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May 28, 20260 citationsOpen Access

DUST ARCHITECTURES FOR MARS BASES: From Local Mitigations to Colony-Scale Dust Regimes and Self-Referential Dust Maintenance

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JMJosé Caetano de Mattos

Key Points

  • To develop a framework for understanding how dust affects Martian bases and provide strategies for mitigation.
  • Developed the Dust Architecture Model (DAM) and distinguished it from Local-Mitigation Dust Models (LMDM).
  • Formulated a coupled dynamical system linking dust forcing, base geometry, surface operations, and crew exposure.
  • Derived dust threshold conditions for the self-referential maintenance system.
  • Confirmed that a Mars base colony behaves as a self-referentially self-maintaining system regarding dust management.
  • Established three dust threshold conditions, indicating limits for filter overload (F*), wear accumulation (D*), and chronic health doses (X*).
  • Provided design guidelines for effective dust management including landing pad placement and traffic routing.

Abstract

Martian dust is pervasive, electrostatically active, abrasive, and potentially toxic. Current mitigation strategies are component-centric — better filters, seals, coatings, and cleaning systems — while planetary science studies global transport and storm dynamics. The critical intermediate scale — the colony as a coupled dust system — remains without a formal framework. We develop the Dust Architecture Model (DAM), introduce a Named Binary distinguishing Local-Mitigation Dust Models (LMDM) from Dust Architecture Models (DAM), and formalise the coupled dynamical system linking external dust forcing E(t), base geometry G, surface operations O(t), habitat internal environment H(t), and crew exposure state X(t). We prove that a Mars base colony is a self-referentially self-maintaining (SRSM) system in the dust domain: the maintenance mechanisms that manage dust (cleaning robots, filter systems, decontamination protocols) are themselves degraded by the dust they manage, creating an IRM feedback structure. By the IRM Impossibility Theorem, such a system cannot maintain zero dust impact growth without external reference — and the 'external reference' for a dust-SRSM system is architecture: base geometry and operational patterns that provide an exogenous structural constraint on the dust field, independent of the maintenance mechanism’s current state. We derive the three dust threshold conditions (filter overload F*, wear accumulation D*, and chronic health dose X*) as the IGT proximity functions for the dust-SRSM system, specify the Strongest Formulation in the four-part template, confirm structural invariance across open-pit mining, desert urban planning, cleanroom campus design, and the proposed Mars application, and provide a pre-registerable Collapse Counter-Scenario. Immediate design guidance is derived for landing pad placement, clean/dirty zoning, traffic corridor routing, and dust sink design.

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José Caetano de Mattos (2026) studied this question.

synapsesocial.com/papers/6a17dcbb3fad632b0f9d972fhttps://doi.org/10.5281/zenodo.20390804
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Also Consider

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  4. 4Validation of Martian dust storm trajectories in the Mars PCM using observational datasets2024
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