GLORIA

GEOMAR Library Ocean Research Information Access

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
Filter
  • Osmium isotopes  (2)
  • 113-690C; 74-525A; 86-577A; AGE; Correction; Deep Sea Drilling Project; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP; DSDP/ODP/IODP sample designation; Event label; Glomar Challenger; Inductively coupled plasma - mass spectrometry (ICP-MS); Joides Resolution; Leg113; Leg74; Leg86; North Pacific; Ocean Drilling Program; ODP; Osmium; Osmium-187/Osmium-188, error; Osmium-187/Osmium-188 ratio; Rhenium; Rhenium-187/Osmium-188 ratio; Sample code/label; South Atlantic/CREST; South Atlantic Ocean  (1)
Document type
Keywords
Years
  • 1
    Publication Date: 2024-01-09
    Keywords: 113-690C; 74-525A; 86-577A; AGE; Correction; Deep Sea Drilling Project; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP; DSDP/ODP/IODP sample designation; Event label; Glomar Challenger; Inductively coupled plasma - mass spectrometry (ICP-MS); Joides Resolution; Leg113; Leg74; Leg86; North Pacific; Ocean Drilling Program; ODP; Osmium; Osmium-187/Osmium-188, error; Osmium-187/Osmium-188 ratio; Rhenium; Rhenium-187/Osmium-188 ratio; Sample code/label; South Atlantic/CREST; South Atlantic Ocean
    Type: Dataset
    Format: text/tab-separated-values, 108 data points
    Location Call Number Limitation Availability
    BibTip Others were also interested in ...
  • 2
    Publication Date: 2022-05-25
    Description: Author Posting. © The Author(s), 2015. This is the author's version of the work. It is posted here for personal use, not for redistribution. The definitive version was published in Earth and Planetary Science Letters 437 (2016): 76-88, doi:10.1016/j.epsl.2015.12.040.
    Description: High concentrations of extraterrestrial iridium have been reported in terminal Sturtian and Marinoan glacial marine sediments and are used to argue for long (likely 3-12 Myr) durations of these Cryogenian glaciations. Reanalysis of the Marinoan sedimentary rocks used in the original study, supplemented by sedimentary rocks from additional terminal Marinoan sections, however, does not confirm the initial report. New platinum group element concentrations, and 187Os/188Os and 3He/4He signatures are consistent with crustal origin and minimal extraterrestrial contributions. The discrepancy is likely caused by different sample masses used in the two studies, with this study being based on much larger samples that better capture the stochastic distribution of extraterrestrial particles in marine sediments. Strong enrichment of redox-sensitive elements, particularly rhenium, up-section in the basal postglacial cap carbonates, may indicate a return to more fully oxygenated seawater in the aftermath of the Marinoan snowball earth. Sections dominated by hydrogenous osmium indicate increasing submarine hydrothermal sources and/or continental inputs that are increasingly dominated by young mantle-derived rocks after deglaciation. Sedimentation rate estimates for the basal cap carbonates yield surprisingly slow rates of a few centimeters per thousand years. This study highlights the importance of using sedimentary rock samples that represent sufficiently large area-time products to properly sample extraterrestrial particles representatively, and demonstrates the value of using multiple tracers of extraterrestrial matter.
    Description: We are grateful for support from a 2008 WHOI Summer Student Fellowship for CAW. BPE acknowledges financial support from WHOI’s Ocean and Climate Change Institute (CH11320) and U.S. NSF SGER grant EAR-0821878. Fieldwork in NW Canada was licensed by the Aurora Research Institute and supported by a grant to PFH from the Astrobiology Institute of the US National Aeronautics and Space Administration (NASA). Fieldwork in NW Canada and Namibia was supported by grants EAR-9905495 and EAR-0417422 (to PFH) from the US NSF. We thank Jon Husson (Harvard University) and Ricardo Trindade (University of São Paulo, Brazil) for excellent support during fieldwork in Namibia in August of 2005.
    Keywords: Snowball earth ; Osmium isotopes ; Iridium ; Helium isotopes ; Extraterrestrial matter ; Cap carbonate
    Repository Name: Woods Hole Open Access Server
    Type: Preprint
    Location Call Number Limitation Availability
    BibTip Others were also interested in ...
  • 3
    Publication Date: 2022-05-26
    Description: Author Posting. © American Geophysical Union, 2017. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geochemistry, Geophysics, Geosystems 18 (2017): 3946–3963, doi:10.1002/2017GC007071.
    Description: The sources of terrestrial material delivered to the California margin over the past 7 Myr were assessed using 187Os/188Os, Nd, and Pb isotopes in hydrogenetic ferromanganese crusts from three seamounts along the central and southern California margin. From 6.8 to 4.5 (±0.5) Ma, all three isotope systems show more radiogenic values at Davidson Seamount, located near the base of the Monterey Canyon System, than in Fe-Mn crusts from the more remote Taney and Hoss Seamounts. At the Taney Seamounts, approximately 225 km farther offshore from Davidson Seamount, 187Os/188Os values, but not Pb and Nd isotope ratios, also deviate from the Cenozoic seawater curve toward more radiogenic values from 6.8 to 4.5 (±0.5) Ma. However, none of the isotope systems in Fe-Mn crusts deviate from seawater at Hoss Seamount located approximately 450 km to the south. The regional gradients in isotope ratios indicate that substantial input of dissolved and particulate terrestrial material into the Monterey Canyon System is responsible for the local deviations in the seawater Nd, Pb, and Os isotope compositions from 6.8 to 4.5 (±0.5) Ma. The isotope ratios recorded in Fe-Mn crusts are consistent with a southern Sierra Nevada or western Basin and Range provenance of the terrestrial material which was delivered by rivers to the canyon. The exhumation of the modern Monterey Canyon must have begun between 10 and 6.8 ± 0.5 Ma, as indicated by our data, the age of incised strata, and paleo-location of the Monterey Canyon relative to the paleo-coastline.
    Description: Funding was provided by the United States Geological Survey Pacific Coastal and Marine Science Center Marine Minerals Group, the University of California Santa Cruz Scholarship for Re-Entry Women in Science, and the UCSC Earth and Planetary Science Department Waters Award.
    Description: 2018-05-15
    Keywords: Ferromanganese crusts ; Osmium isotopes ; Neodymium isotopes ; Lead isotopes ; Monterey Canyon System ; Seawater
    Repository Name: Woods Hole Open Access Server
    Type: Article
    Location Call Number Limitation Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...