Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 A3.

(C1) Continuum line (black solid line) calculated for the 2.7 μm band for (142) Polana’s spectrum (in red). The reflectance is then divided by the continuum line. (C2) Gaussian fits (in yellow) used to produce a multi-Gaussian-based model of the band (in red). The residual difference between the model and the data, as well as the calculated band parameters, are shown as well.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse