QR kód

A Comprehensive Reanalysis of K2-18 b’s JWST NIRISS+NIRSpec Transmission Spectrum

Sub-Neptunes are the most common type of planet in our galaxy. Interior structure models suggest that the coldest sub-Neptunes could host liquid water oceans underneath their hydrogen envelopes—sometimes called “hycean” planets. JWST transmission spectra of the ∼250 K sub-Neptune K2-18 b were recent...

Celý popis

Uloženo v:
Hlavní autoři: Stephen P. Schmidt, Ryan J. MacDonald, Shang-Min Tsai, Michael Radica, Le-Chris Wang, Eva-Maria Ahrer, Taylor J. Bell, Chloe Fisher, Daniel P. Thorngren, Nicholas Wogan, Erin M. May, Piero Ferrari, Katherine A. Bennett, Zafar Rustamkulov, Mercedes López-Morales, David K. Sing
Médium: Artigo
Jazyk:Inglês
Vydáno: IOP Publishing 2025-01-01
Edice:The Astronomical Journal
Témata:
Exoplanets
Exoplanet atmospheres
Exoplanet structure
Habitable planets
Mini Neptunes
Exoplanet atmospheric composition
On-line přístup:https://doi.org/10.3847/1538-3881/ae019a
Tagy: Přidat tag
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!

Podobné jednotky