2025/11/20 by Benjamin Farcy, Benjamin J. Farcy, Darryl Z. Seligman +10 · 1 voice
Physics and Astronomy · #Earth and Planetary Astrophysics (astro-ph.EP) #Exoplanet #FOS: Physical sciences #Habitability #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Mars Exploration Program #Martian #Origins and Evolution of Life #Planet #Planetary habitability #Solar System #Space Science and Extraterrestrial Life #Stellar, planetary, and galactic studies #Terrestrial planet #astro-ph.EP #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.2511.16714
published in arXiv (Cornell University) (Cornell University)
openalex publication_date 2025/11/20 · arxiv published 2025/11/20 · arxiv updated 2025/11/20 · openalex created_date 2025/11/25 · openalex updated_date 2026/08/05
The breadth of topics that encompass the search for life has expanded and evolved significantly since the emergence of the field of astrobiology. Initial astrobiology centered investigations focused on detecting biosignatures in the Martian soil with the Viking lander. The field now encompasses identification of biosignatures throughout the galaxy and habitable worlds, planets with sufficient liquid water and prebiotic chemistry to support life. This evolution mirrors the improvement in our understanding of environments that may harbor life. The bulk planetary chemistry governs the habitability of a planet, which is in turn set by the early solar system environment and planet formation processes. Therefore, investigations of solar and exoplanetary systems as a whole would provide insights into the factors that make a planet habitable. Bulk planetary chemistry govern planetary atmospheres, core sizes, magnetic fields, heat engines, volatile inventories, and silicate mantle compositions. We therefore advocate for investigations of formation conditions that establish planetary chemistry, and by extension, habitability.