Explore the vast range of titles available.

Detailed descriptions of morphological features, morphometrics, neurocranium anatomy, clasper structure and egg case descriptions are provided for the thickbody skate Amblyraja frerichsi; a rare, deep-water species from Chile, Argentina and Falkland Islands. The species diagnosis is complemented from new observations and aspects such as colour, size and distribution are described. Geographic and bathymetric distributional ranges are discussed as relevant features of this taxons biology. Additionally, the conservation status is assessed including bycatch records from Chilean fisheries.

[This corrects the article DOI: 10.1371/journal.pbio.3000366.].

Physiculus cynodon is a member of the Moridae family and possesses a ventral bioluminescent organ. Although it has been captured by commercial vessels for decades, our understanding of its biology and ecology remains fragmented. This paper provides data on the species’ spatial and vertical distributions; age and growth; size, age, sex compositions; and sex ratio in the waters around the Emperor Seamounts and the northwestern Hawaiian Ridge. This information is based on the analysis of multi-year Russian data obtained from scientific surveys and observations on commercial fishing vessels. The northernmost capture of this species has been recorded at Nintoku Seamount. Additionally, this species was regularly encountered at depths ranging from 53 to 900 m on seamounts such as Lira (Annei), Koko, Milwaukee (Yuryaku and Kammu), Colahan, and C-H of the Emperor Seamounts and Hancock, Zapadnaya, and Academician Berg of the northwestern Hawaiian Ridge. Catch rates of P. cynodon gradually decreased in a southeastern direction. Notably, the relative abundance of this species in bottom trawl catches significantly surpasses that in pelagic catches. The age of the fish in the catch varied from 9 to 37 years, and its growth is described by the VBGF equation with the following coefficients: L∞ = 858.6, k = 0.030, t0 = 3.5. While the growth patterns for males and females were similar, it is worth mentioning that males rarely survive beyond the age of 25 years.

We present new observations on the dynamics and locations of deep mantle reservoirs derived from the ages and compositions of Voyager Seamount Chain lava flows. The previously unexplored Voyager Seamount Chain trends NW–SE between the Mid‐Pacific Mountains and the Northwestern Hawaiian Ridge. Volcanic samples were recovered from the chain during the Ocean Exploration Trust expedition NA134. The lava flows are alkalic to highly alkalic in composition. Ages ranged from 81 to 86 Ma (n = 8), with the oldest ages in the NW and an age‐progression toward the SE. The Voyager age‐progression continues southward through the Northern Line Islands region until at least 69 Ma. Mantle flowlines using absolute plate motion models indicate that the Voyagers were emplaced near the modern Marquesas Hotspot location approximately 86–69 Ma. The Sr‐Nd‐Pb‐Hf isotope systematics show the influence of an EMII component and overlap the compositions of Pliocene volcanism from the Marquesas Islands, consistent with the plate motion age model. These data imply a long‐lived plume as the source of the Voyager seamounts and the Marquesas. However, the lack of a clear and continuous seamount chain between the 86–69 Ma Voyager Seamount Chain and the 6–0 Ma Marquesas Islands implies that the mantle plume displays variable buoyancy flux over time. The surface expression of this mantle reservoir experienced a potential hiatus of up to ∼60 m.y. These new data indicate that the mantle beneath the Marquesas Islands region has been discontinuously producing age‐progressive, EMII‐like hotspot volcanism since at least the Late Cretaceous.

