scholarly journals Volcanic evolution of the submarine super volcano, Tamu Massif of Shatsky Rise: New insights from Formation MicroScanner logging imagery

2015 ◽  
Vol 42 (1) ◽  
pp. 36-43
Author(s):  
Masako Tominaga ◽  
Gerardo Iturrino ◽  
Helen F. Evans
Keyword(s):  
Shatsky Rise ◽  
Volcanic Evolution ◽  
Tamu Massif

scholarly journals Post-Plateau Volcanic Evolution of Shatsky Rise (NW Pacific) – Papanin Ridge and Ojin Rise Seamount Province

2020 ◽  
Author(s):  
Antje Dürkefälden ◽  
Jörg Geldmacher ◽  
Folkmar Hauff ◽  
Dieter Garbe-Schönberg ◽  
Maxim Portnyagin ◽  
...  
Keyword(s):  
Shatsky Rise ◽  
Volcanic Evolution

scholarly journals The age of Earth’s largest volcano: Tamu Massif on Shatsky Rise (northwest Pacific Ocean)

2014 ◽  
Vol 103 (8) ◽  
pp. 2351-2357 ◽  
Author(s):  
Jörg Geldmacher ◽  
Paul van den Bogaard ◽  
Ken Heydolph ◽  
Kaj Hoernle
Keyword(s):  
Pacific Ocean ◽  
Northwest Pacific ◽  
Shatsky Rise ◽  
Northwest Pacific Ocean ◽  
Tamu Massif

scholarly journals Zoned Crystal Records of Transcrustal Magma Transport, Storage and Differentiation: Insights from the Shatsky Rise Oceanic Plateau

2020 ◽  
Vol 61 (8) ◽  
Author(s):  
T D van Gerve ◽  
D A Neave ◽  
R R Almeev ◽  
F Holtz ◽  
O Namur
Keyword(s):  
Magma Ascent ◽  
Crystal Mush ◽  
Magmatic Differentiation ◽  
Shatsky Rise ◽  
Magma Transport ◽  
Powerful Approach ◽  
Magmatic Processes ◽  
Plumbing Systems ◽  
Tamu Massif ◽  
Crystal Residence

Abstract Magmatic processes occurring in the deepest parts of sub-volcanic plumbing systems remain poorly constrained. However, crystal mush fragments incorporated into ascending magmas can provide valuable insights into the processes and conditions of transcrustal magma transport, storage and differentiation. Here we use lava samples drilled from Tamu Massif, Shatsky Rise, to understand the magmatic processes taking place in a region of thickened oceanic crust. We observe correlations between crystal textures and compositional zones in plagioclase that reveal relationships between mechanisms of magmatic differentiation and the crustal depths at which they occurred. When combined with geothermobarometric models, our observations indicate that deep crustal crystal storage took place in high-crystallinity mushes at two discrete levels (∼17 and ∼27 km depth). Diffusive constraints from crystal zoning lengthscales indicate that the lifetime of crystals within the mushes exceeded several thousand years. Magmatic recharge was frequent and produced various dissolution textures in plagioclase. In contrast, shallow crystal storage (∼2·4 km depth) took place in a liquid-dominated domain where crystal residence times were much shorter. Crystal zoning patterns indicate that magmas transporting crystals from the deepest environment to the surface sometimes accumulated additional crystals from mid-crustal storage regions and sometimes did not, highlighting the complexity of magma assembly processes. Temperature contrasts in the lower crust at Shatsky Rise are probably low, owing to extensive magma input and a paucity of hydrothermal cooling at depth. Crystal growth morphologies are consequently relatively simple. Crystallization in thick and thermally mature crusts may therefore lead to less complexity in crystal textures than crystallization in thinner crusts where temperature contrasts are higher. Our observations indicate that combining thermobarometry with studies of crystal textures and crystal compositions is a powerful approach for improving our understanding of magmatic differentiation and magma ascent paths.

