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JWST Finds CO2-Dominated Coma on Interstellar Comet 3I/ATLAS as TESS Reveals Early Activity

The CO2‑heavy chemistry offers a rare look at extrasolar ices before the comet’s late‑October perihelion.

Overview

  • JWST spectroscopy from Aug. 6 shows a coma dominated by carbon dioxide with a CO2/H2O mixing ratio of about 8 ± 1, among the highest measured for a comet.
  • NASA’s SPHEREx measured a CO2 production rate near 9.4 × 10^26 molecules per second and set upper limits on water and carbon monoxide outgassing, reinforcing the unusual volatile balance.
  • Hubble imaging on July 21 constrained the nucleus to no larger than roughly 5.6 km across and documented a diffuse dust coma, revising earlier, larger size estimates.
  • Archival TESS data reported Aug. 28 trace detections back to May 7, indicating the object was already active far from the Sun, consistent with outgassing of hypervolatile ices.
  • Trajectory forecasts place perihelion around Oct. 29–30 at ~1.4 AU and closest Earth approach on Dec. 19 at ~1.8 AU, with NASA noting no threat; speculative claims of artificial origin remain disputed by astronomers.