Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal That Terrestrial Planets in Mean Motion Resonances Are Water Rich

Exoplanet mass and radius inferences fundamentally rely on host star mass and radius inferences. Despite the importance of host star mass, radius, and elemental abundance inferences for the derivation of exoplanet internal structure constraints, published constraints have often been based on inferen...

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Váldodahkkit:	Alejandra Ross, Henrique Reggiani, Kevin C. Schlaufman, Mykhaylo Plotnykov, Diana Valencia
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2025-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Exoplanet systems Exoplanet astronomy Exoplanet dynamics Exoplanet formation Exoplanet structure Exoplanets
Liŋkkat:	https://doi.org/10.3847/1538-4357/ae03a5
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