1
|
Zhang JS, Zhou WY, Vu TH, Hodyss R, Yu X. Single-Crystal Elasticity of α-Hydroquinone-An Analogue for Organic Planetary Materials. ACS EARTH & SPACE CHEMISTRY 2025; 9:1-7. [PMID: 39839372 PMCID: PMC11744926 DOI: 10.1021/acsearthspacechem.4c00322] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 10/29/2024] [Revised: 12/27/2024] [Accepted: 12/30/2024] [Indexed: 01/23/2025]
Abstract
In this study, we measured the single-crystal elasticity of α-hydroquinone at ambient conditions using Brillouin spectroscopy to assess the feasibility of this technique for studying the mechanical properties of organic ices in the outer solar system. In this study, α-hydroquinone serves as an ambient temperature analogue for low-temperature organic ices on Titan and other solar system bodies. We found that a satisfactory Brillouin spectrum can be obtained in less than 5 min of experimental time with negligible damage to the sample. The best fit single-crystal elastic moduli of α-hydroquinone were determined as C 11 = 13.67(8) GPa, C 33 = 10.08(6) GPa, C 44 = 4.54(5) GPa, C 12 = 6.9(7) GPa, C 13 = 7.02(7) GPa, C 14 = 0.54(4) GPa, C 25 = 0.51(9) GPa, and C 66 = (C 11 - C 12)/2 = 3.4(3) GPa, with bulk modulus K S = 8.7(2) GPa and shear modulus G = 3.4(3) GPa. These results demonstrate that Brillouin spectroscopy is a powerful tool for characterizing the elastic properties of organic materials. The elastic properties of organic ices can be broadly applied to understand planetary surface processes and also aid in evaluating the feasibility and technical readiness of future lander, sampling, and rover missions in the outer solar system.
Collapse
Affiliation(s)
- Jin S. Zhang
- Department
of Geology and Geophysics, Texas A&M
University, College
Station, Texas 77845, United States
| | - Wen-Yi Zhou
- Department
of Geology and Geophysics, Texas A&M
University, College
Station, Texas 77845, United States
| | - Tuan H. Vu
- Jet
Propulsion Laboratory, California Institute
of Technology, Pasadena, California 91109, United States
| | - Robert Hodyss
- Jet
Propulsion Laboratory, California Institute
of Technology, Pasadena, California 91109, United States
| | - Xinting Yu
- Department
of Physics and Astronomy, University of
Texas at San Antonio, San Antonio, Texas 78249, United States
| |
Collapse
|
2
|
Constraining composition and temperature variations in the mantle transition zone. Nat Commun 2022; 13:1094. [PMID: 35232983 PMCID: PMC8888558 DOI: 10.1038/s41467-022-28709-7] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/06/2021] [Accepted: 01/24/2022] [Indexed: 11/17/2022] Open
Abstract
The mantle transition zone connects two major layers of Earth’s interior that may be compositionally distinct: the upper mantle and the lower mantle. Wadsleyite is a major mineral in the upper mantle transition zone. Here, we measure the single-crystal elastic properties of hydrous Fe-bearing wadsleyite at high pressure-temperature conditions by Brillouin spectroscopy. Our results are then used to model the global distribution of wadsleyite proportion, temperature, and water content in the upper mantle transition zone by integrating mineral physics data with global seismic observations. Our models show that the upper mantle transition zone near subducted slabs is relatively cold, enriched in wadsleyite, and slightly more hydrated compared to regions where plumes are expected. This study provides direct evidence for the thermochemical heterogeneities in the upper mantle transition zone which is important for understanding the material exchange processes between the upper and lower mantle. A new study by @JinZhang_MP models the global distribution of wadsleyite proportion, temperature and water content in the upper mantle transition zone.
