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Paleomagnetism of Four Late Cretaceous Plutons North Cascades, Washington William J

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Paleomagnetism of Four Late Cretaceous Plutons North Cascades, Washington William J Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship 1984 Paleomagnetism of Four Late Cretaceous Plutons North Cascades, Washington William J. (William James) Harrison Western Washington University Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Harrison, William J. (William James), "Paleomagnetism of Four Late Cretaceous Plutons North Cascades, Washington" (1984). WWU Graduate School Collection. 830. https://cedar.wwu.edu/wwuet/830 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. PALEOMAGNETISM OF FOUR LATE CRETACEOUS PLUTONS NORTH CASCADES, WASHINGTON A Thesis Presented to The Faculty of Western Washington University In Partial Fulfillment Of the Requirements for the Degree Master of Science by William J. Harrison PALEOMAGNETISM OF FOUR LATE CRETACEOUS PLUTONS NORTH CASCADES, WASHINGTON by wmiarn J. Harrison Accepted in Partial Completion Of the Requirements for the Degree Master of Science Dean of Graduate School ADVISORY COMMITTEE MASTER'S THESIS In presenting this thesis in partial fulfillment of the requirements for a master"s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files. I acknowledge that I retain ownership rights to the copyright of this work, including but not limited to the right to use all or part of this work in future works, such as articles or books. Library users are granted permission fot^rndividuaf, researc+i an<J non-commereial- reproduction of this work for educational purposes only. Any further digital posting of this document requires specific permission from the author. Any copying or publication of this thesis for commercial purposes, or for financial gain, is not allowed without my written oermission. Name; Signature: Date: ABSTRACT Paleomagnetic directions of samples from the Ten Peak and Sulphur Mtn. plutons, Hidden Lake stock, and Oval Peak batholith in the North Cascades reveal multi-component magnetization and instability. In the Hidden Lake stock and Ten Peak pluton, a strong viscous overprint parallels the present day field. The Sulphur Mountain pluton shows complete magnetic instability; making it impossible to compute a meaningful mean direction. The rocks of the Oval Peak batholith are believed to have been magnetically reset during the Eocene, although the observed declination of 167° and inclination of -67° is significantly different from the expected Eocene direction. The mean direction for the Oval Peak batholith is very similar to directions obtained by Strickler (1982) for the Black Peak batholith, and by Stauss (1982) for dikes in the Corbaley Canyon area. These three units with similar paleomagnetic discordance are found within a panel of rock bound on the east by the Ross Lake fault zone and on the west by the Entiat fault. The rock of the Corbaley Canyon area is Eocene, while the Black Peak batholith has been dated using K/Ar methods at 88.4 Ma and 103 Ma (hornblende), and 73 Ma (biotite). It seems likely that the magnetization of the Black Peak batholith was thermally reset during the Eocene, when it was intruded by the Golden Horn batholith. The inclination for the observed direction from the three units is similar to that expected for the Eocene, but the declination is discordant by approximately 170°. Acquisition of both normal and reverse aberrant directions during anomalous states of the magnetic field is improbable. Bias by an uncleaned overprint might explain the imperfection of antiparallelism, but cannot account for i discordance of both normal and reverse magnetizations. Models involving large scale clockwise rotation or tilt down to the northwest could account for the observed discordance. However, there is no geologic evidence to support either model. A better explanation may be that relatively small blocks have individually rotated clockwise or have undergone large tilts down to the northwest, but again, geologic evidence for such displacement has yet to be recognized. Petrology and magnetic characteristics of rocks from this study were compared to those of magnetically stable intrusive rocks of the Mt. Stuart and Chilliwack batholiths and Fawn Peak stock. Comparison of natural remanent magnetization (NRM) with saturation isothermal remanent magnetization (IRM) for magnetically stable and unstable samples indicates that the magnetization of the unstable samples from this study resides in multi-domain magnetic grains, whereas the magnetically stable samples show single-domain grain magnetic behavior. Tiny grains of magnetite are seen in the plagioclase of the magnetically stable rocks whereas none appear in the magnetically unstable rocks. These tiny magnetite grains may be responsible for magnetic stability in the stable rocks. Lack of magnetite in the plagioclase of the unstable rocks may explain why they are magnetically unstable. Initial magmatic compositions, cooling conditions, or subsequent alteration of plagioclase may be considered as possibilities explaining the lack of magnetite. Petrographic studies show that the magnetically unstable rocks of this study are more altered (i.e., sericitization of plagioclase) and strained (recognized by undulatory extinction and recrystallized quartz) than the magnetically stable rocks from the Mt. Stuart and Chilliwack batholiths and Fawn Peak stock. Magnetically unstable rocks of this study show a persistent VRM overprint stable to approximately lOOoe and parallel to the present day field. Stott and Stacey (I960) have shown that stress may aid a rock in acquiring a VRM. It is not known when these rocks experienced deformation in their history, but, as the field direction has changed little since the Mid-Tertiary, it appears a possibility that stress may have aided in the acquisition of a VRM overprint since that time. iii ACKNOWLEDGEMENTS I would like to thank Myrl Beck, Russ Burmester, and Dave Engebretson for their help and guidance over the course of this project. Thanks to Jonteck Wodzicki, Jim Sevigny, and Jeff Jones who assisted me with the petrology. Chuck Schwarz, Paul Furlong, John Karachewski, Myrl Beck, Dave Strickler, and Kurt Schmierer assisted me in the field and their efforts are greatfully acknowledged. Special thanks to my mother and father, Mary Ellen and Johnny, who've offered unending patience and support in all my endeavors. I would like to extend special thanks to Laurey Cook, Patty Combs, Jeff Jones, Jim Sevigny and Kate Ashworth a group of friends who helped keep me entertained and in the proper frame of mind over the last few years. The research for this project was funded in part by National Science Foundation grant EAR-8106823. iv TABLE OF CONTENTS Page ABSTRACT i ACKNOWLEDGEMENTS iv LIST OF FIGURES vii LIST OF TABLES AND APPENDICES ix INTRODUCTION 1 Regional Geologic Setting 7 Geology of Sampled Units 9 Hidden Lake Stock 9 Oval Peak Pluton H Ten Peak Pluton 13 Sulphur Mtn. Pluton 14 PALEOMAGNETISM 18 Paleomagnetic Methods 18 Sampling 19 Sample and Site Stability; Criteria of Reliability 20 Magnetic and Thermal Cleaning 20 Alternating Field Demagnetization 21 Thermal Demagnetization 22 Sample Stability 23 Site Stability 27 PALEOMAGNETIC RESULTS 28 Hidden Lake Stock 28 Analysis of Results 31 Ten Peak Pluton 31 Analysis of Results 38 Sulphur Mtn. Pluton 40 Oval Peak Batholith 44 Analysis of Results 81 Interpretation 84 DISCUSSION OF STABLE AND UNSTABLE MAGNETIC BEHAVIOR 69 Magnetic Domains and Their Relationship to Magnetic Stability 69 Determination of Effective Domain Size 73 V Petrography Study 74 Petrology of Unstable Sites 77 Petrology of Stable Sites 78 Summary of Petrographic Observations 79 SUMMARY 81 REFERENCES CITED 84 APPENDIX 1 92 APPENDIX 2 93 APPENDIX 3 183 LIST OF FIGURES •Figure 1 Generalized geologic map of the North Cascades. 3 2 Mesozoic intrusives of western North America. 4 3 Geologic map of the Hidden Lake stock. 10 4 Geologic map of the Oval Peak batholith. 12 5 Geologic map of the Ten Peak pluton. 15 6 Geologic map of the Sulphur Mountain pluton. 17 7 Criteria used to define stable and unstable magnetic behavior during AF demagnetization. 24 8 Results of AF demagnetization of specimen HLl.llA. 29 9 Results of AF demagnetization of specimen HL2.01A. 30 10 Site mean directions for the Hidden Lake stock. 32 11 Plot of normalized intensity versus peak alter­ nating field for the Ten Peak pluton. 34 12 Results of AF demagnetization of specimen TP4,11A. 35 13 Results of AF demagnetization of specimen TP1.03A. 37 14 Contour diagrams of point density of directions for the Ten Peak pluton, 39 15 Trace of 7-10% concentrations from contour diagrams with plot of present day. Quaternary, Tertiary, and Cretaceous field directions. 41 16 Plot of normalized intensity versus peak AF and thermal cleaning levels for the Sulphur Mountain pluton. 43 17 Results of AF demagnetization of specimen 0P2.12A. 45 18 Results of AF demagnetization of specimen 0P4.01A. 46 19 Plot of normalized intensity versus peak AF for the Oval Peak batholith. 47 vii 20 Results of thermal demagnetization of specimen 0P2.10B. 48 21 Results of thermal demagnetization of specimen 0P4.03B. 49 22 Plot of normalized intensity versus peak temperature for the Oval Peak batholith. 50 23 Upward and downward directions plotted separately at the 50 oe and 200 oe AF cleaning levels for the Oval Peak batholith. 53 24 Site and overall mean directions for the Oval Peak batholith.
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