PhD candidate, California Institute of Technology, during AGeS project

What makes continental arcs tick?

Proposal Title: Timing of Mafic Intrusions Relative to Granitic Pluton Emplacement in the Sierra Nevada Batholith

Continental arcs are generated when an oceanic plate dives (i.e. subducts) beneath continental crust, causing melting in the mantle and the formation of volcanoes on the overriding continent. In addition to volcanoes at the surface, arcs form a column of solidified and partially crystallized magma from the mantle (30-50 km maximum depth) to just below the surface (~1 km depth). This solidified intrusive section of an arc is known as a batholith, and is commonly exposed at the Earth’s surface millions of years after the cessation of subduction and volcanism.


Simplified cross section of an active continental arc, with intrusive batholith and volcanic sections.

Most studies agree that arcs are the main sources of new continental crust on Earth’s crust today (e.g. Rudnick 1995). However, the rate of magma addition to the crust is not constant over an arc’s lifetime (10s to several hundred million years). The idea of “arc tempos” comes from the observation of cyclical flare-up and lull periods in continental arcs globally (Decelles et al. 2009), showing that 80-90% of the final batholith volume intrudes during ~10-20 million year flare-up periods. The drivers of arc tempos are not well understood, yet have significant implications for the generation of magma in arc settings. This leads to our big question: what makes continental arcs flare-up?


Examples of arc flare-up and lull periods from Cordilleran magmatic arcs, from Ducea et al. 2015. Note the late-Jurassic (160-140 Ma) and late-Cretaceous (105-80 Ma) in the Sierra Nevada batholith

Our natural laboratory for this project is the Sierra Nevada batholith (SNB) in eastern California, a very well exposed paleo-continental arc. The arc was active from ~210-80 million years ago, with flare-up periods in the late-Jurassic and late-Cretaceous. This project approaches the question of tempos through a new lens: what role do mafic melts play in batholith generation? Though this area has been very well studied in terms of the granodiorites that make up the bulk of the batholith, little focus has been given to gabbro to diorite intrusions. Though these bodies are small (25 km2 or less) compared to very large granitoid suites (up to 1200 km2), they are closer in composition to mantle-derived melts. This gives us the opportunity to test whether mantle input influences arc tempos.


Left: generalized outline of the Sierra Nevada Batholith, CA. Right: simplified geologic map of the central-Eastern SNB, showing the locations of mafic complexes (adapted from Frost, 1987)

We visited 17 mafic bodies in the central SNB, collecting representative mafic samples for geochronology as well as some granitic samples from intrusions that had not been dated by any previous studies. Many thanks to my advisor Claire Bucholz, and to my field assistants Juliet Ryan-Davis, Allyson Trussel, Joe Biasi, and Liane Lewis for their help with sampling! Scroll through some field photos below: