Insights on the Rotational State and Shape of Asteroid (203) Pompeja from TESS Photometry

The Main Belt asteroid (203) Pompeja shows evidence of extreme variability in visible and near-infrared spectral slope with time. The observed spectral variability has been hypothesized to be attributed to spatial variations across Pompeja’s surface. In this scenario, the observed spectrum of Pompej...

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Bibliographic Details
Main Authors: Oriel A. Humes, Josef Hanuš
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Planetary Science Journal
Subjects:
Online Access:https://doi.org/10.3847/PSJ/ad8f3a