Collapse
|
3
|
Zhang JS, Irifune T, Hao M, Zhang D, Hu Y, Tkachev S, Dera P, Chen J, Jiang YB, Brearley AJ, Bass JD, Prakapenka V. Grain size dependent high-pressure elastic properties of ultrafine micro/nanocrystalline grossular. Sci Rep 2021; 11:22481. [PMID: 34795364 PMCID: PMC8602367 DOI: 10.1038/s41598-021-01960-6] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/12/2021] [Accepted: 11/08/2021] [Indexed: 11/10/2022] Open
Abstract
We have performed sound velocity and unit cell volume measurements of three synthetic, ultrafine micro/nanocrystalline grossular samples up to 50 GPa using Brillouin spectroscopy and synchrotron X-ray diffraction. The samples are characterized by average grain sizes of 90 nm, 93 nm and 179 nm (hereinafter referred to as samples Gr90, Gr93, and Gr179, respectively). The experimentally determined sound velocities and elastic properties of Gr179 sample are comparable with previous measurements, but slightly higher than those of Gr90 and Gr93 under ambient conditions. However, the differences diminish with increasing pressure, and the velocity crossover eventually takes place at approximately 20-30 GPa. The X-ray diffraction peaks of the ultrafine micro/nanocrystalline grossular samples significantly broaden between 15-40 GPa, especially for Gr179. The velocity or elasticity crossover observed at pressures over 30 GPa might be explained by different grain size reduction and/or inhomogeneous strain within the individual grains for the three grossular samples, which is supported by both the pressure-induced peak broadening observed in the X-ray diffraction experiments and transmission electron microscopy observations. The elastic behavior of ultrafine micro/nanocrystalline silicates, in this case, grossular, is both grain size and pressure dependent.
Collapse
Affiliation(s)
- Jin S. Zhang
- grid.266832.b0000 0001 2188 8502Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131 USA ,grid.266832.b0000 0001 2188 8502Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131 USA
| | - T. Irifune
- grid.255464.40000 0001 1011 3808Geodynamics Research Center (GRC), Ehime University, Matsuyama, Ehime 790-8577 Japan
| | - M. Hao
- grid.266832.b0000 0001 2188 8502Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131 USA
| | - D. Zhang
- grid.170205.10000 0004 1936 7822Center of Advanced Radiation Sources, University of Chicago, Chicago, IL 60637 USA ,grid.410445.00000 0001 2188 0957Department of Geology and Geophysics, School of Ocean and Earth Science and Technology, Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI 96822 USA
| | - Y. Hu
- grid.410445.00000 0001 2188 0957Department of Geology and Geophysics, School of Ocean and Earth Science and Technology, Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI 96822 USA
| | - S. Tkachev
- grid.170205.10000 0004 1936 7822Center of Advanced Radiation Sources, University of Chicago, Chicago, IL 60637 USA
| | - P. Dera
- grid.410445.00000 0001 2188 0957Department of Geology and Geophysics, School of Ocean and Earth Science and Technology, Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI 96822 USA
| | - J. Chen
- grid.59053.3a0000000121679639School of Earth and Space Sciences, University of Science and Technology of China, Hefei, 230026 China
| | - Ying-Bing Jiang
- grid.266832.b0000 0001 2188 8502Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131 USA
| | - Adrian J. Brearley
- grid.266832.b0000 0001 2188 8502Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131 USA
| | - J. D. Bass
- grid.35403.310000 0004 1936 9991Department of Geology, University of Illinois, Urbana, 61801 USA
| | - V. Prakapenka
- grid.170205.10000 0004 1936 7822Center of Advanced Radiation Sources, University of Chicago, Chicago, IL 60637 USA
| |
Collapse
|
4
|
A Review of the Melting Curves of Transition Metals at High Pressures Using Static Compression Techniques. CRYSTALS 2021. [DOI: 10.3390/cryst11040416] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/01/2023]
Abstract
The accurate determination of melting curves for transition metals is an intense topic within high pressure research, both because of the technical challenges included as well as the controversial data obtained from various experiments. This review presents the main static techniques that are used for melting studies, with a strong focus on the diamond anvil cell; it also explores the state of the art of melting detection methods and analyzes the major reasons for discrepancies in the determination of the melting curves of transition metals. The physics of the melting transition is also discussed.
