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A chemical perspective on planet formation in reduced systems

Context. The relative abundances of refractory elements in planets are widely assumed to reflect those of their host stars. However, because elements are classified according to their behaviour in the solar nebula, this implicitly assumes that condensation is independent of nebular chemistry, despit...

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Xehetasun bibliografikoak
Egile Nagusiak: Zaveri Urja, Wang Haiyang S., Sossi Paolo A.
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: EDP Sciences 2026-05-01
Saila:Astronomy & Astrophysics
Gaiak:
Sarrera elektronikoa:https://www.aanda.org/articles/aa/full_html/2026/05/aa58126-25/aa58126-25.html
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