Paterno R. Castillo
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Research Interests
Paterno R. Castillo has a total of 133 co-authors. Here are the top co-authors by number of shared publications:
David R. Hilton
7 shared publications- Philip E. Janney
University of Cape Town Department of Geological Sciences 13 University Avenue, Rondebosch 7701
5 shared publications James W. Hawkins
4 shared publications- Barry B. Hanan
San Diego State University
3 shared publications - James M. D. Day
Scripps Institution of Oceanography University of California San Diego La Jolla California USA
3 shared publications Ji-Feng Xu
3 shared publications
Latest Publications
- Open Access
- 21 April 2026
- Published by National Academy of Sciences in Proceedings of the National Academy of Sciences
- Vol. 123 (17)
Ancient felsic sediments recycled through the deep mantle by plate tectonics
Many petrological, geodynamical, and geochemical perspectives have offered circumstantial evidence for either an early onset of plate tectonics in the first 10% of Earth’s history or a late onset after the great oxidation event (2.5 Ga ago). This calls into question over what timescales plate tectonics have influenced terrestrial geological and geochemical processes. We present geochemical data from the products of ancient crustal subduction, which were recycled into the deep mantle and then tapped by the modern Marquesas volcanic hotspot. We demonstrate that these materials have distinct short-lived radiogenic ( 146 Sm- 142 Nd, t 1/2 = 103 Ma) isotopic compositions (average μ 142 Nd = +2.3 ±1.3, n = 3) compared to other Marquesas lavas (average μ 142 Nd = −0.8 ±1.2, n = 7). These results require that the history of these subduction products diverged from those of other Marquesas magmas more than four billion years ago. Quantitative modeling suggests that the most geochemically enriched Marquesas samples represent up to ~0.6% recycled crustal sediments, which may have been subducted at any time in Earth’s history but were most likely subducted in the late Hadean Eon to early Eoarchean Era. The inferred felsic composition of such materials further requires that both crustal melting and sedimentation processes were active in some form on the early Earth. Further, the preservation of evidence for foundational planetary events in geologically young rocks reveals that Earth’s volcanic hotspots could provide a defining perspective on the early planetary-scale processes that build Earth-like planets.
- 21 April 2026
- Published by National Academy of Sciences in Proceedings of the National Academy of Sciences
- Vol. 123 (17)
Open AccessAncient felsic sediments recycled through the deep mantle by plate tectonics
Many petrological, geodynamical, and geochemical perspectives have offered circumstantial evidence for either an early onset of plate tectonics in the first 10% of Earth’s history or a late onset after the great oxidation event (2.5 Ga ago). This calls into question over what timescales plate tectonics have influenced terrestrial geological and geochemical processes. We present geochemical data from the products of ancient crustal subduction, which were recycled into the deep mantle and then tapped by the modern Marquesas volcanic hotspot. We demonstrate that these materials have distinct short-lived radiogenic ( 146 Sm- 142 Nd, t 1/2 = 103 Ma) isotopic compositions (average μ 142 Nd = +2.3 ±1.3, n = 3) compared to other Marquesas lavas (average μ 142 Nd = −0.8 ±1.2, n = 7). These results require that the history of these subduction products diverged from those of other Marquesas magmas more than four billion years ago. Quantitative modeling suggests that the most geochemically enriched Marquesas samples represent up to ~0.6% recycled crustal sediments, which may have been subducted at any time in Earth’s history but were most likely subducted in the late Hadean Eon to early Eoarchean Era. The inferred felsic composition of such materials further requires that both crustal melting and sedimentation processes were active in some form on the early Earth. Further, the preservation of evidence for foundational planetary events in geologically young rocks reveals that Earth’s volcanic hotspots could provide a defining perspective on the early planetary-scale processes that build Earth-like planets.
- 28 May 2025
- Published by Elsevier in Science Bulletin
- Vol. 70 (20) , 3290-3292
Origin of the Daly gap
- Open Access
- 22 July 2024
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 643
Overlapping hotspot tracks and melts from diffuse plume materials in the upper mantle generated intraplate seamount groups in the West Pacific
- 22 July 2024
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 643
Open AccessOverlapping hotspot tracks and melts from diffuse plume materials in the upper mantle generated intraplate seamount groups in the West Pacific
- Open Access
- 15 October 2023
- Published by Elsevier in Chemical Geology
- Vol. 641, 121780
Petrogenesis of alkaline magmas across a continent to ocean transect, northern Ross Sea, Antarctica
- 15 October 2023
- Published by Elsevier in Chemical Geology
- Vol. 641, 121780
Open AccessPetrogenesis of alkaline magmas across a continent to ocean transect, northern Ross Sea, Antarctica
- 1 December 2020
- Published by Elsevier in Chemical Geology
- Vol. 557
New geochemical and Sr-Nd-Pb isotope evidence for FOZO and Azores plume components in the sources of DSDP Holes 559 and 561 MORBs
- 1 December 2020
- Published by Elsevier in Chemical Geology
- Vol. 557
New geochemical and Sr-Nd-Pb isotope evidence for FOZO and Azores plume components in the sources of DSDP Holes 559 and 561 MORBs
- 1 September 2019
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 261, 1-19
Osmium isotope evidence for a heterogeneous 3He/4He mantle plume beneath the Juan Fernandez Islands
- 1 September 2019
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 261, 1-19
Osmium isotope evidence for a heterogeneous 3He/4He mantle plume beneath the Juan Fernandez Islands
- Open Access
- 8 October 2018
- Published by Springer Nature in Scientific Reports
- Vol. 8 (1) , 1-7
Marine Carbonates in the Mantle Source of Oceanic Basalts: Pb Isotopic Constraints
For almost fifty years, geochemists have been interpreting the clues from Pb isotopic ratios concerning mantle composition and evolution separately. The Pb isotopes of ocean island basalts (OIB) indicate that their mantle source is heterogeneous, most likely due to the presence of end-components derived from recycled crust and sediment. Some OIB have unusually high 206Pb/204Pb coming from one of the end-components with a long time-integrated high 238U/204Pb or μ (HIMU). Most OIB and many mid-ocean ridge basalts (MORB) also have high 206Pb/204Pb, indicating a HIMU-like source. Moreover, measured 232Th/238U (κ) for most MORB are lower than those deduced from their 208Pb/204Pb and 206Pb/204Pb. Such high μ and low κ features of oceanic basalts are inconsistent with the known geochemical behavior of U, Pb and Th and temporal evolution of the mantle; these have been respectively termed the 1st and 2nd Pb paradox. Here we show that subducted marine carbonates can be a source for HIMU and a solution to the Pb paradoxes. The results are consistent with the predictions of the marine carbonate recycling hypothesis that posits the Pb isotopes of oceanic basalts indicate a common origin and/or magma generation process.
- 8 October 2018
- Published by Springer Nature in Scientific Reports
- Vol. 8 (1) , 1-7
Open AccessMarine Carbonates in the Mantle Source of Oceanic Basalts: Pb Isotopic Constraints
For almost fifty years, geochemists have been interpreting the clues from Pb isotopic ratios concerning mantle composition and evolution separately. The Pb isotopes of ocean island basalts (OIB) indicate that their mantle source is heterogeneous, most likely due to the presence of end-components derived from recycled crust and sediment. Some OIB have unusually high 206Pb/204Pb coming from one of the end-components with a long time-integrated high 238U/204Pb or μ (HIMU). Most OIB and many mid-ocean ridge basalts (MORB) also have high 206Pb/204Pb, indicating a HIMU-like source. Moreover, measured 232Th/238U (κ) for most MORB are lower than those deduced from their 208Pb/204Pb and 206Pb/204Pb. Such high μ and low κ features of oceanic basalts are inconsistent with the known geochemical behavior of U, Pb and Th and temporal evolution of the mantle; these have been respectively termed the 1st and 2nd Pb paradox. Here we show that subducted marine carbonates can be a source for HIMU and a solution to the Pb paradoxes. The results are consistent with the predictions of the marine carbonate recycling hypothesis that posits the Pb isotopes of oceanic basalts indicate a common origin and/or magma generation process.
