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Sources3I/ATLASTaylor 2025
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The Kinematic Age of 3I/ATLAS and its Implications for Early Planet Formation

Aster G. Taylor, Darryl Z. Seligman, 2025. ApJL 990, L14.

Kinematic age ~3-11 Gyr; 12% chance host star had [Fe/H] <= -0.4; activity must dominate brightness given the ISO mass budget.

MYS0DFPTE25MVWR · mystery · click to copyM3I/ATLASArticledoi: 10.3847/2041-8213/adfa280

Cited by on this site 2 records

3I/ATLAS
The mystery article
MYS

Cite it

Taylor, A. G., & Seligman, D. Z. (2025). The Kinematic Age of 3I/ATLAS and its Implications for Early Planet Formation. ApJL 990, L14. https://doi.org/10.3847/2041-8213/adfa28
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