SPHEREx Pre-Perihelion Mapping of H2O, CO2, and CO in Interstellar Object 3I/ATLAS

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SPHEREx Pre-Perihelion Mapping of H2O, CO2, and CO in Interstellar Object 3I/ATLAS

Motion of 3I. (a) Color composite from SPHEREx data at 1.185, 1.716, and 2.194 µm for red, green, and blue, respectively. The trajectory of 3I is overplotted, with observed positions marked by crosses. The starting and ending points of our dataset are indicated separately (see legend). (b) Orbital motion of 3I (black) projected onto the ecliptic plane. The orbits of Earth, Mars, and Jupiter are shown in blue, red, and purple, respectively. Numbers indicate the positions of the bodies at the first day of each month. 3I’s retrograde motion and perihelion are marked with arrows. (c) Lightcurve of 3I produced by taking all λ = 1.0−1.8 µm SPHEREx flux measurements and dividing them by the JWST flux (Fig. 2b; Cordiner et al. 2025) to leave only lightcurve variations. Also included are SOLO clear-filter brightness measurements scaled to match their median to that of the SPHEREx/JWST ratio. The resulting lightcurve amplitude is within ±15 %, so the derived reflectance should be correct to within this range considering any lightcurve modulation effects. — astro-ph.EP

From 01- to 15-Aug-2025 UT, the SPHEREx spacecraft observed interstellar object 3I/ATLAS. Using R=40-130 spectrophotometry at λ=0.7-5μm, light curves, spectra, and imaging of 3I were obtained.

From these, robust detections of water gas emission at 2.7-2.8μm and CO2 gas at 4.23-4.27μm plus tentative detections of 13CO2 and CO gas were found. A slightly extended H2O coma was detected, and a huge CO2 atmosphere extending out to at least 4.2×105km was discovered. Gas production rates for H2O, 12CO2, 13CO2, and CO were Qgas=3.2×1026±20%, 1.6×1027±10%, 1.3×1025±25%, and 1.0×1026±25%, respectively.

Co-addition of all λ=1.0-1.5μm scattered light continuum images produced a high SNR image consistent with an unresolved source. The scattered light lightcurve showed ≲15% variability over the observation period. The absolute brightness of 3I at 1.0-1.5μm is consistent with a <2.5km radius nucleus surrounded by a 100 times brighter coma.

The 1.5-4.0μm continuum structure shows a strong feature commensurate with water ice absorption seen in KBOs and distant comets. The observed cometary behavior of 3I, including its preponderance of CO2 emission, lack of CO output, small size, and predominance of large icy chunks of material in a flux-dominant coma is reminiscent of the behavior of short period comet 103P/Hartley 2, target of the NASA Deep Impact extended mission in 2010 and a “hyperactive comet” near the end of its outgassing lifetime.

This correspondence places 3I closer to barely- or non-active 1I/Oumuamua than primitive, ice rich 2I/Borisov, suggesting that ISOs are often highly thermally processed before ejection into the ISM.

Carey M. Lisse, Yoonsoo P. Bach, Sean A. Bryan, Brendan P. Crill, Phil M. Korngut, Ari J. Cukierman, Michael W. Werner, Asantha Cooray, Michael Zemcov, Volker Tolls, Gary J. Melnick, Andreas L. Faisst, C. Darren Dowell, Seungwon Choi, Jooyeon Geem, Masateru Ishiguro, Hangbin Jo, Bumhoo Lim, Max Mahlke, Joseph L. Hora, Yun-Ting Cheng, Spencer Everett, Jeong-Eun Lee, Zafar Rustamkulov, Sunho Jin, Howard Hui, Daniel C. Masters, Chi H. Nguyen, Roberta Paladini, Yujin Yang, James J. Bock, O. Doré, M. L. Sitko, C. Champagne, M. Connelley, J. P. Emery, Y. R. Fernandez, W. T. Reach

Comments: 19 pages, 4 figures, 1 table, submitted to ApJL
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2512.07318 [astro-ph.EP] (or arXiv:2512.07318v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2512.07318
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Submission history
From: Yoonsoo Bach
[v1] Mon, 8 Dec 2025 09:02:41 UTC (1,880 KB)
https://arxiv.org/abs/2512.07318
Astrobiology, Astrochemistry, Astrogeology,

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