Pre-perihelion Emergence of the CN Gas Coma in 3I/ATLAS Temporally and Spatially Resolved by the 7-dimensional Telescope
Authors:
- Gregory S. H. PaekGPGregory S. H. Paek
- Myungshin ImMIMyungshin Im
- Mankeun JeongMJMankeun Jeong
- Hyeonho ChoiHCHyeonho Choi
- Yoonsoo P. BachYBYoonsoo P. Bach
- Masateru IshiguroMIMasateru Ishiguro
- Bumhoo LimBLBumhoo Lim
- Seo-Won ChangSCSeo-Won Chang
- Ji Hoon KimJKJi Hoon Kim
- Jooyeon GeemJGJooyeon Geem
- Willem B. HoogendamWHWillem B. Hoogendam
Open Access
- 12 March 2026
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 1000 (1)
Abstract
We present time series medium-band ( R ∼ 20–40) observations of the third interstellar object (ISO) 3I/ATLAS (C/2025 N1) obtained with the 7-Dimensional Telescope, which enabled spatially resolved monitoring of its gas and dust activity from 2025 July to September. The m400-band image ( λ c = 400 nm, Δ λ ≈ 25 nm) reveals an emergence of a pronounced and spatially extended CN emission at a heliocentric distance of r h < 3 au. This onset is consistently identified across multiple diagnostics, including a break in the light-curve evolution, excess reflectance, inward expansion of annular excess beyond 10,000–20,000 km, growth of the coma half-light radius from ∼11,000 to ∼19,000 km, and a rapid rise in the CN production rate Q CN relative to Afρ . We further separate the CN-emitting and dust-scattered components via two-dimensional surface brightness fitting into inner (dust) and outer (gas) components. We find that the outer component preserves a nearly constant profile shape, varying only in normalization, implying a relatively fast expansion of CN-bearing molecules. Together, these results reveal how a transition occurs in the optical from dust-dominated scattering at large heliocentric distances to volatile-driven, gas-dominated activity as 3I/ATLAS enters the inner solar system. The timing and characteristics of the CN activation resemble the volatile enhancement observed in 2I/Borisov, suggesting that both known active ISOs exhibit comparable activation behavior at heliocentric distances of ∼2–3 au.Keywords
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Funding Information
- Ministry of Science and ICT, South Korea (2021M3F7A1084525)
- NASA SSO Near Earth Observation Program (80NSSC18K0971)
- NASA SSO Near Earth Observation Program (NNX14AM74G)
- NASA SSO Near Earth Observation Program (NNX12AR65G)
- NASA SSO Near Earth Observation Program (NNX13AQ47G)
- NASA SSO Near Earth Observation Program (NNX08AR22G)
- NASA SSO Near Earth Observation Program (80NSSC21K1572)
- Ministry of Science and ICT, South Korea (RS-2023-00245013)
- Ministry of Science and ICT, South Korea (2020R1A2C3011091)
- Ministry of Science and ICT, South Korea (RS-2021-II212068)
- Ministry of Science and ICT, South Korea (RS-2025-00573214)
- Ministry of Science and ICT, South Korea (RS-2025-25436385)
- NSF ∣ National Science Foundation Graduate Research Fellowship Program (2236415)
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