Cathodoluminescence study of Calcite in Martian meteorite T. Nakazato, M. Kayama, H. Nishido, K. Ninagawa, A. Gucsik, and Sz. Bérczi Research Institute.

Slides:



Advertisements
Similar presentations
Dejan Milidragovic and Don Francis
Advertisements

11 CRYOPLASMA IN HELIUM INDUCED BY CORONA DISCHARGE N. Bonifaci, F. Aitken, G2Elab Grenoble, France V Atrazhev, Joint Institute for High Temperatures,
Moon rocks, dust and lunar meteorites Key Features of the Moon: pages and
Cathodoluminescence spectral study of alkali feldspar and plagioclase in Yamato Martian nakhlite meteorites M. Kayama 1, A. Gucsik 2, N. Matsuda 3, H.
Identify, describe and explain the origin of basic and ultrabasic rocks using silica percentage. Basic (gabbro) = % SiO2 Ultrabasic = 44%
Most lasers are made of some material such as a crystal of ruby or a gas that is enclosed in a glass tube, like argon. Suppose an atom was in an excited.
Ultraviolet (UV) region 4 x m to m Region of greatest interest to organic chemists from 2 x m to 4 x meters 10.9 Ultraviolet Spectroscopy.
Olivine Transformation in SAH 293: Constraints on Shock Conditions C. Fudge, J. Hu and T. G. Sharp ASU/NASA Space Grant.
Cathodoluminescence imaging and spectral analyses of phosphates in the Martian meteorites: A review. A. Gucsik 1, W. J. Protheroe, Jr. 2, J.A.R. Stirling.
Very High Frequency Radiation makes Dark Matter Visible December 14th, Original work: R. Benton Metcalf & S.D.M. White: High-resolution.
Deconvolving Terrestrial Alteration Mineral Signatures from Meteorite Reflectance Measurements …to derive a precise and accurate spectrum of a weathered.
Mars High-Pressure Experiments COSMOCHEMISTRY iLLUSTRATED A Martian Primary Magma Olivine compositions in Martian meteorite Y indicate crystallization.
Carbonates on Mars Colin Dundas Ge/Ay 132. Outline Significance of carbonates Carbonate spectra Recent results concerning carbonates on Mars.
Group Meeting Reporter: Welson T.H. Sung Date: 2008/3/5 Topic: Raman and cathodoluminescence study of dislocation in GaN.
The Interior of Mars. Why do we need to know about the interior? Main reason: Because the chemical composition and minerals inside can tell us a lot about.
Minerals and Origin of the Moon Triana Henz. Formation Theories Fission Capture Co-formation Giant Impact.
Textures of Extraterrestrial Basalts COSMOCHEMISTRY iLLUSTRATED High-Ti Lunar Mare Basalt 0.25 mm.
Petrogensis of Diamonds in Ureilites (
© 2012 HORIBA Scientific. All rights reserved. Applications of Raman microspectroscopy to fluid inclusions phase identification. S. Mamedov *, R. S. Darling.
Optical Characterization of GaN-based Nanowires : From Nanometric Scale to Light Emitting Devices A-L. Bavencove*, E. Pougeoise, J. Garcia, P. Gilet, F.
ROCK vs. MINERAL n ROCK n Mixture n Can be separated by physical means n MINERAL n Pure substance n Has specific formula n Cannot be separated by physical.
APPLICATION OF UNDERWATER SPINAL TRACTION WITH UNDERWATER PHOTOTHERAPY FOR DEGENERATIVE-DYSTROPHIC DAMAGE OF THE SPINE. Vladimir Dodtievich BITSOEV State-Financed.
Deconvolving Terrestrial Alteration Mineral Signatures from Meteorite Reflectance Measurements …to derive a precise and accurate spectrum of a weathered.
Light and Energy Chemistry I. Classical description of light Light is an electromagnetic wave. Light consists of elementary particles called photons.
Open Earth Systems: An Earth Science Course For Maryland Teacher Professional Development EARTH HISTORY AND THE FOSSIL RECORD DAY 1 - Weds. July 8 AM Instruction:
Student: Danielle Clarke and Mentor: Briony Horgan ASU/NASA Space Grant Program.
Investigation on Reverse Water-gas Shift over La 2 NiO 4 Catalyst by cw-Cavity Enhanced Absorption Spectroscopy during CH 4 /CO 2 Reforming B.S. Liu, Ling.
SDBS Integrated Spectral Database for Organic Compounds Sample Search for Chemistry 130 Grace Baysinger and Dr. Dave Keller.
