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The Polana–Eulalia Complex with JWST NIRSpec: Connections to Bennu, Ryugu, and Outer Solar System Bodies

  • Authors: Lucas T. McClure, Joshua P. Emery, Driss Takir, Julia de León, Mário de Prá, Brittany Harvison, Bryan Holler, Javier Licandro, Tania Le Pivert-Jolivet, Joseph Masiero, Noemi Pinilla-Alonso

Lucas T. McClure et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 11.

The spectrum of (495) Eulalia (in blue) exhibits minor absorptions from 3.0 to 4.0 μm that are comparable to small bodies within and beyond the main belt. Examples include (142) Polana (red; A. Arredondo et al. 2025), Jovian irregular satellite Himalia (purple; B. N. L. Sharkey et al. 2025), and organic-rich Jovian irregular satellite Sinope (dark orange; B. N. L. Sharkey et al. 2025). Reflectance values are normalized to 4.0 μm and offset by increments of 0.12 μm for (142) Polana (−0.12), Himalia (−0.48), and Sinope (−0.60).

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