Abundances of Elements in Solar Systems
arxiv(2024)
摘要
The relationship between stars and planets provides important information for
understanding the interior composition, mineralogy, and overall classification
of small planets (R ≲ 3.5R_⊕). Since stars and planets are
formed at the same time and from the same material, their compositions are
inextricably linked to one another, especially with respect refractory elements
like Mg, Si, and Fe. As a result, stellar elemental abundances can help break
the degeneracy inherent to planetary mass-radius models and determine whether
planets may be similar to the Earth in composition or if additional factors,
such as formation near the host star or a giant impact, may have influenced the
planet's make-up. To this end, we now have observations of the abundances of
extrasolar rocks that were pulled onto the surfaces of a white dwarfs, whose
compositions act as a direct insight into the interiors of small exoplanets.
From measurements of ∼30 of these "polluted" white dwarfs, we have found
that composition of the extrasolar rocks are similar to Solar System chondritic
meteorites.
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