Supporting document for

Slides:



Advertisements
Similar presentations
IC5.5.5 Formulae of salts © Oxford University Press 2011 Formulae of salts How to work out the formulae of salts.
Advertisements

Annihilators at Mars: Are there alternative but reasonable magnetization distributions in the Martian crust that explain the MGS magnetic field observations?
WRITING FORMULA FOR IONIC COMPOUNDS
Ch 12: A Deeper Look at Chemical Equilibrium Up to now we've ignored two points
Temporal Variability of Gamma- Ray Lines from the X-Class Solar Flare of 2002 July 23 Albert Y. Shih 1,2, D. M. Smith 1, R. P. Lin 1,2, S. Krucker 1, R.
THE OCEANS OF EUROPA AND GANYMEDE. AQUEOUS SOLUTION UNDER PRESSURE AS POTENTIAL HABITATS O. Prieto-Ballesteros (1), V. Muñoz-Iglesias (1) and L. Jiménez.
Naming Ionic Compounds
SNC 1D1 –Nomenclature Review
Experimental Methods  Solutions were prepared of 10, 15, 20, 25 wt% MgSO 4 ; and 10.9, 13.7, 17.8, and 18.0 wt% FeSO 4  Experimental conditions inside.
Jian-Yang Li, University of Maryland Marc Kuchner, NASA Goddard Space Flight Center Ron Allen, Space Telescope Science Institute Scott Sheppard, Carnegie.
Figure S1. (A-H) Current/voltage curves in KCl. (I) The conductance at reversal potential with cytosolic [K + ] held at 250 mM and lumenal [K + ] is varied.
Ionic bonds and Compounds. TYPES OF BONDS IONIC BONDS COVALENT BONDS transfer of electrons between a Cation and an Anion resulting bond is neutral sharing.
What is a compound? A substance in which the atoms of two or more different elements combine together Sodium chloride NaCl Carbon dioxide CO 2 Calcium.
CRYSTAL STRUCTURE PARAMETERS AS PREDICTORS OF VNIR SPECTROSCOPY OF SYNTHETIC PYROXENES S. E. Peel 1, M. D. Dyar 1, Rachel L. Klima 2. 1 Dept. of Astronomy,
1. Overview About Washington University / Planetary Data Systems Geosciences Node Initial and continued interactions in China NASA-CNSA Bilateral (July.
Solubility Equilibria (Sec 6-4) K sp = solubility product AgCl(s) = Ag + (aq) + Cl - (aq) K sp = CaF 2 (s) = Ca 2+ (aq) + 2F - (aq) K sp = in general A.
1 Testing of Phase Transition and Bubble Dynamics Using A Four-Point Optical Probe Adam Wehrmeister, Junli Xue, M. H. Al-Dahhan, M. P. Dudukovic Chemical.
“Life in the Atacama” 2013 Rover Field Campaign in Chile Autonomous Analysis of Robotic Core Materials by the Mars Microbeam Raman Spectrometer (MMRS)
Oxygen Tolerance in Methanogens Jill K. Jackson 1,2, Dr. Timothy Kral 2,3 1 William Jewell College Depts. of Biology and Chemistry, 2 University of Arkansas.
Pressure-Temperature Stability Studies of Talc and 10-Å phase using x-ray diffraction. Arianna E. Gleason 1, Martin Kunz 1, Stephen Parry 2, Alison Pawley.
All chemical reactions can be placed into one of six categories. Here they are, in no particular order: 1) Synthesis/Combination 2) Decomposition 3) Single.
New opportunities for in situ sampling of water and carbon- dioxide isotopologues within the soil and atmosphere at LEO.
Lecture 59 Formulas of Hydrates Ozgur Unal 1.  What is the difference between the two fruits? 2  Can you find how much water was removed from the fruit?
Solubility.
Kaiem L. Frink Lecture Series Elizabeth City State University Department of Mathematics and Computer Science Adjunct Professor/Graduate Student Major Applied.
Supporting Information Decomposition kinetics and recycle of binary hydrogen- tetrahydrofuran clathrate hydrate Hiroki Yoshioka 1, Masaki Ota 1,Yoshiyuki.
Chemical Bonds Why Atoms Combine?. Why Would Elements Want to Combine? Most elements are unstable The only stable elements are the _____? So elements.
SELF- AND CO 2 -BROADENED LINE SHAPE PARAMETERS FOR THE 2 AND 3 BANDS OF HDO V. MALATHY DEVI, D. CHRIS BENNER, Department of Physics, College of William.
1 Center for Astrophysics and Space Sciences, University of California, San Diego 9500 Gilman Drive #0424, La Jolla, CA , U.S.A
Chemistry During Accretion of the Earth Laura Schaefer and Bruce Fegley Planetary Chemistry Laboratory McDonnell Center for the Space Sciences Department.
Efflorescence, Deliquescence &
1 Cross sections of neutron reactions in S-Cl-Ar region in the s-process of nucleosynthesis C. Oprea 1, P. J. Szalanski 2, A. Ioan 1, P. M. Potlog 3 1Frank.
NIS – PHYSICAL SCIENCE Lecture 88 – Lecture 89 – Lecture 90
Comparison of lidar water vapor measurements at Fixed PISA 2
EART193 Planetary Capstone
Figures for Subsurface Hydrous Chlorides and Oxychlorine Salts (HyCOS)
Warm-Up Balance the following equations
Methane in the Martian Atmosphere
WATER IN MARS In the first-ever definitive signs of the presence of liquid water -- and possibly life -- on the Red Planet, NASA’s Mars Reconnaissance.
The Quadrennial Ozone Symposium 2016
Thermodynamic behavior of FeCl3-H2O and HCl-FeCl3-H2O
A High-Temperature CO2–Brine Phase-Partitioning Model for
Chapter 15 Water and Aqueous Systems 15.2 Homogeneous Aqueous Systems
Table 1. Seed storage information
Efflorescence, Deliquescence &
Types of Compounds Ch. 5.
Synthesis of Molecules by Cosmic Ion Bombardment
Fresh Exposures of Hydrous Fe-bearing Amorphous Silicates on Mars
Zinc Isotopes Provide Clues to Volatile Loss During Moon Formation
Using Immersive Technology to Introduce Planetary Geology to Undergraduate Maritime Studies Students As part of its scientist engagement efforts, the Lunar.
Predicting Chemical Reactions
ATMOSPHERIC AEROSOL: suspension of condensed-phase particles in air
Science Starter Write a chemical reaction for the following situation. Once written, please balance. Phosphoric Acid reacts with Sodium Hydroxide.
Hydrated Sulfates on Mars: Characterizing Visible To Near-Infrared Spectra and Implications for Rover-Based Imagers Darian Dixon, Western Washington University.
Hydrates Unit 6 Lesson 3.
Modelling Chemical Reactions
The Phase Diagram of FeO
Solar radiation, total column ozone content and aerosol optical properties monitoring at the ground-based station in Kishinev, Moldova A.Aculinin1, A.
a b c d Figure 1. Laboratory set-up for Experiment #3. CaCl2 CO2
Chapter 11 Chemical Reactions 11.2 Types of Chemical Reactions
IONIC COMPOUNDS.
Section 3 Writing & Naming Compounds
Dr. S. B Maulage Dept of Chemistry.
Table 1. Iterative calculation procedure, M is standard at 25°C
Public Engagement Lead LRO and SAM
Warm Up # 1 Using the terms solution, solvent and solute, explain how dissolving works. What property of water allows it to have a lower density in its.
Hydrates Unit 6 Lesson 3.
Table I lab A Prelab Exercise Block 1 Phase at Room Temperature
GSFC Solar System Exploration Division
Data from present research
Presentation transcript:

