Late-Stage Fall Deposits of the Bishop Tuff: Melt Inclusion And
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Geologic Map of the Long Valley Caldera, Mono-Inyo Craters
DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP 1-1933 US. GEOLOGICAL SURVEY GEOLOGIC MAP OF LONG VALLEY CALDERA, MONO-INYO CRATERS VOLCANIC CHAIN, AND VICINITY, EASTERN CALIFORNIA By Roy A. Bailey GEOLOGIC SETTING VOLCANISM Long Valley caldera and the Mono-Inyo Craters Long Valley caldera volcanic chain compose a late Tertiary to Quaternary Volcanism in the Long Valley area (Bailey and others, volcanic complex on the west edge of the Basin and 1976; Bailey, 1982b) began about 3.6 Ma with Range Province at the base of the Sierra Nevada frontal widespread eruption of trachybasaltic-trachyandesitic fault escarpment. The caldera, an east-west-elongate, lavas on a moderately well dissected upland surface oval depression 17 by 32 km, is located just northwest (Huber, 1981).Erosional remnants of these mafic lavas of the northern end of the Owens Valley rift and forms are scattered over a 4,000-km2 area extending from the a reentrant or offset in the Sierran escarpment, Adobe Hills (5-10 km notheast of the map area), commonly referred to as the "Mammoth embayment.'? around the periphery of Long Valley caldera, and The Mono-Inyo Craters volcanic chain forms a north- southwestward into the High Sierra. Although these trending zone of volcanic vents extending 45 km from lavas never formed a continuous cover over this region, the west moat of the caldera to Mono Lake. The their wide distribution suggests an extensive mantle prevolcanic basement in the area is mainly Mesozoic source for these initial mafic eruptions. Between 3.0 granitic rock of the Sierra Nevada batholith and and 2.5 Ma quartz-latite domes and flows erupted near Paleozoic metasedimentary and Mesozoic metavolcanic the north and northwest rims of the present caldera, at rocks of the Mount Morrisen, Gull Lake, and Ritter and near Bald Mountain and on San Joaquin Ridge Range roof pendants (map A). -
Bursting the Bubble of Melt Inclusions†K
American Mineralogist, Volume 100, pages 672–673, 2015 HIGHLIGHTS AND BREAKTHROUGHS Bursting the bubble of melt inclusions†k JACOB B. LOWENSTERN1,* 1U.S. Geological Survey, Volcano Science Center, Menlo Park, California 94025, U.S.A. Abstract: Most silicate melt inclusions (MI) con- crystal and trapped liquid create conditions that strongly favor tain bubbles, whose significance has been alternately creation of a low-density phase. In studies of FI, the bubbles are calculated, pondered, and ignored, but rarely if ever studied intensively (Samson et al. 2003). Experimental heating directly explored. Moore et al. (2015) analyze the and homogenization provide insight into the temperature of en- bubbles, as well as their host glasses, and conclude trapment and the conditions of formation. Raman spectroscopy and other techniques can provide quantitative information on that they often hold the preponderance of CO2 in gas species within bubbles. the MI. Their findings entreat future researchers Surprisingly, little has been done to analyze the bubbles within to account for the presence of bubbles in MI when MI—perhaps partly because of interference from the surround- calculating volatile budgets, saturation pressures, ing glass greatly complicates spectroscopic and other analytical and eruptive flux. Keywords: Melt inclusion, glass methods. Many authors recognize that bubbles can contain a inclusion, bubble, volatile, CO2 significant percentage of the volatiles in an inclusion, particularly for those with low solubility in the melt such as CO2 (Anderson On page 806, of this issue, Lowell Moore and colleagues and Brown 1993). But there is little consensus on how to account contribute an exciting, scholarly, and admirably thorough trea- for the presence of bubbles. -
Understanding a Volcano Through a Droplet: a Melt Inclusion Approach
