Additional Information

This article was published in the Special Issue: In memory of Edward R. D. Scott (1947–2021), Volume 59, Issue 4, April 2024, Pages 809-835

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Created:
December 4, 2024
Modified:
December 4, 2024