Volcanic seamount chains on the flanks of mid‐ocean ridges record variability in magmatic processes associated with mantle melting over several millions of years. However, the relative timing of magmatism on individual seamounts along a chain can be difficult to estimate without in situ sampling and is further hampered by Ar40/Ar39 dating limitations. The 8°20’N seamount chain extends ∼170 km west from the fast‐spreading East Pacific Rise (EPR), north of and parallel to the western Siqueiros fracture zone. Here, we use multibeam bathymetric data to investigate relationships between abyssal hill formation and seamount volcanism, transform fault slip, and tectonic rotation. Near‐bottom compressed high‐intensity radiated pulse, bathymetric, and sidescan sonar data collected with the autonomous underwater vehicle Sentry are used to test the hypothesis that seamount volcanism is age‐progressive along the seamount chain. Although sediment on seamount flanks is likely to be reworked by gravitational mass‐wasting and current activity, bathymetric relief and Sentry vehicle heading analysis suggest that sedimentary accumulations on seamount summits are likely to be relatively pristine. Sediment thickness on the seamounts' summits does not increase linearly with nominal crustal age, as would be predicted if seamounts were constructed proximal to the EPR axis and then aged as the lithosphere cooled and subsided away from the ridge. The thickest sediments are found at the center of the chain, implying the most ancient volcanism there, rather than on seamounts furthest from the EPR. The nonlinear sediment thickness along the 8°20’N seamounts suggests that volcanism can persist off‐axis for several million years. Plain Language Summary Most of the volcanism on Earth happens in the oceans, at mid‐ocean ridges where plates spread apart. In some places, however, chains of volcanoes that extend over distances of hundreds of kilometers long can form away from the ridge axis. The formation of these volcanic chains, called off‐axis seamounts, is poorly understood, yet understanding their origins will help learn about processes taking place deep inside Earth's mantle. We used a sonar carried by an underwater robot in water depths of ∼3 km to measure the thickness of sedimentary mud on top of a seamount chain in the eastern Pacific Ocean at 8°20’N. The thicker the sediment, the greater the time that has passed since the last volcanic eruption. We found that sediments do not simply thicken with seafloor age, implying that volcanoes in these types of seamount chains can remain active over millions of years. Key Points Regional bathymetry and near‐bottom sonar surveys investigate the structure and history of the 8°20’N seamount chain, west of the East Pacific Rise (EPR) Sediment thickness from autonomous underwater vehicle subbottom compressed high‐intensity radiated pulse images are used to estimate the relative age of magmatism at nine seamounts along chain Sediment thickness does not increase with distance from the EPR axis, implying that magmatism was episodic and prolonged

Abstract The discharge of hydrothermal vents on the seafloor provides energy sources for dynamic and productive ecosystems, which are supported by chemosynthetic microbial populations. These populations use the energy gained by oxidizing the reduced chemicals contained within the vent fluids to fix carbon and support multiple trophic levels. Hydrothermal discharge is ephemeral and chemical composition of such fluids varies over space and time, which can result in geographically distinct microbial communities. To investigate the foundational members of the community, microbial growth chambers were placed within the hydrothermal discharge at Axial Seamount (Juan de Fuca Ridge), Magic Mountain Seamount (Explorer Ridge), and Kamaʻehuakanaloa Seamount (Hawai'i hotspot). Campylobacteria were identified within the nascent communities, but different amplicon sequence variants were present at Axial and Kamaʻehuakanaloa Seamounts, indicating that geography in addition to the composition of the vent effluent influences microbial community development. Across these vent locations, dissolved iron concentration was the strongest driver of community structure. These results provide insights into nascent microbial community structure and shed light on the development of diverse lithotrophic communities at hydrothermal vents. Microbial diversity is quickly established in growth chambers incubated at hydrothermal vents and nascent communities are driven by chemistry and location.

