AI Article Synopsis

  • The text discusses how the structure of rifted continental margins and associated magmatism provide insights into the strength of the lithosphere and the transition from rifting to seafloor spreading.
  • It distinguishes between narrow rifts, which form due to necking instabilities, and wide rifts, which need mechanisms like lower-crustal flow to control the extension process.
  • Recent findings from the PESCADOR seismic experiment show significant variations in rifting styles and magmatism in the Gulf of California, suggesting that mantle depletion influences wide, magma-poor margins while mantle fertility affects more active volcanic regions.

Article Abstract

Constraints on the structure of rifted continental margins and the magmatism resulting from such rifting can help refine our understanding of the strength of the lithosphere, the state of the underlying mantle and the transition from rifting to seafloor spreading. An important structural classification of rifts is by width, with narrow rifts thought to form as necking instabilities (where extension rates outpace thermal diffusion) and wide rifts thought to require a mechanism to inhibit localization, such as lower-crustal flow in high heat-flow settings. Observations of the magmatism that results from rifting range from volcanic margins with two to three times the magmatism predicted from melting models to non-volcanic margins with almost no rift or post-rift magmatism. Such variations in magmatic activity are commonly attributed to variations in mantle temperature. Here we describe results from the PESCADOR seismic experiment in the southern Gulf of California and present crustal-scale images across three rift segments. Over short lateral distances, we observe large differences in rifting style and magmatism--from wide rifting with minor synchronous magmatism to narrow rifting in magmatically robust segments. But many of the factors believed to control structural evolution and magmatism during rifting (extension rate, mantle potential temperature and heat flow) tend to vary over larger length scales. We conclude instead that mantle depletion, rather than low mantle temperature, accounts for the observed wide, magma-poor margins, and that mantle fertility and possibly sedimentary insulation, rather than high mantle temperature, account for the observed robust rift and post-rift magmatism.

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http://dx.doi.org/10.1038/nature06035DOI Listing

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