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The James Webb Space Telescope NIRSpec-PRISM Transmission Spectrum of the Super-puff, Kepler-51d

Kepler-51 is a 500 Myr G dwarf hosting three “super-puffs” and one low-mass nontransiting planet. Kepler-51d, the coolest ( T _eq ∼ 350 K) transiting planet in this system is also one of the lowest-density super-puffs known to date ( ρ _p = 0.038 ± 0.009 g cm ^−3 ). With a planetary mass of M _p = 5...

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Detaylı Bibliyografya
Asıl Yazarlar: Jessica E. Libby-Roberts, Aaron Bello-Arufe, Zachory K. Berta-Thompson, Caleb I. Cañas, Yayaati Chachan, Renyu Hu, Yui Kawashima, Catriona Murray, Kazumasa Ohno, Armen Tokadjian, Suvrath Mahadevan, Kento Masuda, Leslie Hebb, Caroline Morley, Guangwei Fu, Peter Gao, Kevin B. Stevenson
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2026-01-01
Seri Bilgileri:The Astronomical Journal
Konular:
Online Erişim:https://doi.org/10.3847/1538-3881/ae33c0
Etiketler: Etiketle
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