Upwelling and decompression of mantle plumes is the primary mechanism for large volumes of intraplate volcanism; however, many seamounts do not correlate spatially, temporally, or geochemically with plumes. One region of enigmatic volcanism in the ocean basins that is not clearly attributable to plume‐derived magmatism is the Geologist Seamounts and the wider South Hawaiian Seamount Province (∼19°N, 157°W). Here we present new bathymetric maps as well as 40Ar/39Ar age determinations and major and trace element geochemistry for six remote‐operated vehicle recovered igneous rock samples (NOAA‐OER EX1504L3) and two dredged samples (KK840824‐02) from the Geologist Seamounts. The new ages indicate that volcanism was active from 90 to 87 Ma and 74 to 73 Ma, inferring that in conjunction with previous ages of ∼84 Ma, seamount emplacement initiated near the paleo Pacific‐Farallon spreading ridge and volcanism spanned at least ∼17 m.y. Geochemical analyses indicate that Geologist Seamount lava flows are highly alkalic and represent low‐degree partial mantle melts primarily formed from a mixture of melting within the garnet and spinel stability field. The ages and morphology inferred that the seamounts were likely not related to an extinct plume. Instead, we build upon previous models that local microblock formation corresponded to regional lithospheric extension. We propose that the microblock was bounded by the Molokai and short‐lived Kana Keoki fracture zones. Regional deformation and corresponding volcanism among the Geologist Seamounts associated with the microblock potentially occurred in pulses contemporaneous to independently constrained changes in Pacific Plate motion—indicating that major changes in plate vectors can generate intraplate volcanism. Plain Language Summary Seamounts are volcanic structures on the seafloor that do not breach the surface of the ocean. Most large (e.g., >3 km tall) seamounts are generated from mantle plumes, which are buoyant “blobs” of anomalously hot mantle that are derived from deep in the Earth's interior. These mantle plumes tend to be fixed in their geographic position relative to the mobile lithosphere, ultimately resulting in chains of age‐progressive volcanoes (e.g., Hawaiian Islands). However, many seamounts within the ocean basins are not consistent with mantle plume related characteristics like age‐progressions. Here we provide new eruption age and chemistry information for volcanics situated within the Geologists Seamount Cluster. The Geologist Seamount Cluster is a group of Cretaceous aged seamounts south of the Hawaiian Islands within the U.S. exclusive economic zone. The lava flows range in age from 90 to 73 Ma, indicating that at least 17 million years of volcanic activity occurred in the region. The best model to explain the origin of this volcanism is the thinning of the oceanic lithosphere, which causes the hot mantle to ascend and melt, while the structure of the nearby divergent plate boundary (ancient Pacific‐Farallon Ridge) was being reconfigured. Key Points Volcanic episodes within the Geologist Seamount clusters range from 90 to 73 Ma Each volcanic episode has distinct seamount morphology Pulses of deformation of the young oceanic lithosphere appear to be the best fit for the origin of the volcanism

Seamounts are isolated elevations in the seafloor with circular or elliptical plans, comparatively steep slopes, and relatively small summit area (Menard, 1964). The vertical gravity gradient (VGG), which is the curvature of the ocean surface topography derived from satellite altimeter measurements, has been used to map the global distribution of seamounts (Kim & Wessel, 2011, https://doi.org/10.1111/j.1365-246x.2011.05076.x). We used the latest grid of VGG to update and refine the global seamount catalog; we identified 19,325 new seamounts, expanding a previously published catalog having 24,643 seamounts. Seven hundred thirty‐nine well‐surveyed seamounts, having heights ranging from 421 to 2,500 m, were used to estimate the typical radially symmetric seamount morphology. First, an Empirical Orthogonal Function (EOF) analysis was used to demonstrate that these small seamounts have a basal radius that is linearly related to their height—their shapes are scale invariant. Two methods were then used to compute this characteristic base to height ratio: an average Gaussian fit to the stack of all profiles and an individual Gaussian fit for each seamount in the sample. The first method combined the radial normalized height data from all 739 seamounts to form median and median‐absolute deviation. These data were fit by a 2‐parameter Gaussian model that explained 99.82% of the variance. The second method used the Gaussian function to individually model each seamount in the sample and further establish the Gaussian model. Using this characteristic Gaussian shape we show that VGG can be used to estimate the height of small seamounts to an accuracy of ∼270 m. Key Points We used the latest vertical gravity gradient maps to update and refine a global seamount catalog, finding 19,325 new seamounts Smaller seamounts (<2,500 m tall) having good bathymetry coverage (739) were modeled with a radially symmetric Gaussian function Two modeling approaches show that smaller seamounts have a sigma to height ratio of 2.4 which agrees with an earlier study by Smith (1988)

