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Heterogeneous outgassing regions identified on active centaur 29P/Schwassmann–Wachmann 1

  • Sara Faggi,
  • Geronimo L. Villanueva,
  • Adam McKay,
  • Olga Harrington Pinto,
  • Michael S. P. Kelley,
  • Dominique Bockelée-Morvan,
  • Maria Womack,
  • Charles A. Schambeau,
  • Lori Feaga,
  • Michael A. DiSanti,
  • James M. Bauer,
  • Nicolas Biver,
  • Kacper Wierzchos,
  • Yanga R. Fernandez

摘要

Centaurs are transitional objects between primitive trans-Neptunian objects and Jupiter-family comets. Their compositions and activities provide fundamental clues regarding the processes affecting the evolution of and interplay between these small bodies. Here we report observations of centaur 29P/Schwassmann–Wachmann 1 (29P) with the James Webb Space Telescope (JWST). We identified localized jets with heterogeneous compositions driving the outgassing activity. We employed the NIRSpec mapping spectrometer to study the fluorescence emissions of CO and obtain a definitive detection of CO2 for this target. The exquisite sensitivity of the instrument also enabled carbon and oxygen isotopic signatures to be probed. Molecular maps reveal complex outgassing distributions, such as jets and anisotropic morphology, which indicate that 29P’s nucleus is dominated by active regions with heterogeneous compositions. These distributions could reflect that it has a bilobate structure with compositionally distinct components or that strong differential erosion takes place on the nucleus. As there are no missions currently planning to visit a centaur, these observations demonstrate JWST’s unique capabilities in characterizing these objects.