Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis
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arXiv
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| Format: | Preprint |
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2026
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| author | Kaplan, Murat |
| author_facet | Kaplan, Murat |
| contents | The spectral evolution of asteroid surfaces reflects the competition between space weathering and impact resurfacing. While previous studies focused primarily on age-dating, the role of family population size remains largely unexplored. We tested whether population-dependent collisional activity affects observable surface properties by analyzing 154 asteroid families using NEOWISE thermal infrared photometry, validated by independent AKARI observations and error propagation analysis. We introduced the V-Dominance Index (VDI) to quantify the incidence of extreme resurfacing signatures within families, defined as the fraction of members with visible-to-infrared albedo ratios p_V/p_IR > 1.2. Among tested parameters, family population size (N) emerged as the dominant correlate of VDI across both silicaceous (S-complex: r_s = 0.58) and carbonaceous (C-complex: r_s = 0.44) taxonomic types, with a full-sample correlation r_s = 0.476 (p = 4.31 x 10^-10). This correlation survived Monte Carlo permutation tests, binomial null model validation, age-matched contrast analyses, and heliocentric independence tests. Percentile sensitivity analysis demonstrated that VDI isolates rare resurfacing events detectable only at extreme thresholds. In families older than 2 Gyr, large populations maintained statistically significant fresh tails (p < 10^-4), whereas small populations were saturated. These results indicate that massive families experience elevated collisional resurfacing rates that counteract space weathering saturation. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_23347 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis Kaplan, Murat Earth and Planetary Astrophysics The spectral evolution of asteroid surfaces reflects the competition between space weathering and impact resurfacing. While previous studies focused primarily on age-dating, the role of family population size remains largely unexplored. We tested whether population-dependent collisional activity affects observable surface properties by analyzing 154 asteroid families using NEOWISE thermal infrared photometry, validated by independent AKARI observations and error propagation analysis. We introduced the V-Dominance Index (VDI) to quantify the incidence of extreme resurfacing signatures within families, defined as the fraction of members with visible-to-infrared albedo ratios p_V/p_IR > 1.2. Among tested parameters, family population size (N) emerged as the dominant correlate of VDI across both silicaceous (S-complex: r_s = 0.58) and carbonaceous (C-complex: r_s = 0.44) taxonomic types, with a full-sample correlation r_s = 0.476 (p = 4.31 x 10^-10). This correlation survived Monte Carlo permutation tests, binomial null model validation, age-matched contrast analyses, and heliocentric independence tests. Percentile sensitivity analysis demonstrated that VDI isolates rare resurfacing events detectable only at extreme thresholds. In families older than 2 Gyr, large populations maintained statistically significant fresh tails (p < 10^-4), whereas small populations were saturated. These results indicate that massive families experience elevated collisional resurfacing rates that counteract space weathering saturation. |
| title | Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2605.23347 |