Overview
- Space-based solar observatories STEREO, SOHO and GOES‑19 recorded an unusually steep pre‑perihelion brightening (≈ r^-7.5) and a visible shift to bluer color around Oct. 29–30.
- JWST/NIRSpec and SPHEREx measured extreme volatiles in the coma, with CO2/H2O ≈ 7.6±0.3 and CO/H2O ≈ 1.65±0.09, far outside typical solar‑system comet trends.
- An arXiv analysis interprets the spectra and red continuum slopes as evidence of galactic cosmic‑ray alteration, estimating an irradiated crust roughly 15–20 meters deep that current outgassing samples.
- Most planetary scientists and NASA officials describe the object as a natural, CO2‑driven comet, while Avi Loeb promotes artificial‑origin and “non‑gravitational acceleration” claims that others say are unsubstantiated by the available data.
- Ground follow‑up is constrained by solar conjunction until mid‑ to late‑November, with planned observations expected to probe whether deeper, less‑processed material becomes exposed and to refine any non‑gravitational terms.