Paleoceanography of the eastern equatorial Pacific over the past 4 million years and the geologic origins of modern Galápagos upwelling
Introduction
The Galápagos Archipelago (GA) is comprised of over one hundred islands and islets, many of which are volcanically active. While it is generally accepted that subaerial islands have existed in the GA for at least 17 million years (Werner et al., 1999, Werner and Hoernle, 2003), the timeline of their formation, emergence, and paleogeography remains highly uncertain (Geist et al., 2014). This uncertainty has broad implications; for example, it hinders our ability to piece together the evolution and migration of species in one of Earth's most famous natural laboratories.
The unique environmental conditions on the GA are in large part driven by the interaction of the islands themselves with basin-scale oceanography. Specifically, the GA stands directly in the path of the Equatorial Undercurrent (EUC) as it flows along the equator from the western Pacific toward South America at depth (Fig. 1). The direct result of this geologic coincidence is a very intense upwelling of cold, nutrient–rich water from the EUC along the western shores of the westernmost islands in the GA (Isabela and Fernandina). The effects of this tropical oasis of cold, highly productive surface water are felt throughout the entire GA ecosystem including on large animals such as penguins and fur seals (Boersma et al., 2013, Karnauskas et al., 2015).
The physical influence of the GA on ocean currents and sea surface temperature (SST) in the eastern equatorial Pacific (EEP) has been studied extensively through in situ observations (Stevenson and Taft, 1971, Christensen, 1971, Pak and Zaneveld, 1973, White, 1973, Leetmaa, 1982, Lukas, 1986, Steger et al., 1998, Sweet et al., 2009; Karnauskas et al., 2010, Karnauskas et al., 2014) and ocean general circulation model (OGCM) experiments (Brentnall, 1999, Eden and Timmermann, 2004, Cravatte et al., 2007; Karnauskas et al., 2007, Karnauskas et al., 2008, Karnauskas et al., 2014). The salient result, gleaned from observations and common across all model experiments, is that the presence of the GA serves to obstruct the EUC, thus cooling SST in the region immediately west of the GA (out to ∼95°W) and warming SST east of the GA (between the GA and mainland South America). In other words, the robust oceanographic fingerprint of the GA is a positive cross-island SST gradient (CI SST east of the GA–SST west of the GA), whereas the absence of the GA would correspond to a negative CI.
Over the past several decades, the paleoceanographic community has conducted extensive drilling operations throughout the world ocean, including the Pacific basin, toward reconstructing variations in Earth's climate spanning the past several million years (Fig. 1a). Quite fortuitously, the combined set of paleoceanographic SST proxy records from the far EEP (Fig. 1b) constitutes a paleo-observing network well suited for detecting potential geologic changes in the GA given its known oceanographic fingerprint. The primary goal of this study is to leverage the existing paleoceanographic SST reconstructions from the EEP along with a wide range of OGCM experiments to provide a new constraint on the geologic and biogeographic history of the GA. The paleoceanographic records and suite of model simulations are summarized in the following section, results are presented in section 3, implications for local geologic history and biogeography, as well as basin-scale climate transitions are discussed in section 4, and concluding remarks are offered in section 5.
Section snippets
Paleoceanographic reconstructions
We examine paleoceanographic reconstructions of SST at several locations throughout the global tropics and subtropics (Fig. 1) including the western equatorial Pacific (WPAC), the eastern equatorial Pacific near the GA (WGAL, SGAL, EGAL), and the margins of California (CAL1, CAL2), Peru (PERU), and western Africa (WAFR; Table 1). To calculate CIΔT, we employ three SST reconstructions based upon: 1) alkenone–only proxies, 2) combining alkenone and Mg/Ca proxies, and 3) combining alkenone and
Results
The mean alkenone–only CIΔT record since ∼1 Ma (∼0.2 °C) is very close to the modern annual mean CIΔT of 0.17 ± 0.29 °C as observed by high-resolution satellite observations (indicated by the gray error bar in Fig. 3; observational error bars ±2 standard errors of the mean using ). All three paleoceanographic reconstructions of CI reveal a shift in their mean values, including a change of sign, at approximately 1.6 Ma (Fig. 3). Based on the alkenone–only CIΔT record, the mean CIΔT for
Implications for geologic and biogeographic uncertainties
Hotspot volcanoes (e.g., Hawaii) generally form linear chains of seamounts and islands that exhibit a regular age progression as older volcanoes are carried away from the underlying mantle plume by tectonic plate motions (Wilson, 1973); magmatic activity in these cases is primarily limited to the youngest island in the chain. In contrast, historical volcanism in the GA occurs over a broad area encompassing several islands (e.g., Poland, 2014). Such widespread volcanism makes it difficult to
Summary and conclusions
The evolution of the regional-scale gradient of SST across the Galápagos Islands over the past ∼3 Ma was analyzed in multiple paleoceanographic SST reconstructions, revealing a highly significant shift in the mean CIΔT of over 1.5 °C at ∼1.6 Ma. The CIΔT was found to be consistent with that expected based on ocean model experiments isolating the effect of the Galápagos Islands, their emergence, and their impact on regional ocean circulation. Several important implications stem from this new
Acknowledgments
The authors thank Delia Oppo for helpful discussions on paleoclimate data sets and interpretations, Sloan Coats for assistance with change point calculations, Kira Lawrence and Alexey Fedorov for sharing some of the proxy records, and the NOAA Paleoclimate FTP portal for providing much of the proxy data. We are very grateful to the Ocean Drilling Program (ODP) including all whose work led to the acquisition, processing, and archival of paleoceanographic archives. R.M. acknowledges NASA PO and
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