Toddlers in Resonance I: low masses and eccentricities of the 17 Myr giant planets HIP 67522 bc from transit timing variations
astro-ph.EP
Submitted: 2026-09-28
Updated: 2026-09-28
Terminology
Sources
- Fast Learning Requires Good Memory: A Time-Space Lower Bound for Parity Learning
- Perpendicular laser cooling with a rotating wall potential in a Penning trap
- Chaotic Advection at the Pore Scale: Mechanisms, Upscaling and Implications for Macroscopic Transport
- Transit timing and starspot-induced transit depth variations in the about 17 Myr old HIP 67522 system
- Two-stage disruption of resonant chains
- The Prevalence of Resonance Among Young, Close-in Planets
- Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
- The occurrence of small, short-period planets younger than 200 Myr with TESS
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