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Mineralogical Analysis of Quadrangle Ac-H-10 Rongo on the Dwarf Planet Ceres

Zambon, F. and Carrozzo, F. G. and Tosi, F. and Ciarniello, M. and Combe, J.-P. and Frigeri, A. and Desanctis, M.C. and Thangiam, G. and Nathues, A. and Hoffmann, M. and Longobardo, A and Stephan, Katrin and Raponi, A. and Ammannito, E. and Krohn, Katrin and McFadden, L.A. and Palomba, E. and Raymond, C.A. and Russell, C.T. (2019) Mineralogical Analysis of Quadrangle Ac-H-10 Rongo on the Dwarf Planet Ceres. Icarus: International Journal of Solar System Studies, 318, pp. 212-229. Elsevier. doi: 10.1016/j.icarus.2017.09.021. ISSN 0019-1035.

Full text not available from this repository.

Official URL: http://www.sciencedirect.com/science/article/pii/S0019103517303378

Abstract

Quadrangle Ac-H-10 ‘Rongo’ (Lat 22°S to 22°N, Lon 288°–360°E) shows a fairly homogeneous topography, with the presence of notable elevations such as Ahuna Mons, Liberalia Mons, and part of Samhain and Uhola Catenae. The deepest areas correspond to the Rongo crater region, the areas between Samhain and Uhola catenae, and the region of the quadrangle south of Ahuna Mons. A substantial variability in the 2.7-µm band depth distribution is observed across the Rongo quadrangle, indicating an east-west gradient in the abundance of Mg-phyllosilicates. The NH4-phyllosilicates distribution appears quite homogeneous, except some localized regions, such as crater Haulani's ejecta, the flanks of Ahuna Mons, and crater Begbalel. The two band depths at 2.7 and 3.1 µm display an overall low correlation, suggesting a variable degree of mixing between Mg-phyllosilicates and NH4-phyllosilicates. At the local scale, mineralogical phases other than phyllosilicates are observed. Quadrangle Rongo includes sodium carbonate-rich regions, such as the flanks of Ahuna Mons, the ejecta of Xevioso crater located in the southern edge of Liberalia Mons, and crater Begbalel, which often display a reduction in both the 2.7- and 3.1-µm band depths, associated with an increased band depth at ∼4 µm, related to the presence of Na-rich carbonate phases. This suggests recent hydrothermal activity in this area, due to several episodes of cryovolcanism, or impacts that unveiled a peculiar composition in the shallow subsurface. Alternatively, the crust in this region might show a variable degree of compactness, such that the formation of Na-carbonates is favored only in specific locations (De Sanctis et al., 2016; Ruesch et al., 2016; Zambon et al., 2017). From a geological standpoint, quadrangle Ac-H-10 Rongo shows a correlation between its two main geologic units (Platz et al., 2017) and the distribution of Mg-phyllosilicates, suggesting a link between geology and mineralogy in this area.

Item URL in elib:https://elib.dlr.de/114533/
Document Type:Article
Title:Mineralogical Analysis of Quadrangle Ac-H-10 Rongo on the Dwarf Planet Ceres
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Zambon, F.inaf-iaps, via del fosso del cavaliere 100, i-00133 rome, italyUNSPECIFIEDUNSPECIFIED
Carrozzo, F. G.inaf-iasf istituto di astrofisica spaziale e fisica cosmica, roma italyUNSPECIFIEDUNSPECIFIED
Tosi, F.inaf-iasf istituto di astrofisica spaziale e fisica cosmica, roma italyUNSPECIFIEDUNSPECIFIED
Ciarniello, M.inaf–iaps, istituto di astrofisica e planetologia spaziali, area di ricerca di tor vergata, via del fosso del cavaliere, 100, 00133 rome, italyUNSPECIFIEDUNSPECIFIED
Combe, J.-P.bear fight center, a columbus technologies and services inc. affiliate, p.o. box 667, 22 fiddler's road, winthrop, wa 98862, usaUNSPECIFIEDUNSPECIFIED
Frigeri, A.istituto di astrofisica e planetologia spaziali, istituto nazionale di astrofisica,via del fosso del cavaliere, 00133 roma, italyUNSPECIFIEDUNSPECIFIED
Desanctis, M.C.inaf, istituto di astrofisica spaziale e fisica cosmica, roma, italyUNSPECIFIEDUNSPECIFIED
Thangiam, G.Max Planck Institute for Solar System Research, Justus - von - Liebig - Weg 3, D - 37077 Göttingen, GermanyUNSPECIFIEDUNSPECIFIED
Nathues, A.max-planck institute for solar system research, katlenburg-lindau, germanyUNSPECIFIEDUNSPECIFIED
Hoffmann, M.max planck institute for solar system research , katlenburg-lindau, germanyUNSPECIFIEDUNSPECIFIED
Longobardo, Ainaf-laps, via del fosso del cavaliere 100, i-00133 rome, italyUNSPECIFIEDUNSPECIFIED
Stephan, KatrinKatrin.Stephan (at) dlr.deUNSPECIFIEDUNSPECIFIED
Raponi, A.inaf-iaps istituto di astrofisica e planetologia spaziali, rome, italyUNSPECIFIEDUNSPECIFIED
Ammannito, E.institute of geophysics and planetary physics, university of califor - nia at los angeles, los angeles, california, usaUNSPECIFIEDUNSPECIFIED
Krohn, Katrinkatrin.krohn (at) dlr.dehttps://orcid.org/0000-0001-8518-4985UNSPECIFIED
McFadden, L.A.nasa goddard space flight center, greenbelt, md 20770UNSPECIFIEDUNSPECIFIED
Palomba, E.inaf-iaps, rome, italyUNSPECIFIEDUNSPECIFIED
Raymond, C.A.jet propulsion laboratory, california institute of technology, pasadena, ca 91109-8099, usaUNSPECIFIEDUNSPECIFIED
Russell, C.T.institute of geophysics, university of california, los angeles, los angeles, ca 90095UNSPECIFIEDUNSPECIFIED
Date:2019
Journal or Publication Title:Icarus: International Journal of Solar System Studies
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:318
DOI:10.1016/j.icarus.2017.09.021
Page Range:pp. 212-229
Publisher:Elsevier
ISSN:0019-1035
Status:Published
Keywords:Dawn, Ceres
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - Project DAWN (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Geology
Deposited By: Stephan, Dr.rer.nat. Katrin
Deposited On:09 Oct 2017 13:30
Last Modified:05 Dec 2019 14:49

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