#LPSC2023
#LPSC2023

Program with Links to Abstracts
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Lunar Processes: Molten Mantle and Dynamic Dynamos
Monday, March 13, 2023, 2:15 PM
Waterway Ballroom 1
Chairs:
Yuanyuan Liang
Jeff Andrews-Hanna
Jeff Andrews-Hanna
Moderator:
Sonia Tikoo
2:15 PM
Session Introduction
2:20 PM
Schwinger S.*
Röhlen R.
Wiesner N.
Contribution of Impact Material to the Lunar Magma Ocean Liquid and Solid Cumulates
[#2025]
Where does material impacting the lunar magma ocean end up — in the solid cumulate or the magma liquid? And how does this affect mantle reservoir compositions?
Where does material impacting the lunar magma ocean end up — in the solid cumulate or the magma liquid? And how does this affect mantle reservoir compositions?
2:30 PM
Fu H.*
Jacobsen S. B.
Sedaghatpour F.
Timeline of Lunar Differentiation Recorded in Calcium and Magnesium Stable Isotopes
[#2400]
Ca and Mg stable isotope evidence revealed from lunar samples refines the timescale of the lunar differentiation to <10–30 or 30–150 million years.
Ca and Mg stable isotope evidence revealed from lunar samples refines the timescale of the lunar differentiation to <10–30 or 30–150 million years.
2:40 PM
Andrews-Hanna J. C.*
Evans A. J.
Mallik A.
Forming the Lunar Asymmetries
[#2507]
The lunar crustal and topographic asymmetry could have formed from a degree-one instability during magma ocean crystallization.
The lunar crustal and topographic asymmetry could have formed from a degree-one instability during magma ocean crystallization.
2:50 PM
Jones M. J.*
Evans A. J.
Fate of Th- and Ti-Bearing Lunar Magma Ocean Cumulates in the Aftermath of Major Basin-Forming Impacts
[#1750]
Oh, KREEP! where are you? / Hiding beneath the surface / Hugging the Moon’s core?
Oh, KREEP! where are you? / Hiding beneath the surface / Hugging the Moon’s core?
3:00 PM
Panel Q&A
3:20 PM
Scholpp J. S.*
Dygert N.
Hybridization of Lunar Mantle Sources by Garnet-Bearing Cumulates During Overturn Reconciles the REE, and Nd and Hf Isotopic Characteristics of High-Ti Basalts
[#1569]
Computational modeling of the impacts that lunar cumulate overturn and hybridization processes would have on REE and isotope compositions of mantle sources.
Computational modeling of the impacts that lunar cumulate overturn and hybridization processes would have on REE and isotope compositions of mantle sources.
3:30 PM
Ji D. J.*
Dygert N. D.
New Experimental Constraints on REE Partitioning Between Apatite and Silicate Melts and a Temperature and Composition-Dependent Predictive Partitioning Model
[#1255]
The work presents new apatite-melt partitioning experiments relevant to the lunar magma ocean and a predictive model for apatite-melt trace element partitioning.
The work presents new apatite-melt partitioning experiments relevant to the lunar magma ocean and a predictive model for apatite-melt trace element partitioning.
3:40 PM
Chaffee T.*
Tikoo S. M.
Abubo R.
Boeschen S. G.
Weiss B. P.
Testing Whether Lunar Melt Glasses Preserve Records of Impact-Generated Magnetic Fields
[#1741]
South Ray melt glasses / Do they record impact fields? / We put this to test.
South Ray melt glasses / Do they record impact fields? / We put this to test.
3:50 PM
Liang Y.*
Tikoo S. M.
Krawczynski M. J.
Experimentally Testing Whether Magmatic Processes Can Produce Strong Lunar Crustal Magnetism
[#2572]
Lunar magnetism / Attracts our lab to resolve / Abnormalities.
Lunar magnetism / Attracts our lab to resolve / Abnormalities.
4:00 PM
Panel Q&A
4:20 PM
Jung J.*
Tikoo S. M.
Burns D. H.
Exploring the Possible Origins of Magnetization Recorded in Apollo 11 Mare Basalts
[#1810]
We conducted paleomagnetic investigations on four Apollo 11 mare basalts to explore the possible origin of their magnetizations.
We conducted paleomagnetic investigations on four Apollo 11 mare basalts to explore the possible origin of their magnetizations.
4:30 PM
Zhou T.*
Tarduno J. A.
Cottrell R. D.
Neal C. R.
Nimmo F.
et al.
A Lunar Core Dynamo Limited to the Moon’s First 200 Million Years
[#2261]
New zero magnetic field measurements from Apollo samples as old as 4.3 Ga limits a strong, sustained lunar core dynamo to the Moon’s first 200 million years.
New zero magnetic field measurements from Apollo samples as old as 4.3 Ga limits a strong, sustained lunar core dynamo to the Moon’s first 200 million years.
4:40 PM
Vervelidou F.*
Shah J.
Eckley S.
Weiss B. P.
Zeigler R. A.
Evidence for Temporal Variability of the Lunar Dynamo
[#2369]
We conducted controlled-atmosphere, double-heating paleointensity analyses on three lunar regolith breccias of different assembly ages.
We conducted controlled-atmosphere, double-heating paleointensity analyses on three lunar regolith breccias of different assembly ages.
4:50 PM
Weiss B. P.*
Wieczorek M. A.
Gattacceca J.
Tikoo S. M.
McDonald C.
et al.
Evidence for a Long-Lived Lunar Dynamo from Magnetization in Apollo Samples and the Lunar Crust
[#1627]
The paleomagnetism of lunar rocks provides overwhelming evidence for a lunar dynamo lasting beyond 4.2 Ga ago and likely until at least 1.5 Ga ago.
The paleomagnetism of lunar rocks provides overwhelming evidence for a lunar dynamo lasting beyond 4.2 Ga ago and likely until at least 1.5 Ga ago.
5:00 PM
Panel Q&A
5:20 PM
Session Closure
*presenter