Pre-perihelion Volatile Evolution of Interstellar Comet 3I/ATLAS Indicating Significant Contribution from Extended Source in the Coma
Juncen Li, Xian Shi, Man-To Hui, Jianchun Shi

TL;DR
This study presents radio and millimeter observations of interstellar comet 3I/ATLAS, revealing volatile compositions and significant contributions from extended sources in its coma, enhancing understanding of interstellar cometary activity.
Contribution
It provides new measurements of volatile production rates and demonstrates the importance of extended sources in the comet's coma, a novel insight for interstellar comet studies.
Findings
OH production rates at different distances from the Sun
CO/H2O ratio of approximately 28%
Extended source sublimation accounts for up to 80% of water measurements
Abstract
Interstellar comets provide rare opportunities for probing the diversity of refractory and volatile inventory around other stars. As the second ever interstellar comet, and the third interstellar object, 3I/ATLAS has been the focus of telescopic observations since its discovery in July 2025. Following the previous observations at multi-wavelengths, we present further radio observations of the 1665/1667 MHz ground-state OH lines and millimeter observations of the CO(=1-0) transition at 115.271 GHz that trace the coma and CO abundances, respectively. We derived OH production rates of at 2.27 au and at 1.96 au as well as an average CO production rate of between 2.33 and 1.75 au, inferring a CO/ ratio of (). With the mean HCN…
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Taxonomy
TopicsAstro and Planetary Science · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
