Implications of the Temporal Distribution of High‐Mg Magmas for Mantle Plume Volcanism Through Time Author(S): Ann E
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Implications of the Temporal Distribution of High‐Mg Magmas for Mantle Plume Volcanism through Time Author(s): Ann E. Isley and Dallas H. Abbott Source: The Journal of Geology, Vol. 110, No. 2 (March 2002), pp. 141-158 Published by: University of Chicago Press Stable URL: http://www.jstor.org/stable/10.1086/338553 Accessed: 22-01-2016 15:05 UTC Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at http://www.jstor.org/page/ info/about/policies/terms.jsp JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. University of Chicago Press is collaborating with JSTOR to digitize, preserve and extend access to The Journal of Geology. http://www.jstor.org This content downloaded from 129.236.224.227 on Fri, 22 Jan 2016 15:05:16 UTC All use subject to JSTOR Terms and Conditions Implications of the Temporal Distribution of High-Mg Magmas for Mantle Plume Volcanism through Time Ann E. Isley and Dallas H. Abbott1 Department of Earth Sciences, Oswego State University of New York, Oswego, New York 13126, U.S.A. (e-mail: [email protected]) ABSTRACT We compile a 3.7-b.yr.-long time series of ultramafic and mafic rocks including extrusives and shallow intrusives (dikes and sills). We infer that peaks in the time series represent mantle plume events. Rocks erupted from plumes are becoming more Ti rich through time, and several rock types having 118 wt % MgO are Phanerozoic analogs for komatiites. These include meimechites, ankaramites, and rocks previously called “picrites.” Spectral analysis reveals the time series is driven by periods of ∼800 and ∼273 m.yr. Two 256-m.yr.-long data subsets, one sampling the Archean -.m.yr., respectively. The ∼800-m.yr 4.5 ע and 34.5 3 ע and one sampling the Phanerozoic, are driven by periods of26 long energy may reflect changes in the rate of impacts of extraterrestrial objects, tectonic slab cascades into the mesosphere, or resonance between free-core nutations and those forced by solar torques. We suggest that the 273 m.yr. period reflects the cosmic year. The latter modulates fluctuation in cometary impacts that occur with a 30–35 m.yr. period (Matese et al. 1996). Thus, there may be more than one driving force for mantle plume volcanism, including forces endogenic and exogenic to Earth. Introduction In a recent article, we discussed the temporal dis- mantle plume events because they capture both tribution of Archean and Paleoproterozoic mafic continental and putative oceanic flood basalt se- and ultramafic igneous events and inferred that ep- quences. Although they were once thought to be isodes of substantially increased basic magmatism typical of Archean mid-ocean ridge crust, komati- reflect mantle plume volcanism (Isley and Abbott ites actually had sources a few to several 100ЊC 1999). Since that work, we have compiled a data hotter than the average mantle, even in the Ar- set of the ages of high-Mg volcanic units and high- chean (Abbott et al. 1994; Puchtel et al. 1998b; Mg dikes and sills spanning more than 3.7 Ga of therefore, even Precambrian komatiites are now Earth history. (For brevity’s sake, this data set has generally acknowledged as expressions of mantle been included in The Journal of Geology’s data de- plume volcanism (Campbell et al. 1989; Campbell pository.) In this article, we analyze the time series to evaluate secular changes in the chemistry of and Griffiths 1990). However, the degree to which high-Mg lavas and to determine whether there are all komatiites reflect high mantle temperatures is well-defined periodicites in the data set. This work debatable since komatiites could have formed by may provide insights into the forces that ultimately melting of a hydrous mantle with temperatures drive mantle plume events. only 150ЊC higher at the top of the asthenosphere In our previous work, we investigated four prox- than at present (Gromshei et al. 1990). Some have ies of mantle plume activity: komatiites, continen- argued that komatiites are not necessarily the prod- tal flood basalts, mafic dikes, and layered (ul- ucts of mantle plumes (Burke 1997; De Wit 1998). tra)mafic intrusions (Isley and Abbott 1999). However, the lack of both degassing structures and Komatiites proved particularly robust proxies of porphyritic textures in most komatiites and their chemical and isotopic signatures led Arndt et al. Manuscript received October 31, 2000; accepted August 14, (1998) to conclude that, although some rare ko- 2001. 1 Lamont-Doherty Earth Observatory of Columbia Univer- matiites were hydrous, most were not. We concur sity, Palisades, New York 10964, U.S.A. and maintain that, while komatiites may not be [The Journal of Geology, 2002, volume 110, p. 141–158] ᭧ 2002 by The University of Chicago. All rights reserved. 