Kepler-9 TTV data permits broad ranges of planetary masses (b: 31.6-47.1 M⊕; c: 21.8-32.3 M⊕) linked by a tight mass ratio, showing that previous single-mode mass determinations were illusory.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
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astro-ph.EP 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Reassessment of 12 TTV claims finds only two systems with compelling unique solutions for the perturbing planet, six with multiple viable solutions, and two with weak evidence overall.
Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.
citing papers explorer
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The Illusory Precision of TTV Masses: Hidden Solutions Behind Kepler-9's Tight Mass Ratio
Kepler-9 TTV data permits broad ranges of planetary masses (b: 31.6-47.1 M⊕; c: 21.8-32.3 M⊕) linked by a tight mass ratio, showing that previous single-mode mass determinations were illusory.
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TTV-Not-So-Fast: Uniqueness and Degeneracy in Perturbing Planet Parameters
Reassessment of 12 TTV claims finds only two systems with compelling unique solutions for the perturbing planet, six with multiple viable solutions, and two with weak evidence overall.
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Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
Young M dwarf flares exert greater chemical stress on primordial exo-Earth atmospheres than previous models, with potential for lasting changes in mixing ratios especially for low-abundance species.