New Application of Cathodoluminescence to Earth and Planetary Sciences
Crust-atmosphere coupling and CO 2 sequestration on Mars Adrienne Macartney School of Geographical & Earth Sciences.
Compositional and Microtextural Analysis of Basaltic Pyroclastic Feedstock Materials Used for the 2010 ISRU Field Tests, Mauna Kea, Hawaii N. Marin, J.
Raman spectroscopy of volcanic lavas and inclusions of relevance to astrobiological exploration by Susana E. Jorge-Villar, and Howell G. M. Edwards Philosophical.
Laboratory of Molecular Spectroscopy, Pusan National University, Pusan, Republic of Korea Spectroscopic identification of isomeric trimethylbenzyl radicals.
Conversations with the Earth Tom Burbine
Sz. S. Józsa1, A. Gucsik2, Sz. Bérczi1, K. Ninagawa3, H
RAMAN INVESTIGATION OF TEMPERATURE PROFILES OF PHOSPHOLIPID DISPERSIONS IN THE BIOCHEMISTRY LABORATORY NORMAN C. CRAIG, Department of Chemistry and Biochemistry,
CONTENTS Emission Measurements Samples Preparation Fluorescence spectra Difficulties and limits Results and conclusions.
INTRACAVITY LASER SPECTRA OF METHANE 790 AND 861 nm BANDS AT LOW TEMPERATURES SADASIVAN SHAJI and JAMES J O’BRIEN Department of Chemistry & Biochemistry.
Slide 1 The Earth is differentiated How and When did this occur? Two Sets of Constraints: Physical Mechanisms and Chemical Signatures.
Jeff TaylorAges, Mantle Sources, Differentiation1 SNC Ages, Mantle Sources, and the Differentiation of Mars Crystallization ages of Martian meteorites.
Cathodoluminescence Properties of Silicon Thin Films Crystallized by Electron Beam Exposure P47 Advanced Display Research Center, Kyung Hee University.
Date of download: 6/25/2016 Copyright © 2016 SPIE. All rights reserved. Lensfree imaging module. (a) Schematic illustrating the principle of lensfree image.
The Study of Light. The Electromagnetic Spectrum  includes gamma rays, X-rays, ultraviolet light, visible light, infrared radiation, microwaves, and.
High-Order Sideband Generation Jordan Grace Physics Mentor: Hunter Banks Faculty Advisor: Prof. Mark Sherwin Institute for Terahertz Science and Technology.
Aqueous Alteration on Mars
The Study of Light.
Second MPSE Workshop Warsaw, 3-5 June WROONA Group, Institute of Geological Sciences PAS, Wrocław, Poland 2 Space Research Centre PAS, Warsaw, Poland.
Jamie Wallis, Daryl H. Wallis, Max K Wallis + N. Chandra Wickramasinghe EPSC2014 session TP4.1 Portugal Sept
Leah Salditch February 27, 2017 Mars Final Project
Raman spectroscopy study of shocked olivine in Hungarian
Mingyun Li & Kevin Lehmann Department of Chemistry and Physics
Chapter 15 Structure Determination by Spectroscopy (II): UV-Vis & Mass
Author Name 1, Author Name 2, & Author Name 3
Introduction to Mineralogy Dr
Volcanism and an Ancient Atmosphere on the Moon
TITLE Authors Institution RESULTS INTRODUCTION CONCLUSION AIMS METHODS
Pamela Aaron, Dr. Charles Shearer, and Paul Burger
ADINA INSTITUTE OF SCIENCE AND TECHNOLOGY
New Martian Meteorite: Northwest Africa (NWA 7034)
ADINA INSTITUTE OF SCIENCE AND TECHNOLOGY
Author Name 1, Author Name 2, & Author Name 3
Author Name 1, Author Name 2, & Author Name 3
Damp Moon Rising Overview: The discovery in 2008 by Alberto Saal (Brown University) and colleagues that lunar volcanic glasses contain water surprised.
by J. L. Jayanthi, V. Nandakumar, and S. S. Anoop
Molecular Vibrations and IR Spectroscopy
Author Name 1, Author Name 2, & Author Name 3
Fig. 3 Raman spectroscopy of the phonon-polariton laser and the reference laser with GaAaSb barriers. Raman spectroscopy of the phonon-polariton laser.
Fig. 3 Raman spectra for the composite materials of the TS.
Fig. 4 Micro-Raman analyses of high-pressure SiO2 phases.
Fig. 3 Micro-Raman analyses of another amygdaloidal silica micrograin in the breccia matrix. Micro-Raman analyses of another amygdaloidal silica micrograin.
Presentation transcript:

