Venus Life Finder Habitability Mission: Motivation, Science Objectives, and Instrumentation
Sara Seager, Janusz J. Petkowski, Christopher E. Carr, Sarag J., Saikia, Rachana Agrawal, Weston P. Buchanan, David H. Grinspoon, Monika U., Weber, Pete Klupar, Simon P. Worden, Iaroslav Iakubivskyi, Mihkel Pajusalu,, Laila Kaasik (for the VLF Collaboration)

TL;DR
This paper proposes an astrobiology-focused Venus atmospheric mission with advanced instruments to assess habitability, detect biosignatures, and inform future sample return efforts in the planet's cloud layers.
Contribution
It introduces a comprehensive instrument suite and mission concept for in situ analysis of Venus's clouds to evaluate habitability and search for signs of life.
Findings
Measurement of cloud particle acidity and water content
Detection of metals, organics, and biosignature gases
Assessment of cloud particle heterogeneity
Abstract
For over half a century, scientists have contemplated the potential existence of life within the clouds of Venus. Unknown chemistry leaves open the possibility that certain regions of the Venusian atmosphere are habitable. In situ atmospheric measurements with a suite of modern instruments can determine whether the cloud decks possess the characteristics needed to support life as we know it. The key habitability factors are cloud particle droplet acidity and cloud-layer water content. We envision an instrument suite to measure not only the acidity and water content of the droplets (and their variability) but additionally to confirm the presence of metals and other non-volatile elements required for life's metabolism, verify the existence of organic material, and search for biosignature gases as signs of life. We present an astrobiology-focused mission, science goals, and instruments…
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