Collapse
|
5
|
A Practical Review of the Laser-Heated Diamond Anvil Cell for University Laboratories and Synchrotron Applications. CRYSTALS 2020. [DOI: 10.3390/cryst10060459] [Citation(s) in RCA: 17] [Impact Index Per Article: 3.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
In the past couple of decades, the laser-heated diamond anvil cell (combined with in situ techniques) has become an extensively used tool for studying pressure-temperature-induced evolution of various physical (and chemical) properties of materials. In this review, the general challenges associated with the use of the laser-heated diamond anvil cells are discussed together with the recent progress in the use of this tool combined with synchrotron X-ray diffraction and absorption spectroscopy.
Collapse
|
6
|
Smith D, Smith JS, Childs C, Rod E, Hrubiak R, Shen G, Salamat A. A CO 2 laser heating system for in situ high pressure-temperature experiments at HPCAT. THE REVIEW OF SCIENTIFIC INSTRUMENTS 2018; 89:083901. [PMID: 30184683 DOI: 10.1063/1.5040508] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/17/2018] [Accepted: 07/07/2018] [Indexed: 06/08/2023]
Abstract
We present a CO2 laser heating setup for synchrotron x-ray diffraction inside a diamond anvil cell, situated at HPCAT (Sector 16, Advanced Photon Source, Argonne National Lab, Illinois, USA), which is modular and portable between the HPCAT experiment hutches. The system allows direct laser heating of wide bandgap insulating materials to thousands of degrees at static high pressures up to the Mbar regime. Alignment of the focused CO2 laser spot is performed using a mid-infrared microscope, which addressed past difficulties with aligning the invisible radiation. The implementation of the mid-infrared microscope alongside a mirror pinhole spatial filter system allows precise alignment of the heating laser spot and optical pyrometry measurement location to the x-ray probe. A comparatively large heating spot (∼50 μm) relative to the x-ray beam (<10 μm) reduces the risk of temperature gradients across the probed area. Each component of the heating system and its diagnostics have been designed with portability in mind and compatibility with the various experimental hutches at the HPCAT beamlines. We present measurements on ZrO2 at 5.5 GPa which demonstrate the improved room-temperature diffraction data quality afforded by annealing with the CO2 laser. We also present in situ measurements at 5.5 GPa up to 2800 K in which we do not observe the postulated fluorite ZrO2 structure, in agreement with recent findings.
Collapse
Affiliation(s)
- Dean Smith
- Department of Physics and Astronomy and HiPSEC, University of Nevada Las Vegas, Las Vegas, Nevada 89154, USA
| | - Jesse S Smith
- High Pressure Collaborative Access Team, Geophysical Laboratory, Carnegie Institution of Washington, Argonne, Illinois 60439, USA
| | - Christian Childs
- Department of Physics and Astronomy and HiPSEC, University of Nevada Las Vegas, Las Vegas, Nevada 89154, USA
| | - Eric Rod
- High Pressure Collaborative Access Team, Geophysical Laboratory, Carnegie Institution of Washington, Argonne, Illinois 60439, USA
| | - Rostislav Hrubiak
- High Pressure Collaborative Access Team, Geophysical Laboratory, Carnegie Institution of Washington, Argonne, Illinois 60439, USA
| | - Guoyin Shen
- High Pressure Collaborative Access Team, Geophysical Laboratory, Carnegie Institution of Washington, Argonne, Illinois 60439, USA
| | - Ashkan Salamat
- Department of Physics and Astronomy and HiPSEC, University of Nevada Las Vegas, Las Vegas, Nevada 89154, USA
| |
Collapse
|