Journal of Geochemical Exploration 171 (2016) 4–19 Contents lists available at ScienceDirect Journal of Geochemical Exploration journal homepage: www.elsevier.com/locate/jgeoexp Understanding a volcano through a droplet: A melt inclusion approach C. Cannatelli a,b,⁎,A.L.Dohertya, R. Esposito c,A.Limaa, B. De Vivo a a Dipartimento di Scienze della Terra, dell'Ambiente e delle Risorse, Università di Napoli Federico II, Italy b Department of Geology and Andean Geothermal Centre of Excellence (CEGA), Universidad de Chile, Plaza Ercilla 803, Santiago, Chile c Earth, Planetary and Space Sciences, UC Los Angeles, CA, USA article info abstract Article history: This review paper is intended to be a guideline to novices on how to conduct research on silicate melt inclusions Received 29 January 2015 in volcanic environments, which analytical techniques are more suitable to gather the desired data and the major Revised 9 July 2015 pitfalls scientist may encounter. Silicate melt inclusions (SMIs) are small quantities of silicate melt that are Accepted 3 October 2015 trapped in minerals during their growth or crystallization. They contain liquids formed in equilibrium with Available online 23 October 2015 their host minerals and therefore record the liquid line of descent of magmatic systems. Upon trapping, SMIs be- come ideally closed to the surrounding environment, and behave as time capsules, giving important information Keywords: Melt inclusions about processes that originated magmas and the nature of their mantle source. A melt inclusions investigation -
Compositional Zoning of the Bishop Tuff
JOURNAL OF PETROLOGY VOLUME 48 NUMBER 5 PAGES 951^999 2007 doi:10.1093/petrology/egm007 Compositional Zoning of the Bishop Tuff WES HILDRETH1* AND COLIN J. N. WILSON2 1US GEOLOGICAL SURVEY, MS-910, MENLO PARK, CA 94025, USA 2SCHOOL OF GEOGRAPHY, GEOLOGY AND ENVIRONMENTAL SCIENCE, UNIVERSITY OF AUCKLAND, PB 92019 AUCKLAND MAIL CENTRE, AUCKLAND 1142, NEW ZEALAND Downloaded from https://academic.oup.com/petrology/article/48/5/951/1472295 by guest on 29 September 2021 RECEIVED JANUARY 7, 2006; ACCEPTED FEBRUARY 13, 2007 ADVANCE ACCESS PUBLICATION MARCH 29, 2007 Compositional data for 4400 pumice clasts, organized according to and the roofward decline in liquidus temperature of the zoned melt, eruptive sequence, crystal content, and texture, provide new perspec- prevented significant crystallization against the roof, consistent with tives on eruption and pre-eruptive evolution of the4600 km3 of zoned dominance of crystal-poor magma early in the eruption and lack of rhyolitic magma ejected as the BishopTuff during formation of Long any roof-rind fragments among the Bishop ejecta, before or after onset Valley caldera. Proportions and compositions of different pumice of caldera collapse. A model of secular incremental zoning is types are given for each ignimbrite package and for the intercalated advanced wherein numerous batches of crystal-poor melt were plinian pumice-fall layers that erupted synchronously. Although released from a mush zone (many kilometers thick) that floored the withdrawal of the zoned magma was less systematic than previously accumulating rhyolitic melt-rich body. Each batch rose to its own realized, the overall sequence displays trends toward greater propor- appropriate level in the melt-buoyancy gradient, which was self- tions of less evolved pumice, more crystals (0Á5^24 wt %), and sustaining against wholesale convective re-homogenization, while higher FeTi-oxide temperatures (714^8188C). -
Bailey-1976.Pdf
VOL. 81, NO. 5 JOURNAL OF GEOPHYSICAL RESEARCH FEBRUARY 10, 1976 Volcanism, Structure,and Geochronologyof Long Valley Caldera, Mono County, California RoY A. BAILEY U.S. GeologicalSurvey, Reston, Virginia 22092 G. BRENT DALRYMPLE AND MARVIN A. LANPHERE U.S. GeologicalSurvey, Menlo Park, California 94025 Long Valley caldera, a 17- by 32-km elliptical depressionon the east front of the Sierra Nevada, formed 0.7 m.y. ago during eruption of the Bishoptuff. Subsequentintracaldera volcanism included eruption of (1) aphyric rhyolite 0.68-0.64 m.y. ago during resurgentdoming of the caldera floor, (2) porphyritic hornblende-biotiterhyolite from centersperipheral to the resurgentdome at 0.5, 0.3, and 0.1 m.y. ago, and (3) porphyritic hornblende-biotiterhyodacite from outer ring fractures0.2 m.y. ago to 50,000 yr ago, a sequencethat apparently records progressivecrystallization of a subjacentchemically zoned magma chamber. Holocene rhyolitic and phreatic eruptions suggestthat residual magma was present in the chamber as recentlyas 450 yr ago. Intracaldera hydrothermalactivity beganat least0.3 m.y. ago and was widespreadin the caldera moat; it has sincedeclined due to self-sealingof near-surfacecaldera sediments by zeolitization, argillization, and silicificationand has becomelocalized on recentlyreactivated north- west-trendingSierra Nevada frontal faults that tap hot water at depth. INTRODUCTION concentrates were treated with a dilute HF solution to remove small bits of attached glassand fragments of other mineral In the westernUnited States,only three calderasare known grains. Obsidian used for dating was totally unhydrated and to be large enoughand young enoughto possiblystill contain not devitrified. Small blocks sawed from many of the hand residual magma in their chambers:the Vailes caldera (•1.1 specimenswere used for dating. -
