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Evidence for an Atmosphere on the Ultra-short-period Super-Earth HD 3167 b

“Lava worlds”, Earth-sized planets hot enough ( T _eq  ≳ 1100 K) to melt their dayside silicate surfaces, have emerged as promising candidates for atmospheric detection and characterization. Thermal emission observations show an apparent dichotomy: The hottest lava worlds have colder daysides than t...

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Furkejuvvon:
Váldodahkkit: Brandon Park Coy, Qiao Xue, Megan Weiner Mansfield, Jason D. Eastman, Anjali A. A. Piette, Tyler Fairnington, Cole Smith, Michael Zhang, Eliza M.-R. Kempton, Jacob L. Bean, Xuan Ji, Peter Gao, Jegug Ih, Daniel D. B. Koll, Rafael Luque, Jaume Orell-Miquel, Edwin S. Kite
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2026-01-01
Ráidu:The Astrophysical Journal Letters
Fáttát:
Exoplanet atmospheres
Exoplanet atmospheric composition
Extrasolar rocky planets
Exoplanets
Super Earths
Liŋkkat:https://doi.org/10.3847/2041-8213/ae7f23
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