File:Nysa 2015 TC25 Rantila spectra Cantillo et al. 2026 Fig 17.jpg
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Summary
| Description |
English: Visible to near-infrared spectra of the two Rantila aubrite grain size end-members (slab and <45 μm) plotted against near-earth asteroid 2015 TC25 and main-belt asteroid (44) Nysa. The range in slope observed across the samples of Rantila may explain the discrepancy between 2015 TC25 and (44) Nysa (rough NEA surface versus fine-grained main belt surface). In addition, Rantila may be linked with (44) Nysa due to the similar 0.9 μm absorption feature. |
| Date | |
| Source | Figure 17 of Cantillo et al. https://iopscience.iop.org/article/10.3847/PSJ/ae6db2/meta |
| Author | Cantillo et al. (2026)/American Astronomical Society |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:48, 8 August 2026 | | 1,200 × 812 (352 KB) | wikimediacommons>Nrco0e | Uploaded a work by Cantillo et al. (2026)/American Astronomical Society from Figure 17 of Cantillo et al. https://iopscience.iop.org/article/10.3847/PSJ/ae6db2/meta with UploadWizard |
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