Revisiting The Radius Valley Across Stellar Types: A Transit-Only Analysis of M, K, G, and F Stars with Updated NASA Exoplanet Archive Data

editorAstrobiology15 hours ago1 Views

Revisiting The Radius Valley Across Stellar Types: A Transit-Only Analysis of M, K, G, and F Stars with Updated NASA Exoplanet Archive Data

Radius distributions of exoplanets around M, K, G, and F stars. The valley is centered at ∼1.6 R⊕ for M dwarfs, ∼1.8 R⊕ for K and G dwarfs, and ∼1.9 R⊕ for F dwarfs. The sharpness of the valley depends on stellar type, being strongest for G/K stars and weaker for M and F stars. — astro-ph.EP

The radius valley — a deficit of exoplanets between super-Earths and sub-Neptunes — is a key diagnostic of planet formation and atmospheric evolution.

We investigate how the radius valley depends on stellar type by analyzing an updated, transit-only sample of exoplanets from the NASA Exoplanet Archive. Planets are selected with P<100 days and divided by host spectral class (M, K, G, F).

We construct weighted radius distributions and apply statistical tests to quantify the valley depth. We recover a pronounced valley centered near ∼1.8R for G/K stars, but shifted to ∼1.6R for M dwarfs and ∼1.9R for F stars.

These results support the view that the radius valley is shaped by stellar-dependent processes such as photoevaporation, core-powered mass loss, and orbital migration.

Sukdev Mahapatra

Comments: 7 Pages, 3 Figures, 2 Tables
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2509.03549 [astro-ph.EP] (or arXiv:2509.03549v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2509.03549
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Submission history
From: Sukdev Mahapatra
[v1] Tue, 2 Sep 2025 18:38:15 UTC (450 KB)
https://arxiv.org/abs/2509.03549
Astrobiology, exoplanet,

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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