The formerly continuous Vitiaz Arc broke into its Vanuatu and Fijian portions during a reversal of subduction polarity in the Miocene. Basaltic volcanism in Fiji that accompanied the breakup ranged from shoshonitic to low‐K and boninitic with increasing distance from the broken edge of the arc that, presumably, marks the broken edge of the slab. The Sr‐Pb‐Nd isotope ratios of the slab‐derived component in the breakup basalts most closely match those of the isotopically most depleted part of the Samoan seamount chain on the Pacific Plate that was adjacent to the site of breakup at 4–8 Ma, and differ from those of subsequent basalts in spreading segments of the surrounding backarc North Fiji and Lau Basins. Subduction of the Samoan Chain along the Vitiaz Trench Lineament may have controlled the limit of polarity reversal and, hence, where the double saloon doors (Martin, 2013) opened. Prior to breakup, Fijian volcanics were more similar isotopically to the Louisville Seamount Chain. Plain Language Summary The subduction zone that included Tonga and Fiji was once connected to Vanuatu. We attribute the arc breakup to subduction of the Samoan Seamount Chain. Volcanism in Fiji accompanying breakup ranges from shoshonitic closest the tear in the arc, to low‐K and boninitic farthest from it. The ambient mantle source of magma during breakup was the same as earlier in arc history but the slab‐derived component changed during breakup. Post‐breakup volcanism came from different mantle unaffected by subduction and derived from beneath the Pacific Plate. Key Points The breakup between Fiji and Vanuatu may have been triggered by subduction of Samoan seamounts Shoshonitic to low‐K and boninitic volcanism accompanied breakup with increasing distance from the break The mantle source of later basalts in surrounding backarc basins and islands came from beneath the Pacific Plate north of the breakup site

Enriched mid‐ocean ridge basalts (E‐MORB) commonly erupt at mid‐ocean ridges (MOR) and seamounts, but their relationship to “depleted” MORB (D‐MORB) and the processes controlling their magmatic evolution at MORs are not fully understood, hence raising more general questions about magma generation in the mantle. We here explore this conundrum through an investigation of the Masirah ophiolite (southeast Oman), a near‐unique “true” MOR ophiolite. Unlike most (e.g., Tethyan) ophiolites, it was not affected by subduction and is therefore potentially able to provide valuable geological insights into the magmatic evolution of a full section of oceanic crust. Previous work has shown that the igneous crust at Masirah was thin (1.5–2.0 km) and constructed from both D‐ and E‐MORB magmas, concluding that it formed at a slow‐spreading ridge at ∼150 Ma followed by an episode of “Nb‐enriched” magmatism with trace‐element enrichments exceeding E‐MORB during intraplate rifting ∼20 Ma later. We reinvestigate the geology of Masirah and present new field observations, geochemical data and high‐precision U‐Pb ages to constrain the magmatic history of seafloor spreading and off‐axis magmatism. We found that D‐MORB and E‐MORB magmatism at Masirah was synchronous and overlapped in both composition and time with the Nb‐enriched magmatism (no older than 135 Ma). Both types of magmatism were therefore integral in the formation of the Masirah ocean crust. The relationship between D‐MORB and E‐MORB magmatism described here may be applicable to modern MORs more broadly, but is especially prominent at Masirah due to reduced magmatism and hence a weaker crustal filter. Plain Language Summary The oceanic crust forms approximately two‐thirds of the Earth's surface and is continuously being formed at mid‐ocean ridges. Due to the difficulties involved in accessing oceanic crust directly, especially the deeper stratigraphic levels, the magmatic processes involved in forming the oceanic crust remain poorly understood. Ophiolites, fragments of oceanic lithosphere that were emplaced onto the continent, can offer valuable insights to geologists, but since most ophiolites are thought to have originated in marginal oceanic basins or at the initiation of subduction, a direct comparison remains problematic. In this study, we circumvent this problem by investigating the Masirah Ophiolite, a rare example of a “true” mid‐ocean ridge ophiolite. By combining field observations, geochemistry and geochronology at a level of detail not possible for present‐day oceanic crust, we reconstruct the magmatic evolution of the Masirah paleoridge. We present a more accurate formation age for Masirah and find that magmatism was compositionally variable throughout crustal accretion, with later off‐axis melts becoming more enriched in incompatible trace elements. We propose that the large geochemical variations observed at Masirah may be commonplace at modern mid‐ocean ridges, but that these are often masked due to the typically higher volumes of magmatism that enhance mixing and homogenization. Key Points Two ophiolite nappes exposed on Masirah were formed by ocean crustal accretion at 135 and 131 Ma respectively On‐axis magmatism shows varying degrees of trace element enrichment and depletion, and is followed by Nb‐enriched “near‐axis” magmatism Similar processes may be common along modern mid‐ocean ridges but masked by the homogenizing effect of an enhanced “crustal filter”