A Tale of 3 Dwarf Planets: Ices and Organics on Sedna, Gonggong, and Quaoar from JWST Spectroscopy
J.P. Emery, I. Wong, R. Brunetto, J.C. Cook, N. Pinilla-Alonso, J.A., Stansberry, B.J. Holler, W.M. Grundy, S. Protopapa, A.C. Souza-Feliciano, E., Fern\'andez-Valenzuela, J.I. Lunine, D.C. Hines

TL;DR
This study uses JWST spectroscopy to analyze ices and organics on Sedna, Gonggong, and Quaoar, revealing complex organic molecules and hydrocarbons, and suggesting internal melting and geochemical evolution.
Contribution
First detailed JWST spectral analysis of these three dwarf planets, revealing their surface compositions and organic chemistry, and proposing internal evolution processes.
Findings
Detection of ethane, acetylene, and ethylene on Sedna.
Presence of complex organic molecules indicated by spectral features.
Evidence of internal melting and geochemical evolution.
Abstract
We observed Sedna, Gonggong, and Quaoar with the NIRSpec instrument on the James Webb Space Telescope (JWST). All three bodies were observed in the low-resolution prism mode at wavelengths spanning 0.7 to 5.2 m. Quaoar was also observed at 10x higher spectral resolution from 0.97 to 3.16 m using medium-resolution gratings. Sedna's spectrum shows a large number of absorption features due to ethane (CH), as well as acetylene (CH), ethylene (CH), HO, and possibly minor CO. Gonggong's spectrum also shows several, but fewer and weaker, ethane features, along with stronger and cleaner HO features and CO complexed with other molecules. Quaoar's prism spectrum shows even fewer and weaker ethane features, the deepest and cleanest HO features, a feature at 3.2 m possibly due to HCN, and CO ice. The higher-resolution medium grating…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
