2025/08/06 by Zexi Xing, Shawn Oset, Xing, Zexi +6 · 7 voices · 14 citations
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Spacecraft and Cryogenic Technologies #astro-ph.EP #astro-ph.GA
paper · pdf · doi:10.48550/arxiv.2508.04675
openalex publication_date 2025/08/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We report the detection of water activity in the third confirmed interstellar object, 3I/ATLAS, based on ultraviolet imaging with the Neil Gehrels Swift Observatory's Ultraviolet/Optical Telescope (UVOT). Assuming a reddening of 29% between 3325.7~Å and 5437.8~Å, measurements on 2025 July 31 -- August 1 yielded a first, marginal detection of OH (A2Σ -- X2Π) emission near 3085~Å, corresponding to a water production rate of (0.74 ± 0.50) × 1027 molecules s-1. The subsequent visit on 2025 August 18 -- 20 revealed a clear OH detection, implying a higher water production rate of (1.36 ± 0.35) × 1027 molecules s-1 (40 kg~s-1) at a heliocentric distance of 2.90~au. This places 3I/ATLAS among the few comets with confirmed OH emission beyond 2.5~au, where water ice sublimation from the nucleus is typically inefficient. The inferred production rate at 2.9 au implies an active area of at least 7.8~km2, assuming equilibrium sublimation. This requires that over 8% of the surface is active, which is larger than activity levels observed in most solar system comets. Contemporaneous near-infrared spectroscopy indicated the presence of icy grains in the coma, which may serve as an extended source of water vapor.