Deciphering Redox State for a Metal-Rich World

被引:0
|
作者
Timothy J. McCoy
Steven D. Dibb
Patrick N. Peplowski
Clara Maurel
Hannah L. Bercovici
Catherine M. Corrigan
James F. Bell
Benjamin P. Weiss
David J. Lawrence
Daniel D. Wenkert
Thomas H. Prettyman
Lindy T. Elkins-Tanton
机构
[1] Smithsonian Institution,Dept. of Mineral Sciences, National Museum of Natural History
[2] Arizona State University,School of Earth and Space Exploration
[3] Johns Hopkins Applied Physics Laboratory,Dept. of Earth, Atmospheric and Planetary Sciences
[4] Massachusetts Institute of Technology,Mission Systems and Operations Division, Jet Propulsion Laboratory
[5] California Institute of Technology,undefined
[6] Planetary Science Institute,undefined
来源
Space Science Reviews | 2022年 / 218卷
关键词
Psyche; Oxidation-reduction; Iron meteorites; Chemical composition; Spectroscopy;
D O I
暂无
中图分类号
学科分类号
摘要
The Psyche mission’s Oxidation-Reduction Working Group is focused on understanding, determining, and applying the redox state of (16) Psyche to understand the origin of a metal-rich world. The oxidation-reduction state of an asteroid, along with its temperature, parent body size, and composition, is a key parameter in determining the history of an asteroid. Determining the redox state from spacecraft data is most easily done by examining potential metal-oxide buffer pairs. The occurrence of Ni, Fe, C, Cr, P and Si, in that order, in the metal or sulfide phase of an asteroidal body indicates increasingly reduced conditions. Key observations by the Imager and Gamma-Ray and Neutron Spectrometer (GRNS) of Psyche can bracket the redox state using metal-oxide buffers. The presence of Fe,Ni metal can be confirmed by the ratios of Fe/O or Fe/Si and the concentration of Ni variability in metal across the asteroid can be determined by GRNS. The FeO concentration of silicates is complementary to the Ni concentration of metal and can be constrained using filters on the Imager. The presence of FeO in silicates from ground-based observations is one of the few measurements we already have of redox state, although available data permit a wide range of silicate compositions and mineralogies. The presence of C, P or Si concentrated in the metallic, Fe-rich portion of the asteroid, as measured by GRNS, or Ca-sulfide, determined by imaging, would indicate increasingly reducing conditions. Linkage to known types of meteorites, whether metal-rich chondrites, stony-irons or irons, expands the mineralogical, chemical and isotopic data not available from remote observations alone. Redox also controls both silicate and metal mineralogy, influencing differentiation, solidification, and subsolidus cooling, including the relative abundance of sulfur in the core and possible magnetic signatures. The redox state of Psyche, if a fully-differentiated metallic core, might constrain the location and timing of both the formation of Psyche and any oxidation it might have experienced.
引用
收藏
相关论文
共 50 条
  • [41] NEW PROCESS HYDROTREATS METAL-RICH FEEDSTOCKS
    VANZIJLLLANGHOUT, WC
    OUWERKERK, C
    PRONK, KMA
    OIL & GAS JOURNAL, 1980, 78 (48) : 120 - 126
  • [42] The Sgr dSph hosts a metal-rich population
    Bonifacio, P
    Sbordone, L
    Marconi, G
    Pasquini, L
    Hill, V
    ASTRONOMY & ASTROPHYSICS, 2004, 414 (02) : 503 - 514
  • [43] The metal-rich disk population - Oxygen abundances
    Feltzing, S
    Gustafsson, B
    NEW LIGHT ON GALAXY EVOLUTION, 1996, (171): : 372 - 372
  • [44] The metal-rich globular clusters of the Milky Way
    Heitsch, F
    Richtler, T
    ASTRONOMY & ASTROPHYSICS, 1999, 347 (02) : 455 - 472
  • [45] CRYSTAL STRUCTURES OF METAL-RICH TRANSITION METAL SULFIDES AND SELENIDES
    FRANZEN, HF
    ABSTRACTS OF PAPERS OF THE AMERICAN CHEMICAL SOCIETY, 1969, (SEP): : P167 - &
  • [46] Metal-rich, neutral and cationic organotin clusters
    Richards, AF
    Eichler, BE
    Brynda, M
    Olmstead, MM
    Power, PP
    ANGEWANDTE CHEMIE-INTERNATIONAL EDITION, 2005, 44 (17) : 2546 - 2549
  • [47] COOL DEGENERATE DWARF WITH A METAL-RICH ATMOSPHERE
    HINTZEN, P
    TAPIA, S
    ASTROPHYSICAL JOURNAL, 1975, 199 (01): : L31 - L33
  • [48] On some properties of very metal-rich stars
    Mowlavi, N
    Meynet, G
    Maeder, A
    Schaerer, D
    Charbonnel, C
    ASTRONOMY & ASTROPHYSICS, 1998, 335 (02): : 573 - 582
  • [49] The Strikingly Metal-rich Halo of the Sombrero Galaxy
    Cohen, Roger E.
    Goudfrooij, Paul
    Correnti, Matteo
    Gnedin, Oleg Y.
    Harris, William E.
    Chandar, Rupali
    Puzia, Thomas H.
    Sanchez-Janssen, Ruben
    ASTROPHYSICAL JOURNAL, 2020, 890 (01):
  • [50] Failure to launch: industrialisation in metal-rich Philippines
    Ofreneo, Rene E.
    JOURNAL OF THE ASIA PACIFIC ECONOMY, 2009, 14 (02) : 194 - 209