#LPSC2023
#LPSC2023
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The Importance of Sample Return: ANGSA and Chang'E
Friday, March 17, 2023, 8:20 AM
Waterway Ballroom 1
Chairs:
Cordula Haupt
Timmons Erickson
Timmons Erickson
Moderator:
Susana Hoyos
8:20 AM
Session Introduction
8:25 AM
Neuman M.*
Koefoed P.
Wang K.
Jolliff B. L.
Korotev R. L.
et al.
Composition of Apollo 17 Double Drive Tube 73001 / 73002
[#1625]
We determined the bulk chemistry of every 0.5-cm interval of Apollo 17 double drive tube 73001/73002 and used the data to model major lithologic components.
We determined the bulk chemistry of every 0.5-cm interval of Apollo 17 double drive tube 73001/73002 and used the data to model major lithologic components.
8:35 AM
Valenciano J. L.*
Neal C. R.
Shearer C. K.
ANGSA Science Team
Chemical Stratigraphy of Apollo 17 Drive Tube 73001
[#2141]
An investigation of the regolith found in Apollo 17 drive tube 73001.
An investigation of the regolith found in Apollo 17 drive tube 73001.
8:45 AM
Shearer C. K.*
Simon S. B.
Dottin J.
Cato M.
McCubbin F. M.
et al.
Investigating Pyroclastic Volcanism in the Taurus-Littrow Valley (TLV) Using The Station 3 Double Drive Tube 73001-73002
[#1773]
Pyroclastic volcanism is represented in the regolith and regolith breccias sampled in the TLV at Station 3. What new perspectives do these samples provide?
Pyroclastic volcanism is represented in the regolith and regolith breccias sampled in the TLV at Station 3. What new perspectives do these samples provide?
8:55 AM
Jolliff B. L.*
Carpenter P. K.
Yen C. J.-K.
Neuman M. D.
Ogliore R. C.
et al.
In Search of Tycho Ejecta in Apollo 17 Double Drive Tube 73001/2 Using Continuous Core Thin Section Quantitative Analysis
[#1818]
Searching for distinctive Tycho ejecta / In 73001/2 double drive tube, recently opened / Low FeO and HCP > LCP, still looking; haven’t found it yet.
Searching for distinctive Tycho ejecta / In 73001/2 double drive tube, recently opened / Low FeO and HCP > LCP, still looking; haven’t found it yet.
9:05 AM
Panel Q&A
9:25 AM
Elsila J. E.*
Aponte J. C.
Dworkin J. P.
Glavin D. P.
McLain H. L.
et al.
Organic Compounds and Cyanide in the Apollo 17 Specially Curated ANGSA Samples
[#1640]
Low levels of organic compounds are present in the ANGSA core and frozen samples. Volatile compounds may be better preserved under sealed curation conditions.
Low levels of organic compounds are present in the ANGSA core and frozen samples. Volatile compounds may be better preserved under sealed curation conditions.
9:35 AM
Erickson T. M.*
Simon J. I.
Christoffersen R. G.
Shearer C.
Hahn T.
et al.
Microstructural Characterization of Felsite Fragments from the Apollo Next Generation Sample Analysis (ANGSA) Double Drive Tube 73001/73002
[#1666]
We will present coordinated SEM, CL, EBSD, EPMA, and TEM data from evolved fragments within the ANGSA Double Drive Tube 73001/73002.
We will present coordinated SEM, CL, EBSD, EPMA, and TEM data from evolved fragments within the ANGSA Double Drive Tube 73001/73002.
9:45 AM
Guo Z.*
Li C.
Li Y.
Wen Y.
Wu Y.
et al.
Impact-Induced Formation of Sub-Microscopic Magnetite Within Chang’E-5 Sulfide Grains
[#1130]
Magnetite is rarely present on the Moon, and submicroscopic magnetite formed by eutectic reaction during the impact process was observed in Chang’E-5 lunar soil.
Magnetite is rarely present on the Moon, and submicroscopic magnetite formed by eutectic reaction during the impact process was observed in Chang’E-5 lunar soil.
9:55 AM
Ling Z. C.*
Cao H. J.
Jolliff B. L.
Wang A.
Chen J.
et al.
Raman Spectroscopic Characterization of Chang'E-5 Drilled Subsurface Soil CE5Z0107
[#1904]
We investigate the mineral modes and geochemistry of the subsurface soil CE5Z0107 and make comparisons with those of the surface soil sample CE5C0600.
We investigate the mineral modes and geochemistry of the subsurface soil CE5Z0107 and make comparisons with those of the surface soil sample CE5C0600.
10:05 AM
Panel Q&A
10:25 AM
Li Y. H.*
Wang Z. C.
Zhang W.
Zhou L.
Zong K. Q.
et al.
Rb-Sr Systematics of Chang’E-5 Lunar Soils and Records of Complex Thermal Modification
[#1783]
We in-situ analyzed Rb-Sr isotope of basaltic/mineral fragments in CE-5 lunar soil and the results record a complex thermal modification history.
We in-situ analyzed Rb-Sr isotope of basaltic/mineral fragments in CE-5 lunar soil and the results record a complex thermal modification history.
10:35 AM
Hoyos S. H.*
Grove T. L. G.
Petrogenesis of the Chang’E-5 Mare Basalts: Implications for the Origin of the Youngest Sampled Lunar Magmas
[#1858]
We have conducted crystallization experiments on the most primitive Chang’E 5 basalts to constrain the Moon’s thermal and magmatic evolution during the last 2 Ga.
We have conducted crystallization experiments on the most primitive Chang’E 5 basalts to constrain the Moon’s thermal and magmatic evolution during the last 2 Ga.
10:45 AM
Haupt C. P.*
Renggli C. J.
Klaver M.
Steenstra E.
Berndt J.
et al.
Experimental and Petrological Investigations into the Origin of the Lunar Change'5 Basalts
[#1059]
We present results of high-P and high-T experiments on Chang’E 5 basalt compositions to decipher their origin and understand young lunar volcanic activity.
We present results of high-P and high-T experiments on Chang’E 5 basalt compositions to decipher their origin and understand young lunar volcanic activity.
10:55 AM
Elardo S. M.*
Cone K. A.
Williams S. J.
Palin R. M.
A Shallow Mantle Source for the Chang'E 5 Basalts Indicates Prolonged Indirect Heating of the Upper Mantle by KREEP
[#2624]
Phase equilibrium experiments show that the young evolved basalt returned by Chang’E 5 was likely derived from a shallow source heated indirectly by KREEP.
Phase equilibrium experiments show that the young evolved basalt returned by Chang’E 5 was likely derived from a shallow source heated indirectly by KREEP.
11:05 AM
Panel Q&A
11:25 AM
Session Closure
*presenter