SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS

Abstract In mid-August 2025, 0.75–5.0 μ m SPHEREx imaging spectrophotometric and ancillary NASA-IRTF/SpeX 0.7–2.5 μ m low-resolution spectral observations of 3I/ATLAS were obtained. The combined spectrophotometry is dominated by features due to water ice absorption and CO 2 gas emission. A bright, ∼3′ radius CO 2 gas coma was clearly resolved, corresponding to Q gas,CO2 ∼9.4 × 10 26 molecules s −1 . From the SPHEREx photometry, we put conservative, preliminary 3 σ upper limits on the gas production rates for H 2 O and CO of 1.5 × 10 26 and 2.8 × 10 26 molecules s −1 , respectively. No obvious jet, tail, or trail structures were found in SPHEREx images. If we assume all observed 1 μ m flux is scattered light from a p v = 0.04 albedo spherical nucleus, then the radius would be R nuc ∼ 23 km. Given the nucleus size limit R nuc < 2.8 km from D. Jewitt et al., we conclude >99% of the measured SPHEREx continuum flux is from coma dust.

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Publication Details

Journal
Research Notes of the AAS
Published
2025-09-09
DOI
https://doi.org/10.3847/2515-5172/ae0293
Citations
16
Primary Topic
Atmospheric Ozone and Climate
Type
article
Field-Weighted Citation Impact
20.81
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article

SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS

Sean Bryan, Volker Tolls, Joshua P. Emery, Gary J. Melnick et al.
16 citations
Research Notes of the AAS
Atmospheric Ozone and Climate
20.81
article

SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS

Sean Bryan, Volker Tolls, Joshua P. Emery, Gary J. Melnick, Olivier Doré, Phillip Korngut, B. P. Crill, Zafar Rustamkulov, Beth Fabinsky, A. Cukierman, Bo Yang, C. M. Lisse, M. W. Werner, Michael L. Sitko, Michael S. Connelley, Y. R. Fernández, Andreas L. Faisst, Yoonsoo P. Bach, Chansey Champagne
article en
16 citations

Abstract

Abstract In mid-August 2025, 0.75–5.0 μ m SPHEREx imaging spectrophotometric and ancillary NASA-IRTF/SpeX 0.7–2.5 μ m low-resolution spectral observations of 3I/ATLAS were obtained. The combined spectrophotometry is dominated by features due to water ice absorption and CO 2 gas emission. A bright, ∼3′ radius CO 2 gas coma was clearly resolved, corresponding to Q gas,CO2 ∼9.4 × 10 26 molecules s −1 . From the SPHEREx photometry, we put conservative, preliminary 3 σ upper limits on the gas production rates for H 2 O and CO of 1.5 × 10 26 and 2.8 × 10 26 molecules s −1 , respectively. No obvious jet, tail, or trail structures were found in SPHEREx images. If we assume all observed 1 μ m flux is scattered light from a p v = 0.04 albedo spherical nucleus, then the radius would be R nuc ∼ 23 km. Given the nucleus size limit R nuc < 2.8 km from D. Jewitt et al., we conclude >99% of the measured SPHEREx continuum flux is from coma dust.

Research Notes of the AASVol. 9(9)
University of Central Florida (US), California Institute of Technology (US), Space Science Institute (US), Planetary Science Institute (US), Jet Propulsion Laboratory (US), Northern Arizona University (US), Korea Astronomy and Space Science Institute (KR), Johns Hopkins University Applied Physics Laboratory (US), University of Hawaii at Hilo (US), Center for Astrophysics Harvard & Smithsonian (US), Infrared Processing and Analysis Center (US), Arizona State University (US)
Openalex Percentile: Top 0%
Atmospheric Ozone and Climate
20.81
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