A PETROLOGIC AND ISOTOPIC STUDY OF LODRANITES - EVIDENCE FOR EARLY FORMATION AS PARTIAL MELT RESIDUES FROM HETEROGENEOUS PRECURSORS

Citation
Tj. Mccoy et al., A PETROLOGIC AND ISOTOPIC STUDY OF LODRANITES - EVIDENCE FOR EARLY FORMATION AS PARTIAL MELT RESIDUES FROM HETEROGENEOUS PRECURSORS, Geochimica et cosmochimica acta, 61(3), 1997, pp. 623-637
Citations number
69
Categorie Soggetti
Geochemitry & Geophysics
ISSN journal
00167037
Volume
61
Issue
3
Year of publication
1997
Pages
623 - 637
Database
ISI
SICI code
0016-7037(1997)61:3<623:APAISO>2.0.ZU;2-Z
Abstract
We have conducted petrologic, chemical, and isotopic studies of lodran ites in an attempt to constrain their genesis. Lodran, Gibson, Y-79149 1, Y-791493, Y-74357, Y-8002, Y-75274, MAC 88177, LEW 88280, EET 84302 , FRO 90011, and QUE 93148 are classified as lodranites. Lodranites an d acapulcoites are indistinguishable on the basis of oxygen isotopic c ompositions but are distinct in average grain sizes of their mafic sil icates, with lodranites being significantly coarser-grained. Lodranite s exhibit a diverse range of petrologic and mineralogic features: they range widely in mafic silicate compositions (Fa(3-13)), plagioclase ( 0-11.4 vol%), Fe,Ni metal (0.5-20 vol%), and troilite (0.2-5.3 vol%) c ontents; and shock levels (S1-S4). They appear to have experienced hig h peak temperatures and rapid cooling in the temperature range recorde d by metallographic cooling rates (i.e., 700-350 degrees C). The only dated lodranite, Gibson, cooled to Ar closure temperatures at 4.49 +/- 0.01 Ga. Lodranites formed from chemically and isotopically heterogen eous precursors in which the mineral and oxygen isotopic compositions were correlated. Heating of their parent body to temperatures between similar to 1050-1200 degrees C resulted in formation of Fe,Ni-FeS and basaltic partial melts. Depletions of troilite and/or plagioclase in m ost lodranites testify to the removal of some of these partial melts, although melt migration was complex. Lodranites appear to have experie nced a complex cooling history of slow cooling at high temperatures, f ollowed by rapid cooling at intermediate temperatures, possibly relate d to breakup of the parent body. Lodranites were liberated from their parent body during 1-3 impact events, with most having cosmic ray expo sure ages of 5.5-7 Ma. The acapulcoites are samples from the same pare nt body but were heated to lower temperatures and, thus, experienced l ower degrees of partial melting. Copyright (C) 1997 Elsevier Science L td.