Testing the Icy Pebble Accretion Hypothesis with Primordial Main-belt Asteroids
Large main-belt asteroids (diameter D ≳ 120 km) exhibit a surface composition gradient as a function of heliocentric distance, ranging from anhydrous bodies to those rich in hydrated and, possibly, ammoniated materials. Their primordial nature holds key clues to the evolution of the solar system. I...
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| Asıl Yazarlar: | , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2026-01-01
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| Seri Bilgileri: | The Astrophysical Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-4357/ae4900 |
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