Melt Inclusions in Chassignites: a Connection Between Martian Meteorites and in Situ Evolved Rocks at Gale Crater
51st Lunar and Planetary Science Conference (2020) 2342.pdf MELT INCLUSIONS IN CHASSIGNITES: A CONNECTION BETWEEN MARTIAN METEORITES AND IN SITU EVOLVED ROCKS AT GALE CRATER. P. Wu1, E. Gazel1, and A. Udry2 1Department of Earth and Space Sciences, Cornell University ([email protected], [email protected]); 2Department of Geoscience, UNLV ([email protected]). Introduction: UnderstandinG the compositional Methods: We used six parental magma composi- diversity of igneous rocks is the key to investigate tions calculated from NWA 2737 melt inclusions by conditions of meltinG and sources within the martian He et al. [3] as startinG compositions for the modeling. interior. Meteorites, our only martian samples, can be He et al. [3] analyzed nine melt inclusions in a sinGle analyzed with the most advanced laboratory analytical thin section of NWA 2737. Measured phase composi- techniques and thus has dominated our knowledge of tions and phase abundances are used to calculate the martian iGneous chemistry. Most martian meteorites bulk composition of inclusions [3]. are classified into three major cateGories, sherGottite, AmonG the nine melt inclusions, olivine, low-Ca nakhlite, and chassignite (SNC). As a type of olivine pyroxene, kaersutitic amphibole, augite, apatite, chro- cumulates with abundant melt inclusions, chassiGnites mite, sulfide, alkali-rich Glass, and some Ti-biotite can provide key information on the compositions of were identified [3]. Since MI-4 and MI-5 are likely parental magmas, volatile budgets, and early crystalli- off-center cuts and MI-6 includes some biotite and zation processes. Chassigny, Northwest Africa (NWA) may represent composite Grains, we excluded MI-4, 2737 and Northwest Africa (NWA) 8694 are the only MI-5, and MI-6 from our study. -
High Pre-Eruptive Water Contents Preserved in Lunar Melt Inclusions
REPORTS and the catalyst tolerates useful substrate func- 10. P. P. Fu, R. G. Harvey, Chem. Rev. 78, 317 (1978). 25. L. H. Heitman et al., J. Med. Chem. 52, 2036 tional groups, including aromatic and heteroatom 11. T. Moriuchi, K. Kikushima, T. Kajikawa, T. Hirao, (2009). Tetrahedron Lett. 50, 7385 (2009). 26. R. A. Sheldon, J. M. Sobczak, J. Mol. Catal. 68, substituents. With the development of improved 12.C.S.Yi,D.W.Lee,Organometallics 28, 947 1 (1991). methods for safe and scalable aerobic oxidation (2009). 27. J. E. Bercaw, N. Hazari, J. A. Labinger, J. Org. Chem. 73, reactions (30), dehydrogenation methods of this 13.P.F.Schuda,W.A.Price,J. Org. Chem. 52, 1972 8654 (2008). type could have an important impact on laboratory- (1987). 28. J. E. Bercaw, N. Hazari, J. A. Labinger, P. F. Oblad, Angew. Chem. Int. Ed. 47, 9941 (2008). and industrial-scale chemical synthesis. 14. J. Muzart, J. P. Pete, J. Mol. Catal. 15, 373 (1982). 15. T. T. Wenzel, J. Chem. Soc. Chem. Commun. 1989, 932 29. G. E. Dobereiner, R. H. Crabtree, Chem. Rev. 110,681 (1989). (2010). 30. X. Ye, M. D. Johnson, T. Diao, M. H. Yates, S. S. Stahl, References and Notes 16. J. Muzart, Eur. J. Org. Chem. 2010, 3779 (2010). Green Chem. 12, 1180 (2010). 1. J. H. P. Tyman, Synthetic and Natural Phenols (Elsevier, Acknowledgments: We are grateful to the NIH New York, 1996). 17. D. R. Buckle, in Encyclopedia of Reagents for Organic Synthesis, D. Crich, Ed. (Wiley, New York, 2010). -
A Melt Inclusion Study on Volatile Abundances in the Lunar Mantle
