#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Venus 2: A Surface By Any Other Name…
Wednesday, March 15, 2023, 8:20 AM
Waterway Ballroom 5
Chairs:
Debra Buczkowski
Gabriel Eggers
Gabriel Eggers
Moderator:
Margaret Deahn
8:20 AM
Session Intorduction
8:25 AM
O'Hara S. T.*
McGovern P. J.
vonLembke D. W.
Constraints on Depth and Thickness of an Oblate Magma Chamber at Sapas Mons, Venus
[#2558]
Cracks on Sapas Mons / Magma chamber wide and flat / Collapsing inward.
Cracks on Sapas Mons / Magma chamber wide and flat / Collapsing inward.
8:35 AM
Hahn R. M.*
Byrne P. K.
Characterizing Styles of Volcano Gravitational Collapse on Venus
[#2190]
Volcanoes collapse / And create certain structures / What can they tell us?
Volcanoes collapse / And create certain structures / What can they tell us?
8:45 AM
Roberts E. K.*
Treiman A. H.
Eggers G. L.
Filiberto J.
Gina Crater Area, Venus: Multiple Overlapping Deformation and Volcanic Events Suggest Complex Active Tectonics
[#2870]
Tectonic and volcanic activity overlapped in time; deformation of Gina Crater implies recent events.
Tectonic and volcanic activity overlapped in time; deformation of Gina Crater implies recent events.
8:55 AM
Herrick R. R.*
Hensley S.
Direct Observation of Volcanic Activity on Venus from Repeat Magellan Imaging
[#1061]
A volcanic vent on Venus changed between Magellan Cycles 1 and 2.
A volcanic vent on Venus changed between Magellan Cycles 1 and 2.
9:05 AM
Panel Q&A
9:25 AM
Flynn I. T. W.*
Crown D. A.
Ramsey M. S.
Chevrel M. O.
Mapping and Modeling Venusian Lava Flows: Implications for Future Missions
[#1151]
There is much still to learn regarding the emplacement of Venusian lava flows. We seek to further our understanding through detailed mapping and modeling.
There is much still to learn regarding the emplacement of Venusian lava flows. We seek to further our understanding through detailed mapping and modeling.
9:35 AM
Eggers G. L.*
Filiberto J.
D'Incecco P.
Mari N.
Monaco C.
et al.
Spectroscopy of Mount Etna Lava Flows as a Proxy for Age: A Potential Analogue to Recent Volcanism on Venus
[#2480]
Weathered lava flows / Spectra can estimate age / But not so neatly.
Weathered lava flows / Spectra can estimate age / But not so neatly.
9:45 AM
D'Incecco P.*
Filiberto J.
Garvin J. B.
Arney G. N.
Getty S. A.
et al.
The Project “Analogs for VENus’ GEologically Recent Surfaces” (AVENGERS): A Comprehensive Database of Terrestrial Active Volcanoes for the Analysis of Ongoing Volcanism on Venus
[#2476]
The Project “Analogs for VENus’ GEologically Recent Surfaces” (AVENGERS) will analyze terrestrial analogs for the identification of active volcanism on Venus.
The Project “Analogs for VENus’ GEologically Recent Surfaces” (AVENGERS) will analyze terrestrial analogs for the identification of active volcanism on Venus.
9:55 AM
Nunes D. C.*
Smrekar S. E.
Hensley S.
Adeli S.
Andrews-Hanna J.
et al.
Seeking Venus on Earth: The VERITAS/DLR Analog Field Campaign
[#2319]
The VERITAS Science Team and DLR are planning a joint Iceland 2023 campaign to study Venus volcanic and tectonic analogs with airborne and in-situ measurements.
The VERITAS Science Team and DLR are planning a joint Iceland 2023 campaign to study Venus volcanic and tectonic analogs with airborne and in-situ measurements.
10:05 AM
Panel Q&A
10:25 AM
Kane S. R.*
Adams A. D.
Arney G.
Head J. W.
Kopparapu R.
et al.
Venus in the Context of Exoplanet Demographics
[#2443]
Venus lays the foundation for studying terrestrial planet evolution and habitability, and interpreting the substantial amount of exoplanet data.
Venus lays the foundation for studying terrestrial planet evolution and habitability, and interpreting the substantial amount of exoplanet data.
10:35 AM
Ganesh I.*
Gilmore M. S.
Detailed Magellan Radar Reflectivity Variations Within Sudenitsa Tessera, Venus
Venus
[#1847]
Venus tesserae / Do they vary place to place? / Can radar tell us?
Venus tesserae / Do they vary place to place? / Can radar tell us?
10:45 AM
Whitten J. L.*
Campbell B. A.
Characterizing the Impact of Crater Ejecta on the Surface Evolution of Tesserae
[#2849]
We analyze backscatter data derived from Magellan SAR and fitered by emissivity and the presence of crater ejecta in order to characterize the diversity of tesserae.
We analyze backscatter data derived from Magellan SAR and fitered by emissivity and the presence of crater ejecta in order to characterize the diversity of tesserae.
10:55 AM
Austin T. J.*
O'Rourke J. G.
Izenberg N.
Silber E. A.
Venus Airbursts: Implications for Global Resurfacing
[#2534]
The surface of Venus is covered in hundreds of large scars from meteor airbursts. We examine their spatial distribution in the context of global resurfacing.
The surface of Venus is covered in hundreds of large scars from meteor airbursts. We examine their spatial distribution in the context of global resurfacing.
11:05 AM
Panel Q&A
11:25 AM
Session Closure
*presenter