#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Poster Session: Giant Planet System Potpourri
Wednesday, March 15, 2023, 6:30 PM
iPosters/Gather.town
Mandt K. E.*
Mousis O.
Simon A.
Hofstadter M.
Do Juno MWR Results Invalidate Galileo Probe Noble Gas and Isotope Measurements? — CANCELED
[#1197]
Nitrogen isotopes and noble gas abundances, critical for determining the origin of the ice giants, can be measured reliably with a single atmospheric probe.
Nitrogen isotopes and noble gas abundances, critical for determining the origin of the ice giants, can be measured reliably with a single atmospheric probe.
Struck J.-T.*
Solar System Planetary Debris Flow
[#2602]
Solar system planetary debris flow can be studied to protect satellites from injury and harm.
Solar system planetary debris flow can be studied to protect satellites from injury and harm.
Bradak B.*
Kimura J.
Gomez C.
Introduction to Dione`s Wispy Terrain, as a Putative Model Region for Wilson-Cycles on Icy Satellites
[#1178]
The relationship between impact craters and tectonic features on Wispy Terrain (Dione) may indicate compression and theoretically, subsumption-like processes.
The relationship between impact craters and tectonic features on Wispy Terrain (Dione) may indicate compression and theoretically, subsumption-like processes.
Vidmachenko A. P.*
Steklov O. F.
Summer is Coming Soon on Saturn’s Moon Titan
[#1095]
Summer in Titan’s S-hemisphere will lead to methane rain and fill seas. In 2023–2030 IR observations on large telescopes will confirm hypothesis on Titan’s seasons.
Summer in Titan’s S-hemisphere will lead to methane rain and fill seas. In 2023–2030 IR observations on large telescopes will confirm hypothesis on Titan’s seasons.
Vashist A. S.*
Heslar M.
Barnes J. W.
Hennen C.
Lorenz R. D.
Titan’s North-South Asymmetry at Visible Wavelengths over the Cassini Mission
[#2030]
We observe a near-complete boundary latitude transition, a 3-year loss in albedo contrast, and a tilt of Titan’s NSA using VIMS cubes taken from 2004 to 2017.
We observe a near-complete boundary latitude transition, a 3-year loss in albedo contrast, and a tilt of Titan’s NSA using VIMS cubes taken from 2004 to 2017.
Naseem M.*
Neveu M.
Howell S.
Lesage E.
Daswani M. M.
et al.
Salt Distribution from Freezing Intrusions in Ice Shells on Ocean Worlds
[#1672]
Understanding the influence of compositional heterogeneities on transport through ice shells through numerical modeling of freezing intrusions.
Understanding the influence of compositional heterogeneities on transport through ice shells through numerical modeling of freezing intrusions.
Leeseberg P. R.*
Nixon C. A.
Thelen A. E.
Cordiner M. A.
Searching for C4H3N Isomers on Titan Using ALMA
[#2585]
Methylcyanoacetylene was recently discovered on Titan, prompting an investigation of the other structural isomers of C4H3N.
Methylcyanoacetylene was recently discovered on Titan, prompting an investigation of the other structural isomers of C4H3N.
Li J.*
Li C.
Sulfur Chemistry on the Surface Ice of Europa
[#1317]
We show that sulfuric acid is the dominant species on the surface of Europa and sulfur chemistry may play an important role in the formation of O2.
We show that sulfuric acid is the dominant species on the surface of Europa and sulfur chemistry may play an important role in the formation of O2.
Goossens S.*
van Noort B. G.
Mateo Aguaron A.
Mazarico E.
van der Wal W.
Enceladus Gravity and Titan Gravity and Tides from Cassini Tracking Data
[#1528]
Analysis of Cassini tracking data for Enceladus and Titan gravity and tides, with results consistent with earlier analysis but a lower Love number for Titan.
Analysis of Cassini tracking data for Enceladus and Titan gravity and tides, with results consistent with earlier analysis but a lower Love number for Titan.
Klaiber L.*
Thomas N.
Marschall R.
Three Dimensional Modeling of the Dynamics of Io’s Atmosphere
[#2609]
We are presenting a 3D numerical model of the dynamics of Io’s atmosphere and the interaction of various atmospheric processes.
We are presenting a 3D numerical model of the dynamics of Io’s atmosphere and the interaction of various atmospheric processes.
Vidmachenko A. P.*
Steklov O. F.
On Seasonal Growth of Geyser Activity in the South Polar Region of Enceladus
[#1096]
In 2024 Enceladus will transit to summer in S-hemisphere. Therefore observations on large telescopes in 2023–2030 should find an increase in geyser activity.
In 2024 Enceladus will transit to summer in S-hemisphere. Therefore observations on large telescopes in 2023–2030 should find an increase in geyser activity.
*presenter