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Poster Session 1: Mars and Mars Sample Return
Tuesday, July 30, 2024, 5:30 PM
Marble Room
Nefedyev Y. A.*
Andreev A. O.
Physical Parameters of the Surface and Gravitational Field of Mars Based on Fractal Analysis Methods
[#6097]
In this work, the fractal dependencies for martian topographic model and anomalies of gravitational potential in both longitude and latitude are determined.
In this work, the fractal dependencies for martian topographic model and anomalies of gravitational potential in both longitude and latitude are determined.
Lai B. Y.
Long T.*
Che X. C.
Xie S. W.
Nemchin A. A.
Impact Event Recorded by U-Pb Ages of Phosphate Minerals in the Martian Metorite Northwest Africa 7397
[#6351]
Magnetite in NWA 7397 martian meteorite likely has a secondary origin. Ca-phosphate textures suggest late-stage magma differentiation. U-Pb dating indicates a resetting impact event, with magnetite formed from troilite desulphurization.
Magnetite in NWA 7397 martian meteorite likely has a secondary origin. Ca-phosphate textures suggest late-stage magma differentiation. U-Pb dating indicates a resetting impact event, with magnetite formed from troilite desulphurization.
Zhang X. R.*
Wang Y.
Zhao K.
Liao S. Y.
Petrology, U-Pb Chronology, and Geochemistry of the Enriched Shergottite Northwest Africa (NWA) 12564
[#6392]
We report the magmatic process, U-Pb chronology, and geochemical characteristics of the mantle source of the enriched shergottite NWA 12564.
We report the magmatic process, U-Pb chronology, and geochemical characteristics of the mantle source of the enriched shergottite NWA 12564.
Sefton-Nash E.
Graham H. V.
Herd C. D. K.
Carrier B. L.
Haltigin T.
et al.
Mars Sample Return (MSR) Sample Receiving Project (SRP) Measurement Definition Team (MDT-1): Overview and Status
[#6403]
Overview and report of the Mars Sample Return Sample Receiving Project Measurement Definition Team.
Overview and report of the Mars Sample Return Sample Receiving Project Measurement Definition Team.
Carrier B. L.
Graham H. V.
Herd C. D. K.
Sefton-Nash E.
Haltigin T.
et al.
Report of the Sample Receiving Project Measurement Definition Team: Deriving a Proposed Instrument Suite for the Sample Receiving Facility
[#6415]
Sample Receiving Project Measurement Definition Team: Deriving a proposed instrument suite and concept of operations for the Sample Receiving Facility.
Sample Receiving Project Measurement Definition Team: Deriving a proposed instrument suite and concept of operations for the Sample Receiving Facility.
Debaille V.*
Bridges J. C.
Herd C. D. K.
Duprat J.
Harrington A. D.
et al.
Report of the Sample Receiving Project Measurement Definition Team: Igneous Samples, Chronology, Cratering, and Dynamics Working Groups
[#6452]
Sample Receiving Project Measurement Definition Team (MDT): Igneous Samples, Chronology, Cratering, and Dynamics Working Groups.
Sample Receiving Project Measurement Definition Team (MDT): Igneous Samples, Chronology, Cratering, and Dynamics Working Groups.
Fortier V.*
Debaille V.
Dehant V.
Bultel B.
Laboratory Experiment Vs. Numerical Modeling in the Context of Hydrothermal Serpentinization on Mars
[#6419]
Laboratory experiment and numerical modelling are complementary methods to study complex geological systems. In this work, we plan to compare results from both methods in the context of hydrothermal serpentinizing systems in Mars-like coditions.
Laboratory experiment and numerical modelling are complementary methods to study complex geological systems. In this work, we plan to compare results from both methods in the context of hydrothermal serpentinizing systems in Mars-like coditions.
Almayrac M. G.*
Ruzié-Hamilton L.
Clay P. L.
Holland G.
Burgess R.
Homogeneity of Martian Mantle from Halogen Measurements in Shergottites
[#6444]
Here we will discuss insights into the halogen composition (Cl, Br and I) of the martian interior that can be accessed from the analysis of shergottite meteorites, whose parental magmas were formed by partial melting of martian mantle.
Here we will discuss insights into the halogen composition (Cl, Br and I) of the martian interior that can be accessed from the analysis of shergottite meteorites, whose parental magmas were formed by partial melting of martian mantle.
*presenter
