File:Polana-Eulalia families a-H V-shape plot.jpg
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Summary
| Description |
English: Envelopes in semi-major axis of the Polana and Eulalia families over the full magnitude range. The “V”-shapes are due to size-dependent drift from the Yarkovsky effect (see Vokrouhlický et al. 2006). Objects in this work are represented by star shapes with colors corresponding to the family envelope outline, with the three Polana family asteroids: (2441) Hibbs, (6712) Hornstein, and (6769) Brokoff (shown in pink) and (495) Eulalia (in blue). (142) Polana is highlighted as a pink diamond for reference, with Polana and Eulalia family members in light pink and dark blue dots, respectively. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article). |
| Date | |
| Source | Figure 1 of https://arxiv.org/abs/2607.16518 |
| Author | Lucas McClure et al. (2026) |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 00:58, 14 August 2026 | | 900 × 700 (289 KB) | wikimediacommons>Nrco0e | Crop, label 142 Polana |
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