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 249 (2019) 17–41 www.elsevier.com/locate/gca A melt inclusion study on volatile abundances in the lunar mantle Peng Ni (倪鹏) a,⇑, Youxue Zhang (张有学) a, Sha Chen (陈沙) a, Joel Gagnon b a Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109-1005, USA b Department of Earth and Environmental Sciences, University of Windsor, Windsor, Ontario N9B 3P4, Canada Received 22 December 2017; accepted in revised form 23 December 2018; Available online 08 January 2019 Abstract Earth’s Moon was thought to be highly depleted in volatiles due to its formation by a giant impact. Over the last decade, however, evidence has been found in apatites, lunar volcanic glass beads, nominally anhydrous minerals and olivine-hosted melt inclusions, to support a relatively ‘‘wet” Moon. In particular, based on H2O/Ce, F/Nd, and S/Dy ratios, recent melt inclusion (MI) work estimated volatile (H2O, F, and S) abundances in lunar rocks to be similar to or slightly lower than the terrestrial depleted mantle. Uncertainties still occur, however, in whether the limited numbers of lunar samples studied are representative of the primitive lunar mantle, and whether the high H2O/Ce ratio for pyroclastic sample 74220 is due to local heterogeneity. In this paper, we report major element, trace element, volatile, and transition metal data in MIs for 5 mare basalt samples (10020, 12040, 15016, 15647 and 74235) and a pyroclastic deposit (74220). With our new lunar MI data, H2O/Ce ratios are still found to vary significantly among different lunar samples, from 50 for 74220, to 9 for 10020, 3 for 74235, 1.7 to 0.9 for 12008, 15016, and 15647, and 0.5 for 12040. -
Mineral-Hosted Melt Inclusions How Do We Read the Stories They Have to Tell?
Mineral-Hosted Melt Inclusions How do we read the stories they have to tell? Woods Hole Oceanographic Institution Woods Hole, MA, USA August 10-12, 2018 Thank you to our sponsors. Mineral-Hosted Melt Inclusions, Woods Hole, MA, USA, 10-12 August 2018 Welcome to Mineral-Hosted Melt Inclusions: How do we read the stories they have to tell? Thank you to our sponsors. The study of mineral-hosted melt inclusions traces Over the next two days, fifteen invited speakers its origins all the way back to the mid-nineteenth will discuss the state of our knowledge with respect century. In 1857, Henry Clifton Sorby recognized to mineral-hosted melt inclusions. Topics range that the presence of “glass cavities” demonstrates from the origin and fidelity of mineral-hosted that the host crystals had a magmatic – rather than melt inclusions to the application of state-of-the- an aqueous – origin and used this observation to art micro-analytical techniques to quantify their argue that granite is the product of fusion rather compositions. Each talk will be followed by a than precipitation from a fluid. Today, these small discussion session intended to promote interaction pockets of silicate melt entrapped within growing among all the attendees. One objective is to mineral grains are used to study everything from develop guidelines for publication of data from melt mantle heterogeneity to pre-eruptive magmatic inclusion studies to be summarized in a collegial volatiles and the oxidation state of the upper mantle. manuscript that the organizers will submit for The information recorded in melt inclusions is publication shortly after the workshop. -
Development of a Groundwater Flow Model for the Bishop/Laws Area
DEVELOPMENT OF A GROUNDWATER FLOW MODEL FOR THE BISHOP/LAWS AREA FINAL REPORT FOR LOCAL GROUNDWATER ASSISTANCE GRANT AGREEMENT NO. 4600004129 Robert Harrington, PhD, R.G. INYO COUNTY WATER DEPARTMENT APRIL, 2007 TABLE OF CONTENTS EXECUTIVE SUMMARY ………………………………………. 3 INTRODUCTION ………………………………………………. 5 CONCEPTUAL MODEL ………………………………………… 8 SIMULATION MODEL …………………………………………. 5 PREDICTIVE SIMULATIONS …………………………………. 23 SUMMARY AND CONCLUSIONS ……………………………. 26 REFERENCES …………………………………………………… 28 APPENDIX 1 ……………………………………………………. 51 APPENDIX 2 ……………………………………………………. 54 LIST OF FIGURES Figure 1. Study area location……………………………………………… 30 Figure 2. Geology…………………………………………………………. 31 Figure 3. Hydraulic conductivity distribution…………………………….. 32 Figure 4. Aquifer test locations…………………………………………… 33 Figure 5. Well locations…………………………………………………... 34 Figure 6. Layer 1 hydraulic conductivity zones…………………………... 35 Figure 7. Layer 2 hydraulic conductivity zones………………………….. 36 Figure 8. Layer 3 hydraulic conductivity zones…………………………. 37 Figure 9. Layer 4 hydraulic conductivity zones…………………………. 38 Figure 10. Layer 5 hydraulic conductivity zones………………………… 39 Figure 11. Quaternary faults and horizontal flow barriers………………. 40 Figure 12. Recharge zones……………………………………………….. 41 Figure 13. Evapotranspiration zones……………………………………… 42 Figure 14. Boundary conditions………………………………………….. 43 Figure 15. Observed vs. residuals………………………………………… 44 Figure 16. Distribution of residuals………………………………………. 45 Figure 17. Spatial distribution of residuals………………………………. 46 Figure 18. Drawdown -
