#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Chondritic Planetary Bodies and the Protoplanetary Disk
Thursday, March 16, 2023, 8:20 AM
Waterway Ballroom 6
Chairs:
Jangmi Han
Larry Nittler
Larry Nittler
Moderator:
Michael Zolensky
8:20 AM
Session Introduction
8:25 AM
Spitzer F.*
Burkhardt C.
Kleine T.
Hayabusa2 Initial Analysis Chem. Team
Hayabusa2-Initial-Analysis core
Ni Isotopic Composition of Ryugu Samples Returned by the Hayabusa2 Mission
[#2488]
The Ni isotopic composition of Ryugu is identical to that of CIs and different from all other CC and NC meteorites indicating a distinct formation region.
The Ni isotopic composition of Ryugu is identical to that of CIs and different from all other CC and NC meteorites indicating a distinct formation region.
8:35 AM
Kita N. T.*
Kitajima K.
Kawasaki N.
Nagashima K.
Sakamoto N.
et al.
High Precision SIMS Oxygen Isotope Analyses of Carbonates in Ryugu
[#1669]
We report high-precision SIMS oxygen three-isotope analyses of dolomite and breunnerite in Ryugu and address the evolution of aqueous fluid in the parent asteroid.
We report high-precision SIMS oxygen three-isotope analyses of dolomite and breunnerite in Ryugu and address the evolution of aqueous fluid in the parent asteroid.
8:45 AM
Nittler L. R.*
Barosch J.
Wang J.
Alexander C. M. O'D.
Water in Asteroid Ryugu is Deuterium-Rich Compared to Earth and CI Chondrites
[#1411]
Use oxygen ions / Measure Ryugu water / Deuterium-rich!
Use oxygen ions / Measure Ryugu water / Deuterium-rich!
8:55 AM
Aléon J.*
Mostefaoui S.
Bureau H.
Vangu D.
Khodja H.
et al.
An Exploration of Hydrogen Content in Magnetite from Asteroid Ryugu
[#1974]
H content of magnetite from asteroid Ryugu has been measured by NanoSIMS and was found to be correlated with Si content, morphology, and O isotopes.
H content of magnetite from asteroid Ryugu has been measured by NanoSIMS and was found to be correlated with Si content, morphology, and O isotopes.
9:05 AM
Panel Q&A
9:25 AM
Bose M.*
Root R. A.
Ryugu Particles Contain Sulfur in Multiple Oxidation States
[#2205]
Sulfur chemistry in Ryugu — rich.
Sulfur chemistry in Ryugu — rich.
9:35 AM
Verchovsky A. B.*
Feargus F. A. J.
Anand M.
Franch I. A.
Grady M. M.
et al.
Ryugu's Volalatiles Investigated Using Stepped Combustion and EGA Methods
[#2471]
The Hayabusa2 A0219 sample has been anlysed using stepped combustion and evoled gas analyses for C, N, and other common volatiles (H2O, H2, S and noble gases).
The Hayabusa2 A0219 sample has been anlysed using stepped combustion and evoled gas analyses for C, N, and other common volatiles (H2O, H2, S and noble gases).
9:45 AM
Cody G. D.*
Alexander C. M. O'D.
Foustoukos D. I.
Kebukawa Y.
The Evolution of Hydrogen Isotopes in Chondritic Insoluble Organic Solids
[#1506]
Reduction in D/H with molecular evolution of insoluble organic matter in CCs results from loss of aliphatic hydrogen and D-H exchange with D depleted water.
Reduction in D/H with molecular evolution of insoluble organic matter in CCs results from loss of aliphatic hydrogen and D-H exchange with D depleted water.
9:55 AM
Burton A. S.*
Berger E. L.
Investigating Amino Acid Heterogeneity in Milligram-Scale Samples of the Murchison CM2 Carbonaceous Chondrite
[#2484]
The extent of amino acid heterogeneity in multiple samples of the Murchison meteorite, all collected from the same 250-mg chip, were investigated.
The extent of amino acid heterogeneity in multiple samples of the Murchison meteorite, all collected from the same 250-mg chip, were investigated.
10:05 AM
Panel Q&A
10:25 AM
Caplan C. E.*
Dominguez G.
Gillis-Davis J. J.
McKeegan K. D.
Liu M. C.
Detection of Oxygen Implantation via Electron Irradiation of Water Ice on Silicon Using AFM-IR Techniques
[#2430]
Water-ice-covered silicon wafers were electron irradiated to understand the heterogenous nature of oxygen implantation using AFM-IR to improve SIMS measurements.
Water-ice-covered silicon wafers were electron irradiated to understand the heterogenous nature of oxygen implantation using AFM-IR to improve SIMS measurements.
10:35 AM
Yang X.*
Ciesla F. J.
Heck P. R.
Quantification of the High Early Solar Activity Using Cosmogenic Neon Nuclides in Meteoritic Minerals
[#1344]
The protosun has been thought to be highly active but not well-constrained. Here we provide an improved estimate of the young Sun’s activity with a new model.
The protosun has been thought to be highly active but not well-constrained. Here we provide an improved estimate of the young Sun’s activity with a new model.
10:45 AM
Asphaug E.*
Hysteretic Evolution of Accreting Planetary Interiors
[#1686]
Why meteorites / Are so weird may be due to / Hysteretic growth.
Why meteorites / Are so weird may be due to / Hysteretic growth.
10:55 AM
Estrada P. R.*
Umurhan O. M.
Can the Streaming Instability Form the First Planetesimals in Globally Turbulent Protoplanetary Disks?
[#2950]
We explore whether conditions for the SI can realistically be achieved within the first million years of a globally turbulent protoplanetary disk.
We explore whether conditions for the SI can realistically be achieved within the first million years of a globally turbulent protoplanetary disk.
11:05 AM
Panel Q&A
11:25 AM
Session Closure
*presenter