S. Lea‐Wurzbach’s research while affiliated with Imperial College London and other places

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Publications (1)


Approximate chronostratigraphic charts of the four terrestrial planets and key events. Earth time scale from International Chronostratigraphic Chart v2021/10. Mars time scale from Platz et al. (2013). Mercury time scale from Banks et al. (2017) and Thomas et al. (2014). * = A geological timescale for Venus was proposed by Ivanov and Head (2015) and was reviewed and updated by Head et al. (2023).
Venusian Highlands and the BAT Province, a broadly triangular region bound by the Parga, Devana and Hecate (and Ganis) Chasmata, where RDRs are concentrated and evidence of mature or incipient triple–junction rifting. Red dotted lines indicate the position of rifts in the BAT vicinity (simplified from Guseva (2016) and observations from Magellan altimetry). Regiones have been color–coded using the classification of Stofan et al. (1995), who suggest that RDRs and CDRs exist in a continuum.
Triple Junction Rifting: Afar (Earth) compared with Atla Regio (Venus). Left: Afar rifting, with flood basalts in blue simplified from Ayalew et al. (2021) and rift zones in yellow with red dashed axial trace simplified from Macgregor (2015). Right: Atla Regio rifting, with significant lava flows in blue (simplified from this study) and rift zones in yellow with red dashed axial trace.
(a) Regional geological map of the area around Atla Regio, with units simplified from Ivanov and Head (2011), coronae, volcanoes and landing sites from Airey et al. (2016), VMC hotspots from Shalygin et al. (2015), Parabolic Radar‐Dark Halo impact craters were extracted in this study; and (b) Left‐Look SAR image close‐up with summary map of the major volcanic centers and their lava aprons, with Tara and Aeronwen representing unnamed intermediate sized shield volcanoes, first described in Klidaras and Mason (2022).
Detailed geological map of Atla Regio including Sapas Mons and extending along Dali Chasma down to Ongwuti Mons and Nyingo Fluctus.

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Evolution of Plume Volcanism at Atla Regio, Venus
  • Article
  • Full-text available

February 2025

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111 Reads

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A. Klidaras

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D. Cirium

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S. Lea‐Wurzbach

Atla Regio is a large topographic rise, at the equator of Venus, considered to sit above a young mantle upwelling. Hosting several giant shield volcanoes, including Maat Mons, it is a strong candidate for recent eruptive activity. Through detailed analysis of material units and structures at Ozza, Maat and Sapas Mons, northern Dali Chasma and the surrounding plains, we have unraveled the tectono‐magmatic evolution at Atla Regio. Lithostratigraphic analysis, of the volcanic styles, lava flow relationships, rift–associated shield clusters, graben‐fissure systems and pit cratering, in relation to the regional plains and other older features, has enabled the establishment of a model of the evolution of volcanism. Structural analysis reveals that graben‐fissure systems at Ozza Mons transition outward into three major rifts, and two new, unnamed volcanoes are identified. Our model is evidenced by analysis of lava flow stratigraphy and cross‐cutting relationships with respect to the stratigraphic marker provided by the ejecta halo of the Uvaysi impact, and using sound stratigraphic principles. A relative chronostratigraphic framework for the area around Ozza and Maat Mons has thus been constructed, and our findings are in agreement with prior research. A new regional history is proposed here, where volcanism was initially concentrated along Dali Chasma, before plume volcanism took over at Ozza Mons and finally, Maat Mons became the most recent locus of volcanism. We propose that the pattern of large shield volcanoes with displaced centers here is indicative of minor crustal adjustments above a relatively long‐lived mantle plume.

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