- Open Access
- 15 March 2018
- Published by American Geophysical Union (AGU) in Geochemistry, Geophysics, Geosystems
- Vol. 19 (3) , 807-837
Geology of the Alarcon Rise, Southern Gulf of California
Meter‐scale AUV bathymetric mapping and ROV sampling of the entire 47 km‐long Alarcon Rise between the Pescadero and Tamayo transforms show that the shallowest inflated portion of the segment hosts all four active hydrothermal vent fields and the youngest, hottest, and highest effusion rate lava flows. This shallowest inflated part is located ∼1/3 of the way between the Tamayo and Pescadero transforms and is paved by a 16 km2 channelized flow that erupted from 9 km of en echelon fissures and is larger than historic flows on the East Pacific Rise or on the Gorda and Juan de Fuca Ridges. Starting ∼5 km south of the Pescadero transform, 6.5 km of the Alarcon Rise is characterized by faulted ridges and domes of fractionated lavas ranging from basaltic andesite to rhyolite with up to 77.3 wt % SiO2. These are the first known rhyolites from the submarine global mid‐ocean ridge system. Silicic lavas range from >11.7 ka, to as young as 1.1 ka. A basalt‐to‐basaltic andesite sequence and an andesite‐to‐dacite‐to‐rhyolite sequence are consistent with crystal fractionation but some intermediate basaltic andesite and andesite formed by mixing basalt with dacite or rhyolite. Magmatism occurred along the bounding Tamayo and Pescadero transforms as extensive channelized flows. The flows erupted from ring faults surrounding uplifted sediment hills inferred to overlie sills. The transforms are transtensional to accommodate magma migration from the adjacent Alarcon Rise.
- 15 March 2018
- Published by American Geophysical Union (AGU) in Geochemistry, Geophysics, Geosystems
- Vol. 19 (3) , 807-837
Open AccessGeology of the Alarcon Rise, Southern Gulf of California
Meter‐scale AUV bathymetric mapping and ROV sampling of the entire 47 km‐long Alarcon Rise between the Pescadero and Tamayo transforms show that the shallowest inflated portion of the segment hosts all four active hydrothermal vent fields and the youngest, hottest, and highest effusion rate lava flows. This shallowest inflated part is located ∼1/3 of the way between the Tamayo and Pescadero transforms and is paved by a 16 km2 channelized flow that erupted from 9 km of en echelon fissures and is larger than historic flows on the East Pacific Rise or on the Gorda and Juan de Fuca Ridges. Starting ∼5 km south of the Pescadero transform, 6.5 km of the Alarcon Rise is characterized by faulted ridges and domes of fractionated lavas ranging from basaltic andesite to rhyolite with up to 77.3 wt % SiO2. These are the first known rhyolites from the submarine global mid‐ocean ridge system. Silicic lavas range from >11.7 ka, to as young as 1.1 ka. A basalt‐to‐basaltic andesite sequence and an andesite‐to‐dacite‐to‐rhyolite sequence are consistent with crystal fractionation but some intermediate basaltic andesite and andesite formed by mixing basalt with dacite or rhyolite. Magmatism occurred along the bounding Tamayo and Pescadero transforms as extensive channelized flows. The flows erupted from ring faults surrounding uplifted sediment hills inferred to overlie sills. The transforms are transtensional to accommodate magma migration from the adjacent Alarcon Rise.
- 1 January 2018
- Published by Elsevier in Chemical Geology
- Vol. 476, 280-291
The trace element and Sr-Nd-Pb isotope geochemistry of Juan Fernandez lavas reveal variable contributions from a high-3He/4He mantle plume
- 1 January 2018
- Published by Elsevier in Chemical Geology
- Vol. 476, 280-291
The trace element and Sr-Nd-Pb isotope geochemistry of Juan Fernandez lavas reveal variable contributions from a high-3He/4He mantle plume
- 1 July 2017
- Published by Elsevier in Science Bulletin
- Vol. 62 (14) , 974-975
An alternative explanation for the Hf-Nd mantle array
- 1 July 2017
- Published by Elsevier in Science Bulletin
- Vol. 62 (14) , 974-975
An alternative explanation for the Hf-Nd mantle array