scholarly journals Massive basalt flows on the southern flank of Tamu Massif, Shatsky Rise: a reappraisal of ODP Site 1213 basement units

2010 ◽  
Author(s):  
A.A.P. Koppers ◽  
T. Sano ◽  
J.H. Natland ◽  
M. Widdowson ◽  
R. Almeev ◽  
...  
Keyword(s):  
Shatsky Rise ◽  
Tamu Massif ◽  
Southern Flank

scholarly journals Geothermobarometry of basaltic glasses from the Tamu Massif, Shatsky Rise oceanic plateau

2013 ◽  
Vol 14 (10) ◽  
pp. 3908-3928 ◽  
Author(s):  
Anika Husen ◽  
Renat R. Almeev ◽  
François Holtz ◽  
Jürgen Koepke ◽  
Takashi Sano ◽  
...  
Keyword(s):  
Shatsky Rise ◽  
Oceanic Plateau ◽  
Tamu Massif

scholarly journals IODP Expedition 324: Ocean Drilling at Shatsky Rise Gives Clues about Oceanic Plateau Formation

2011 ◽  
Vol 12 ◽  
pp. 24-31 ◽  
Author(s):  
W. W. Sager ◽  
T. Sano ◽  
J. Geldmacher ◽  
Keyword(s):  
Ocean Drilling Program ◽  
Ontong Java Plateau ◽  
Shatsky Rise ◽  
Oceanic Plateau ◽  
Ocean Drilling ◽  
Integrated Ocean Drilling Program ◽  
High Fluid ◽  
Formation And Evolution ◽  
Effusion Rates ◽  
Tamu Massif

Integrated Ocean Drilling Program (IODP) Expedition 324 cored Shatsky Rise at five sites (U1346–U1350) to study processes of oceanic plateau formation and evolution. Site penetrations ranged from 191.8 m to 324.1 m with coring of 52.6 m to 172.7 m into igneous basement at four of the sites. Average recovery in basement was 38.7%–67.4%. Cored igneous sections consist mainly of variably evolved tholeiitic basalts emplaced as pillows or massive flows. Massive flows are thickest and make up the largest percentage of section on the largest and oldest volcano, late Jurassic age Tamu Massif; thus, it may have formed at high effusion rates. Such massive flows are characteristic of flood basalts, and similar flows were cored at Ontong Java Plateau. Indeed, the similarity of igneous sections at Site U1347 with that cored on Ontong Java Plateau implies similar volcanic styles for these two plateaus. On younger, smaller Shatsky Rise volcanoes, pillow flows are common and massive flows thinner and fewer, which might mean volcanism waned with time. Cored sediments from summit sites contain fossils and structures implying shallow water depths or emergence at the time of eruption and normal subsidence since. Summit sites also show pervasive alteration that could be due to high fluid fluxes. A thick section of volcaniclastics cored on Tamu Massif suggests that shallow, explosive submarine volcanism played a significant role in the geologic development of the plateau summit. Expedition 324 results imply that Shatsky Rise began with massive eruptions forming a huge volcano and that subsequent eruptions waned in intensity, forming volcanoes that are large, but which did not erupt with unusually high effusion rates. Similarities of cored sections on Tamu Massif with those of Ontong Java Plateau indicate that these oceanic plateaus formed in similar fashion. <br><br> doi:<a href="http://dx.doi.org/10.2204/iodp.sd.12.03.2011" target="_blank">10.2204/iodp.sd.12.03.2011</a>

Towards a stable astronomical time scale for the Paleocene: Aligning Shatsky Rise with the Zumaia – Walvis Ridge ODP Site 1262 composite

2015 ◽  
Vol 48 (1) ◽  
pp. 91-110 ◽  
Author(s):  
Frederik J. Hilgen ◽  
Hemmo A. Abels ◽  
Klaudia F. Kuiper ◽  
Lucas J. Lourens ◽  
Mariëtte Wolthers
Keyword(s):  
Time Scale ◽  
Shatsky Rise ◽  
Walvis Ridge ◽  
Astronomical Time
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