Geologists Reveal Secrets Behind Supervolcano Eruption 5 March 2007
Geologists Reveal Secrets Behind Supervolcano Eruption 5 March 2007 author of the paper. The 20-mile-long Long Valley Caldera was created when the supervolcano erupted. The geologists focused their efforts on Bishop Tuff, an expanse of rock that was built up as the hot ash cooled following the eruption. The researchers studied the distribution of titanium in quartz crystals in samples taken from Bishop Tuff. A team from Rensselaer previously discovered that trace levels of titanium can be analyzed to determine the temperature at which the quartz crystallized. By monitoring titanium, Wark and his colleagues confirmed that the outer rims of the A piece of supervolcano and extracted quartz crystals quartz had formed at a much hotter temperature analyzed for titanium. Credit: Rensselaer Polytechnic than the crystal interiors. The researchers Institute/David Wark concluded that after the interiors of the quartz crystals had grown, the magma system was “recharged” with an injection of fresh, hot melt. This caused the quartz to partly dissolve, before Researchers at Rensselaer Polytechnic Institute starting to crystallize again at a much higher have discovered what likely triggered the eruption temperature. of a “supervolcano” that coated much of the western half of the United States with ash fallout Analyses of titanium also revealed that the high- 760,000 years ago. temperature rim-growth must have taken place within only 100 years of the massive volcano’s Using a new technique developed at Rensselaer, eruption. This suggests that the magma recharge the team determined that there was a massive so affected the physical properties of the magma injection of hot magma underneath the surface of chamber that it caused the supervolcano to erupt what is now the Long Valley Caldera in California and blanket thousands of square miles with searing some time within 100 years of the gigantic ash. -
New Perspectives on the Bishop Tuff Magma Chamber from Micro
Micro-analytical perspectives on the Bishop Tuff and its magma chamber. Item type Article Authors Chamberlain, Katy J.; Wilson, Colin J. N.; Wallace, Paul J.; Millet, Marli Bryant Citation Chamberlain, K. J. et al (2015) 'Micro-analytical Perspectives on the Bishop Tuff and its Magma Chamber', Journal of Petrology, 56 (3):605. DOI 10.1093/petrology/egv012 Publisher Oxford Academic Journal Journal of Petrology Rights Archived with thanks to Journal of Petrology Downloaded 13-Jan-2019 02:47:32 Link to item http://hdl.handle.net/10545/622294 1 Micro-analytical Perspectives on the Bishop Tuff and its Magma 2 Chamber 3 4 5 6 7 8 K. J. CHAMBERLAIN1,2*, C. J. N. WILSON1, P. J. WALLACE3 AND M. -A. MILLET 1,2 9 10 11 12 13 1SCHOOL OF GEOGRAPHY, ENVIRONMENT AND EARTH SCIENCES, VICTORIA UNIVERSITY, PO BOX 600, 14 WELLINGTON 6140, NEW ZEALAND 15 2 DEPARTMENT OF EARTH SCIENCES, UNIVERSITY OF DURHAM, DURHAM DH1 3LE, UK 16 3 DEPARTMENT OF GEOLOGICAL SCIENCES, UNIVERSITY OF OREGON, EUGENE, OREGON 97403-1272, USA 17 18 19 This is a pre-copyedited, author-produced version of an article accepted for publication in 20 Journal of Petrology following peer review. The version of record is available online at: 21 https://doi.org/10.1093/petrology/egv012 22 23 24 25 26 27 Manuscript for: Journal of Petrology 28 Running title: Micro-analytical perspectives on the Bishop Tuff 29 30 Keywords: Bishop Tuff, supereruption, magma chamber, compositional zoning, magma 31 mixing. 32 33 Final accepted version 34 35 *Corresponding author. Phone (+44) 191 334 2300, Fax (+44) 191 334 2301 36 Email addresses: [email protected]; [email protected]; 37 [email protected]; [email protected] 38 1 Sensitivity: Internal 39 ABSTRACT 40 New in-situ major and trace element analytical data from crystals (sanidine, plagioclase, 41 biotite, orthopyroxene, clinopyroxene) and matrix glasses are presented from juvenile 42 materials representing the full Bishop Tuff sequence from the earliest fall unit (F1) to the 43 latest ignimbrite package (Ig2Nc).