Supporting document for   The Potential Source Materials for Recurring Slope Lineae on Mars: Subsurface Hydrous Chlorides and Oxychlorine Salts (HyCOS) Authors: Alian Wang1, Zongcheng Ling2, Y. C. Yan1, Alfred S. McEwen3, Michael T. Mellon4, Michael D. Smith5, Bradley L. Jolliff1, James Head6 Affiliations: 1Dept. Earth and Planetary Sciences and McDonnell Center for Space Sciences, Washington University in St. Louis, St. Louis, Missouri, 63130, USA; 2Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, 264209, China; 3Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, 85721, USA; 4Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, 20723, USA 5NASA Goddard Space Flight Center, Greenbelt, Maryland, 20771, USA 6Dept. Earth, Environmental and Planetary Sciences, Brown University, Rhode Island, 02912, USA; This document contains: Figure S1. Stability field and phase boundaries of hydrous Mg-sulfates Figure S2. Stability field and phase boundaries of hydrous Fe3+-sulfates Figure S1. Stability field and phase boundaries of hydrous Fe2+-sulfates Table S1. RHbuffer (T) of ten EH buffers used in experiment #1

brine Figure S1. Stability fields and phase boundaries of hydrous Mg-sulfates 1,2,3 Notice the 7w-deliquescence boundary intersects with 273K isothermal line at about 95%RH. Am=amorphousMgSO4·xH2O (x<3), LH-1w=Low Humidity MgSO4·H2O; 4w=MgSO4·4H2O, 6w=MgSO4·6H2O, 7w=MgSO4·7H2O, LT-7w=low temperature MgSO4·7H2O , 11w=MgSO4·11H2O, deliq=deliquescence, meta=metastable.

