CaltechAUTHORS
  A Caltech Library Service

The origin of abyssal peridotites: a reinterpretation of constraints based on primary bulk compositions

Baker, Michael B. and Beckett, John R. (1999) The origin of abyssal peridotites: a reinterpretation of constraints based on primary bulk compositions. Earth and Planetary Science Letters, 171 (1). pp. 49-61. ISSN 0012-821X. doi:10.1016/S0012-821X(99)00130-2. https://resolver.caltech.edu/CaltechAUTHORS:20130305-074039435

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20130305-074039435

Abstract

We calculated primary bulk compositions for a global suite of abyssal peridotites using primary mineral modes and either analyzed or calculated phase compositions. The latter were obtained through correlations between reported mineral compositions and modal olivine contents. Both the modal data and the mineral compositions were averaged by dredge site, drill hole, or fracture zone (FZ) depending on the amount of available data. Our calculated abyssal peridotite compositions yield major-element oxide-MgO trends that are generally in good agreement with those based on compilations of ultramafic nodules and peridotite massifs. In particular, we find no statistically significant correlation between FeO* (total Fe as FeO) and MgO and, therefore, no evidence for significant olivine accumulation. Previous reports of a positive correlation reflect an artifact of the regressions used to calculate missing phase compositions and result in a relationship between the Mg# of olivine and modal olivine abundance that is inconsistent with observed variations in abyssal peridotites. There is a slight positive correlation between bulk FeO* and MgO if individual thin sections are used to derive the mineral composition versus modal olivine regressions, but the large grain sizes and heterogeneous distributions of phases within abyssal peridotities make it unlikely that individual thin section modes accurately reflect phase proportions in meter-sized dredge-haul samples. The variability of Na and Ti contents in pyroxenes from plagioclase-free abyssal peridotites suggests to us, as it has to other workers, that a majority of these samples interacted to varying degrees with small amounts of melt. On the other hand, lower bounds on Na and Ti contents in the pyroxenes at a given dredge site as a function of modal olivine content are broadly consistent with calculated partial melting residues. Thus, abyssal peridotites may retain information both on the original partial melting process and on concurrent or later interactions with partial melts from other sources.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/S0012-821X(99)00130-2DOIUNSPECIFIED
http://www.sciencedirect.com/science/article/pii/S0012821X99001302PublisherUNSPECIFIED
Additional Information:© 1999 Elsevier Science B.V. Received 13 July 1998; revised version received 1 June 1999; accepted 2 June 1999. This work was supported by NSF grant OCE-9529878 and NASA grant NAG5-4318. Discussions with K. Nolan and formal reviews by D. Francis, F. Frey, and K. Johnson are gratefully acknowledged.
Funders:
Funding AgencyGrant Number
NSFOCE-9529878
NASANAG5-4318
Subject Keywords:peridotites; mineral composition; partial melting; mid-ocean ridge basalts; igneous rocks; genesis
Issue or Number:1
DOI:10.1016/S0012-821X(99)00130-2
Record Number:CaltechAUTHORS:20130305-074039435
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130305-074039435
Official Citation:Michael B. Baker, John R. Beckett, The origin of abyssal peridotites: a reinterpretation of constraints based on primary bulk compositions, Earth and Planetary Science Letters, Volume 171, Issue 1, 15 August 1999, Pages 49-61, ISSN 0012-821X, 10.1016/S0012-821X(99)00130-2.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37284
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 Mar 2013 16:15
Last Modified:09 Nov 2021 23:28

Repository Staff Only: item control page