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A JWST/DiSCo-TNOs portrait of the primordial Solar System through its trans-Neptunian objects

N. Pinilla-Alonso, R. Brunetto, M. De Pra, B. Holler, E. Henault, A. C. Souza-Feliciano, V. Lorenzi, Y. J. Pendleton, D. P. Cruikshank, T. G. Müller, J. Stansberry, J. Emery, C. Schambeau, J. Licandro Goldaracena, B. Harvison, L. McClure, A. Guilbert-Lepoutre, N. Peixinho, M. T. Bannister, I. Wong

Abstract
The detection of molecules on the coldest and outermost objects in our Solar System has long been limited by the terrestrial atmosphere and sensitivity of the available instrumentation. However, near-infrared observations by the James Webb Space Telescope have provided an unprecedented view of the molecular diversity on the surfaces of trans-Neptunian objects (TNOs). Using the low spectral resolution PRISM mode on the near-infrared spectrograph as part of the Cycle 1 large programme, ‘Discovering the Surface Composition of trans-Neptunian objects’, we report the detection of several molecular ices throughout the TNO population, including H2O, CO2, 13CO2, CO, CH3OH and complex molecules and refractory materials containing aliphatic C–H, C≡N, O–H and N–H bonds. As a result of the imprint that these molecules leave on the spectra, three main compositional groups consistently emerge from multiple independent cluster analyses. Our results unlock the long-standing question of the interpretation of colour diversity, providing the much-needed compositional information. The marked separation of the three spectral clusters reveals sharp variations in the surface molecular constituents. The C/O and (CH + NH)/(C + O) ratios on the surface of TNOs are the primary indicators of the spectral differences among the three TNO compositional groups observed. We propose that these objects are fossil remnants of icy planetesimals, and that the three compositional groups provide a picture of the ice retention lines in the Solar System that likely occurred in the outer protoplanetary disk, possibly just before a major planetary migration.

Keywords
Asteroids, comets and Kuiper belt; Early solar system

Nature Astronomy
Volume 9, Page 230
2024 December

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Faculdade de Ciências da Universidade de Lisboa Universidade do Porto Faculdade de Ciências e Tecnologia da Universidade de Coimbra
Fundação para a Ciência e a Tecnologia COMPETE 2020 PORTUGAL 2020 União Europeia