Cathodoluminescence study of Calcite in Martian meteorite T. Nakazato, M. Kayama, H. Nishido, K. Ninagawa, A. Gucsik, and Sz. Bérczi Research Institute of Natural Science, Okayama University of Science Department of Applied Physics, Okayama University of Science Max Planck Institute for Chemistry, Department of Geochemistry Eötvös University, Institute of Physics, Dept. G. Physics, Cosmic Materials Space NASA

Introduction CL and Raman spectroscopy were carried out on Dhofar 019 for origin of calcite. NASA

SNC : Martian meteorites Nakhlite Shergottite Chassignite Olivine bearing Basaltic Shergottite Augite, Pigeonite, Maskelynite Lherzolitic Shergottite Olivine, Pyroxene Shergottite 1865 India Shergotty Nakhlite 1911 Egypt Nakhla Chassignite 1815 France Chassgny Shergottite

Classification : Olivine bearing Basaltic Shergottite Constituent minerals : Pyroxene, Olivine, Maskelynite, merrillite and calcite Shock pressure : 30 GPa or more Formation age : ~ 500Ma Exposure age : ~ 15 million years Finding : Oman desert Weight : 1,056 g No fusion crust Photograph of Dhofar 019 Sample (Dhofar 019) Dhofar region

5mm Color CL images of Dhofar 019 Color CL image of Dhofar 019 : measured area Vein S L

measurement condition 15kv, 1.0nA CL spectra of calcite ( S and L ) S L BSE image of calcite (S, L) CL spectra of calcite (S and L)

BSE image of calcite (Vein) CL spectrum of calcite ( Vein ) Vein CL spectrum of calcite (Vein) measurement condition 15kv, 1.0nA

BSE image of calcite (Vein) CL spectra of calcite S L BSE image of calcite (S and L) Vein CL spectra of calcite in Dhofar019 and terrestrial calcite

Raman spectra of calcite Raman spectra of calcite in Dhofar019 and terrestrial calcite measurement condition light source : Ar-laser, 514.5nm power : 400 mW

Terrestrial (cm -1 ) Vein (cm -1 ) S (cm -1 ) L (cm -1 ) Raman peak shift of calcite Wave numbers of Raman peaks

Terrestrial (cm -1 ) Vein (cm -1 ) S (cm -1 ) L (cm -1 ) Raman peak shift of calcite Wave numbers of Raman peaks

Conclusion CL spectra Calcite in Dhofar 019 shows different spectra from terrestrial one. Raman spectra Calcite in Dhofar 019 show weaker Raman peak than terrestrial one. Calcite in Dhofar019 Martian origin

Thank you, very much.