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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| Asıl Yazarlar: | , |
|---|---|
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2024-01-01
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| Seri Bilgileri: | The Planetary Science Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/PSJ/ad8f3a |
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