#LPSC2023
#LPSC2023

Program with Links to Abstracts
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Poster Session: Impact Potpourri
Wednesday, March 15, 2023, 6:30 PM
iPosters/Gather.town
Shahi N.*
Osinski G. R.
Hydrothermal Alteration Features at the Lac Couture Impact Structure, Canada
[#2495]
The abstract discusses hydrothermal alterations in samples from the Lac Couture impact structure and aims to improve our understanding of such systems on Mars.
The abstract discusses hydrothermal alterations in samples from the Lac Couture impact structure and aims to improve our understanding of such systems on Mars.
Wren P. F.*
Fevig R. A.
Improved Constraints on Main Belt Binary Asteroid Systems Based on Ceres Doublet Impacts
[#2133]
Expanded Ceres doublet crater study and added computational experimentation to improve constraints on the number and sizes of binary asteroids in the main belt.
Expanded Ceres doublet crater study and added computational experimentation to improve constraints on the number and sizes of binary asteroids in the main belt.
Harris T. H. S.*
Indochinite Tektite Suborbital Assessment
[#1333]
Steep first-way reentry angles and rapidly tumbling, irregular shapes reduce or eliminate reentry ablation, consistent with N. hemisphere source east of Indochina.
Steep first-way reentry angles and rapidly tumbling, irregular shapes reduce or eliminate reentry ablation, consistent with N. hemisphere source east of Indochina.
Meador J.
Stooke P. J.*
Apollo 16 Lunar Module Ascent Stage Impact
[#1025]
Orbit modelling suggests the Apollo 16 LM ascent stage crashed near 10 N, 104 E on 29 May 1972. A candidate impact structure is identified at 9.99 N, 104.26 E.
Orbit modelling suggests the Apollo 16 LM ascent stage crashed near 10 N, 104 E on 29 May 1972. A candidate impact structure is identified at 9.99 N, 104.26 E.
Ferrari F.*
Topputo F.
Merisio G.
Franzese V.
Buonagura C.
et al.
The LUMIO CubeSat: Detecting Meteoroid Impacts on the Lunar Farside
[#1456]
LUMIO is a ESA mission aimed at detecting meteoroid impact flashes on the lunar farside. The goal is to refine the meteoroid environment model in the Earth-Moon system.
LUMIO is a ESA mission aimed at detecting meteoroid impact flashes on the lunar farside. The goal is to refine the meteoroid environment model in the Earth-Moon system.
Sharini K. S.*
Osinski G. R.
Impact Melt Distribution in Copernicus Crater on the Moon
[#2176]
Distribution of impact melt units — ponds, flows, channels and veneers in Copernicus crater.
Distribution of impact melt units — ponds, flows, channels and veneers in Copernicus crater.
Harris T. H. S.*
Indochinite Tektite Post-Solidus Alteration
[#1331]
Indochinite tektites exhibit post-solidus alteration indicated by surface texture and morphometric trends consistent with disruption by high-voltage arcing.
Indochinite tektites exhibit post-solidus alteration indicated by surface texture and morphometric trends consistent with disruption by high-voltage arcing.
Sharini K. S.*
Kimi K. B.
Harish
Tuhi S.
Priya R. K. S.
et al.
Modification of Craters in Mare Nectaris on the Moon
[#2555]
Modification of craters (Fracastorius, Beaumont, Bohnenberger and Daguerre) located in the mare-highland boundary of the Nectaris basin.
Modification of craters (Fracastorius, Beaumont, Bohnenberger and Daguerre) located in the mare-highland boundary of the Nectaris basin.
Tada T.*
Kurosawa K.
Isa J.
Ono H.
Hamann C.
et al.
Shock Recovery of Granite: Implications for Feather Features Formation
[#2630]
Shock recovery experiments of granite were conducted to investigate the formation of feather features in quartz.
Shock recovery experiments of granite were conducted to investigate the formation of feather features in quartz.
Minde P.*
A Possible Distal Exposure of the Vakkejokk Impact Ejecta Layer Suggesting Emplacement as Fluidized Ejecta
[#1018]
A breccia exposure, at Roggenjarga peninsula in Lake Torneträsk, Here reported as an distal impactite layer likely linked to the Vakkejokk impact structure.
A breccia exposure, at Roggenjarga peninsula in Lake Torneträsk, Here reported as an distal impactite layer likely linked to the Vakkejokk impact structure.
Trnka M.*
Skála R.
Pecková E.
Venclová S.
Extremely Large Moldavite from Byňov near Nové Hrady (Southern Bohemia): Importance of Source Rock Chemical Composition in the Formation of Muong Nong Type Moldavites
[#1191]
Splash form and Muong Nong-type moldavites were formed from slightly different sediments producing melts of different viscosities under the same PT conditions.
Splash form and Muong Nong-type moldavites were formed from slightly different sediments producing melts of different viscosities under the same PT conditions.
Misra S.*
Newsom H. E.
Ray D.
Involvement of Archaean Basement in Formation of Impact-Melt Bombs from Lonar Crater, India: A Geochemical Hypothesis Originated from Anthropogenic Samples
[#1236]
The model of involvement of Archaean basement in the composition of the Lonar impact-melt bomb is originated from geochemical analyses of anthropogenic brick samples.
The model of involvement of Archaean basement in the composition of the Lonar impact-melt bomb is originated from geochemical analyses of anthropogenic brick samples.
Molnár M.
Ventura K.
Poßekel J.
Ernstson K.*
The Kolešovice 20 km-Diameter Structure (Czech Republic): Evidence of an Airburst Impact Crater
[#1428]
Digital terrain model analyses, geology, and geophysics establish a new 20-km-diameter impact structure of Cretaceous-Tertiary age in the Czech Republic.
Digital terrain model analyses, geology, and geophysics establish a new 20-km-diameter impact structure of Cretaceous-Tertiary age in the Czech Republic.
Keilmann J. U.
Poßekel J.
Ernstson K.*
End Moraine VS. Impact Event: The Cloppenburg (Northern Germany) Peak Ring Structure and the Ice Age Paradox
[#1438]
A 100-km large terminal moraine landscape of the Saale Ice Age turns out to be a large peak-ring impact structure according to digital terrain model analyses.
A 100-km large terminal moraine landscape of the Saale Ice Age turns out to be a large peak-ring impact structure according to digital terrain model analyses.
Aswathi J.*
Saranya R. C.
James S.
Devika P.
Sajinkumar K. S.
PSInSAR as a New Tool to Monitor Subsidence of Ramgarh Crater
[#2794]
This paper describes a remote sensing technique called PSInSAR that was applied to detect the subsidence and displacement of Ramgarh Crater.
This paper describes a remote sensing technique called PSInSAR that was applied to detect the subsidence and displacement of Ramgarh Crater.
Moore R. B.*
Addressing Challenges to Progress on a Previously Proposed Southern Mt Lofty Ranges Multiple Impact
[#2835]
Part of a wider study concerning surface processes associated with oblique impacts.
Part of a wider study concerning surface processes associated with oblique impacts.
Fischer-Gödde M.*
Tusch J.
Goderis S.
Bragagni A.
Mohr-Westheide T.
et al.
Ruthenium Isotope Composition of Terrestrial Impact Rocks — A New Tool for Deducing Genetic Signatures of Meteoritic Projectiles
[#2313]
We report the first nucleosynthetic ruthenium isotope anomlies for terrestrial impact rocks. The anomalies represent genetic fingerprints of the projectiles.
We report the first nucleosynthetic ruthenium isotope anomlies for terrestrial impact rocks. The anomalies represent genetic fingerprints of the projectiles.
Tada T.*
Tada R.
Carling P. A.
Songtham W.
Thuyen L. X.
et al.
Location of the Australasian Tektite Impact Event Based on Distribution of the Ejecta Deposits in the Eastern Indochina
[#2606]
The location of the Australasian tektite impact event was estimated based on the thickness distribution of the ejecta deposit across eastern Indochina.
The location of the Australasian tektite impact event was estimated based on the thickness distribution of the ejecta deposit across eastern Indochina.
Ivanov M. A.*
Head J. W.
Hiesinger H.
Absolute Model Age Estimates of the Fecunditatis Basin and Mare Fecunditatis in the Region of Luna-16 Landing Site
[#1233]
The AMA of ~4.45 Ga characterizes the area (~115 × 115 km) around the landing site.
The AMA of ~4.45 Ga characterizes the area (~115 × 115 km) around the landing site.
Samaddar T.*
Mehar J.
Investigation of Physical Properties of Lunar Crater Facies Using Radar Imagery
[#3015]
To identify and characterize specific crater facies units such as rough boulder units, impact melts, and melt flows using Mini-RF radar data.
To identify and characterize specific crater facies units such as rough boulder units, impact melts, and melt flows using Mini-RF radar data.
Horzempa P.*
Imbrium Double Basin
[#2730]
The structure of the Imbrium basin on the Moon can best be explained by two separate impact events.
The structure of the Imbrium basin on the Moon can best be explained by two separate impact events.
Horzempa P.*
Discovery of Small SPA Lunar Impact Basin
[#2971]
The Lyman-Langmuir basin has been discovered on the farside of the Moon. It is located in the northern sector of the SPA basin region.
The Lyman-Langmuir basin has been discovered on the farside of the Moon. It is located in the northern sector of the SPA basin region.
Watters W. A.*
Fassett C. I.
Shape Distribution and Modification Sequence of Simple Craters in Lunar Maria
[#2773]
Profile and planform crater shape parameters were measured to characterize the modification sequence and test a linear diffusion model.
Profile and planform crater shape parameters were measured to characterize the modification sequence and test a linear diffusion model.
Pathak S.*
Sen R.
Moitra H.
Bhattacharya S.
Gupta S.
Compositional Diversity Within Class-1 Lunar Floor-Fractured Crater Cardanus
[#1380]
In this study, an attempt has been made to infer the compositional variability within the Cardanus Crater, a class-1 lunar FFC, in a spatial context.
In this study, an attempt has been made to infer the compositional variability within the Cardanus Crater, a class-1 lunar FFC, in a spatial context.
Patel D. D.*
Patel S. M.
Solanki P. M.
Compositional and Morphological Study of Rutherfurd Crater
[#2581]
We study the composition and morphology of the Rutherfurd crater located on the lunar nearside from the Moon Mineralogy Mapper and Narrow Angle Camera data.
We study the composition and morphology of the Rutherfurd crater located on the lunar nearside from the Moon Mineralogy Mapper and Narrow Angle Camera data.
*presenter