Hypothesis proposes that a star's galactic position affects potential biological habitability, suggesting new avenues for exploration.
This work presents the Galactic Gravitational Life-Belt Theory (GGLB), a falsifiable astrophysical hypothesis proposing that biological habitability begins at the galactic scale rather than solely at the planetary scale. The theory suggests that a star’s long-term position and orbital history within the galactic gravitational well influence the probability of forming and maintaining stable planetary systems capable of supporting life. A hierarchical framework is introduced in which galactic habitability precedes stellar, orbital, and planetary habitability. The paper develops the theoretical framework, defines observable quantities, proposes testable predictions, and establishes explicit falsification criteria. No observational confirmation is claimed; the work is presented as a hypothesis intended for future observational testing.
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Ali Alhawarat (2026) studied this question.
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