Planetary Exploration 3.0: A Roadmap for Software-Defined, Radically Adaptive Space Systems
Masahiro Ono, Daniel Selva, Morgan L. Cable, Marie Ethvignot, Margaret Hansen, Andreas M. Hein, Elena-Sorina Lupu, Zachary Manchester, David Murrow, Chad Pozarycki, Pascal Spino, Amanda Stockton, Mathieu Choukroun, Soon-Jo Chung, John Day, Alexander Demagall, Anthony Freeman

TL;DR
This paper advocates for a new paradigm in planetary exploration, PE 3.0, emphasizing software-defined, adaptable space systems for efficient, resilient missions to distant worlds.
Contribution
It introduces the PE 3.0 framework, highlighting the role of software-defined systems and adaptive technologies for exploring outer Solar System bodies with fewer missions.
Findings
PE 3.0 enables in situ data-driven science evolution.
Key technologies include reconfigurable hardware and AI onboard.
Three innovative mission concepts are proposed.
Abstract
The surface and subsurface of worlds beyond Mars remain largely unexplored. Yet these worlds hold keys to fundamental questions in planetary science - from potentially habitable subsurface oceans on icy moons to ancient records preserved in Kuiper Belt objects. NASA's success in Mars exploration was achieved through incrementalism: 22 progressively sophisticated missions over decades. This paradigm, which we call Planetary Exploration 2.0 (PE 2.0), is untenable for the outer Solar System, where cruise times of a decade or more make iterative missions infeasible. We propose Planetary Exploration 3.0 (PE 3.0): a paradigm in which unvisited worlds are explored by a single or a few missions with radically adaptive space systems. A PE 3.0 mission conducts both initial exploratory science and follow-on hypothesis-driven science based on its own in situ data returns, evolving spacecraft…
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