brine Figure S2. Stability fields and phase boundaries of hydrous Fe3+ -sulfates 4,5,6,7, Notice the 20W-deliquescence boundary intersects with 273K isothermal line at about 75 %RH. 4w=FeHSO4·4H2O, 5w=Fe2(SO4)3.5H2O, 7w=Fe2(SO4)3.7H2O, p9w=paracoquimbite =Fe2(SO4)3.9H2O, 20w=Fe4.67(SO4)6(OH)2.20H2O, Am=amorphous Fe2(SO4)3.5H2O, deliq=deliquescence.

Chou et al., 2002 10 brine Figure S3. Stability fields and phase boundaries of hydrous Fe2+ -sulfates 8,9 Notice the 7w-deliquescence boundary intersects with 273K isothermal line at about 96%RH. 1w=FeSO4·H2O; deliq=deliquescence.

Table S1. RHbuffer (T) of ten EH buffers used in experiment #1 323K 294K 278K LiBr 5.5 6.6 7.4 LiCl 11.3 MgCl2 30.5 33.0 33.6 Mg(NO3)2 45.4 54.1 58.9 NaBr 51.5 58.8 63.5 KI 64.5 70.0 73.3 NaCl 74.4 75.4 75.7 KCl 81.2 85.0 87.7 KNO3 84.8 94.4 96.3 H2O 100 100.0 *Data from Greenspan 197711.

References cited in supporting document: Wang Alian, Freeman J. F., Jolliff B. L., Chou I. M, (2006) Sulfates on Mars: a Systematic Raman Spectroscopic Study of Hydration States of Magnesium Sulfates, Geochim. Cosmochim. Acta, V70, p6118-6135. Wang Alian, John J. Freeman, Bradley, L. Jolliff (2009), Phase Transition Pathways of the Hydrates of Magnesium Sulfate in the Temperature Range 50 ºC to 5 ºC: Implication for Sulfates on Mars, J. Geophys. Res., 114, doi:10.1029/2008JE003266. Wang Alian, J. J. Freeman, I-Ming Chou, B. L. Jolliff (2011), Stability of Mg-sulfates at -10C and the Rates of Dehydration/Rehydration Processes under Mars Relevant Conditions, J. Geophys. Res., Res., 116, E12006, doi:10.1029/2011JE003818. Wang Alian, Ling Z. C. Freeman J. J. (2012) Stability field and Phase Transition Pathways of Hydrous Ferric Sulfates in the Temperature Range 50 °C to 5 °C: Implication for Martian Sulfates, Icaru, 218, 622-643, doi:10.1016/j.icarus.2012.01.003. Kong, W. G., Alian Wang, and I-M. Chou (2011), Determination of phase boundary between kornelite and pentahydrated Ferric Sulfate by humidity buffer technique and Raman spectroscopy at 0.1 Mpa. Chemical Geology, Vol 284, 333-338. Kong W. G., Alian Wang, John J. Freeman, and Pablo Sobron (2011), A Comprehensive Spectroscopic Study of Synthetic Fe2+, Fe3+, Mg2+, Al3+ Copiapite, J. Raman Spectroscopy, doi10.1002/jrs.2790. Ling Z. C., Alian Wang (2010), A Systematic Spectroscopic Study of Eight Hydrous Ferric Sulfates Relevant to Mars, Icarus, 209, 422-433, doi:/10.1016/j.icarus.2010.05.009. Alian Wang and Kathryn Connor, 2014, Stability fields of hydrous ferrous sulfates and their pathways in dehydration-rehydration processes, Abs #1070 for 8th International Conference on Mars Wang Alian, Yuhang Zhou (2014) Experimental Comparison of the Pathways and Rates of the Dehydration of Al-, Fe-, Mg-, and Ca-Sulfates under Mars Relevant Conditions, ICARUS, 234, 162-173. Chou I.M., R. R. Seal II, B. S. Hemingway, Determination of melanterite-rozenite and Chalcanthite-bonattite equilibria by humidity measurements at 0.1 Mpa, Am. Mineralogists, V87, p108-114. Greenspan, L. Humidity fixed points of binary saturated aqueous solution. J. Res. Natl. Bureau of Standards—A. Phys. Chem. 81A (1), 89–96 (1977).