0022-1376/2002/11002-0002$15.00 141 This content downloaded from 129.236.224.227 on Fri, 22 Jan 2016 15:05:16 UTC All use subject to JSTOR Terms and Conditions 142 A. E. ISLEY AND D. H. ABBOTT perfect recorders of mantle plume activity, they are (2000), and modeled by Sparks (1986) and Jellinek among the most robust indicators available. and Kerr (1999). Rocks with MgO of 10–14 wt % We found other proxies of mantle plume activity whose geochemistries did not dictate admixture of less dynamic (Isley and Abbott 1999). For example, a high-Mg melt with another source were excluded mantle plume events promote mafic dike swarms, from the data set. but not all mafic dike swarms are the result of man- Rocks referred to in this work are described using tle plume volcanism nor are all layered igneous in- the 1989 IUGS classification so that we use the trusions necessarily the result of mantle plume vol- same term that was applied to rocks in the original canism. It may be necessary to cull these data sets studies we cite. We note that the rocks we refer to to obtain clear signals of mantle plume activity. here as “komatiite” and “meimechite” retain that Ernst and Buchan (1997), for example, drew infer- nomenclature in the recent IUGS reclassification ences about plumes by focusing only on giant ra- (Le Bas 2000). However, some of the rocks that were diating dike swarms. previously termed “basaltic komatiite,” “komati- Here, we focus on the geologic record of high-Mg itic basalt,” “picritic basalt,” and “high-Mg basalt” lavas, including komatiites. Most komatiites might now be called “picrite.” Rocks having 118 erupted before the beginning of the Mesoprote- ϩ wt % MgO and 1–2 wt %Na22 O KO , previously rozoic (1.6 Ga). Assessing mantle plume activity labeled picrites, would now be referred to as “mei- from the Mesoproterozoic onward requires a proxy mechites” (Le Bas 2000). or proxies in addition to komatiites. Several other There are several examples of Phanerozoic ko- lithologies are as rich in MgO as komatiites (e.g., matiites in the data set. There is a long-standing meimechites). Because the ratios Mg/Si and Fe/Si conviction that the only Phanerozoic komatiites increase in mafic volcanics as a function of either are those of Gorgona Island (e.g., Kerr et al. 1996). melt-source temperature or degree of melting However, several other sequences have units with (which may also reflect mantle temperature), we an MgO component consistent with komatiitic include other high-Mg rocks in the data set. chemistry. Spinifex texture has been reported for most of these sequences (Buturlinov and Kisil’ Data Set Description 1985; Paraskevopoulos and Economou 1986; Struy- eva 1988; Spadea et al. 1989; Fang and Ma 1994; The Lithologies. The International Union of Geo- Alvarado et al. 1997). logical Sciences (IUGS) recently reclassified high- Many ankaramites from the pre-Cenozoic record Mg rocks (Le Bas 2000). Previously, rocks having have been interpreted as island arc volcanics. These 118 wt % MgO were called “picrites,” “ferropic- ankaramites all are associated with calc-alkaline rites,” “ankaramites,” “komatiites,” or “meime- volcanic sequences. Cenozoic ankaramites com- chites” (using the IUGS recommendations for no- prise some of the volcanic units in the Lesser An- menclature from 1989 and earlier). Rocks with 118 ϩ tilles, Indonesian, Vanuata, and Izu-Bonin arcs wt % MgO andNa22 O KO of 1–2 wt % were called “picrites.” If such rocks were enriched in Fe, (Hawkesworth et al. 1979; Maillet 1982; Foden they were called “ferropicrites” (Gibson et al. 1983; Fukuyama 1983). However, there are many 2000). Ankaramites were a subset of picrites rich more examples of Cenozoic ankaramites associated in titanian augite. Rocks less alkaline than picrites with hotspots and mantle plumes (Isley and Abbott were termed “komatiites” or “meimechites.” Ko- 2000). For example, ankaramites contribute to the ! volcanic extrusives erupting from 120 hotspots, in- matiites had 1wt%TiO2, while meimechites cluding the Jan Mayan, Icelandic, Azores, Trindade, were richer in TiO2. There is a host of lithologies that are compositionally analogous to mixtures of Society, Samoan, and Hawaiian hotspots (Johnson komatiitic, (ferro)picritic, and/or basaltic magmas. et al. 1986; Kennedy et al. 1991; Pegram and Allegre Such rocks include picritic komatiite, basaltic ko- 1992; Stecher 1998; Guest et al. 1999; Fodor and matiite, komatiitic basalt, picritic basalt, and high- Hanan 2000). In this work, we assume that all vol- Mg basalt. The data set includes such mixtures, and canic sequences containing ankaramites but lack- a few of these sequences have units with MgO be- ing dominant associations with calc-alkaline rocks tween 10 and 14 wt %.