The Interplanetary Habitable Zone
The concept of a system-wide measure of the sustainment of life (habitability) for space-faring interplanetary species is introduced and explored.
Although largely agnostic to the details of how interplanetary life might operate (e.g., via technology or by utilizing organism traits that are, as of now, unknown to us), some assumptions must be made about energy harvesting, orbital mobility costs, radiation risks, and resource requirements.
A multi-modal figure of merit is developed for evaluating an interplanetary habitable zone (IHZ). An agent-based model is also developed to simulate the dispersal of interplanetary life in a planetary system and characterize the IHZ. For the solar system, resource weightings between planetary bodies dictate many overall behaviors, including the sequence of migration from Earth to the Moon, Mars, and asteroid belt.
Comparisons with the Trappist-1 exoplanetary system also point to critical sensitivities in the balance between resource availability and risk or cost factors (e.g., radiation risks and orbital Delta-v costs) that determine the structure of an IHZ.
Results suggest that our solar system may have an inherent, and significant, advantage for a space-faring species over a system like Trappist-1. This modeling approach may also have application to emerging space economies in our own solar system.
Caleb Scharf
Comments: 38 pages, 14 color figures, submitted to The Astrobiology Journal
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Popular Physics (physics.pop-ph)
Cite as: arXiv:2602.13404 [astro-ph.EP] (or arXiv:2602.13404v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2602.13404
Focus to learn more
Submission history
From: Caleb A. Scharf
[v1] Fri, 13 Feb 2026 19:13:00 UTC (4,421 KB)
https://arxiv.org/abs/2602.13404
Astrobiology
