Published December 9, 2025 | Version v1
Technical note Open

First Fully Autochthonous Chemical Propulsion System for Mars Ascent: Design, Analysis, and ISRU Production Pathways

  • 1. Independent Researcher

Description

ABSTRACT

Mars Sample Return and human exploration architectures require reliable 
Mars Ascent Vehicle (MAV) systems capable of achieving surface-to-orbit 
trajectories (~4.4 km/s ΔV). Current concepts rely on Earth-supplied 
propellants or partial In-Situ Resource Utilization (ISRU), introducing 
mass penalties, mission risk, and long-term sustainability challenges.

This paper presents the Martian Propellant Matrix (MPM) v3.1, the first 
complete chemical propulsion system producible entirely from Martian 
resources with zero reliance on imported nitrogen-based propellants. 
The architecture integrates four synergistic propulsion subsystems:

(1) MMT-1B: A perchlorate-magnesium solid booster (Isp 245s, 48 kN) 
    for high-thrust surface departure
(2) ANUBIS-M: A methane-oxygen upper stage (Isp 360s, 30 kN) for 
    orbital insertion via Sabatier reaction
(3) H₂O₂-RCS: A hydrogen peroxide monopropellant system (Isp 160s) 
    for attitude control with flight heritage from X-15 and Dream Chaser
(4) TSF-4R: A perchlorate-carbon hybrid (Isp 235s, 15 kN) for abort 
    and emergency maneuvers

Complete mission analysis demonstrates that a 1000 kg dry mass MAV 
requires 2178 kg of propellant, achievable through ISRU processing 
of ~200 tonnes of perchlorate-bearing regolith, atmospheric CO₂ 
capture, and water ice electrolysis. Total energy budget is 16.6 MWh, 
enabling 69-day production cycles with a single 10 kWe Kilopower reactor.

The system achieves a Technology Readiness Level (TRL) assessment of 
7.25/9 through substitution of experimental components (molten perchlorate 
monopropellants, elemental sulfur processing) with validated alternatives 
(H₂O₂ catalytic decomposition, Bosch carbon reduction). This represents 
a 37.6% reduction in energy requirements and elimination of three 
high-temperature (>1000°C) industrial processes compared to earlier 
architectures.

Key innovations include: (1) complete elimination of hydrazine and 
nitrogen-bearing compounds, (2) magnesium-based solid propellants 
requiring 27% less refining energy than aluminum equivalents, and 
(3) unified ISRU supply chains leveraging the same feedstocks 
(perchlorates, CO₂, H₂O) across all subsystems.

Critical validation requirements are identified: experimental 
characterization of Mg/Mg(ClO₄)₂ combustion kinetics, demonstration 
of perchlorate extraction at industrial scale (3.3 tonnes/day regolith 
processing), and thermal-vacuum testing of cryogenic methane storage 
under Martian thermal cycling (-140°C to +20°C).

This work provides a complete reference implementation with open-source 
Python codebase for mission planning, propellant production modeling, 
and performance analysis. The MPM v3.1 architecture represents a viable 
pathway toward sustainable Mars surface operations and reduces Mars 
Sample Return mission mass by an estimated 2-3 tonnes compared to 
Earth-supplied propellant baselines.

KEYWORDS: Mars ISRU, chemical propulsion, Mars Ascent Vehicle, 
perchlorate propellants, methane-oxygen engines, Sabatier reaction, 
sustainable space exploration

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