Cover Image

Resonant and Ultra-short-period Planet Systems are at Opposite Ends of the Exoplanet Age Distribution

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Schmidt, Stephen P., Schlaufman, Kevin C., Hamer, Jacob H.
Format:	Preprint
Published:	2024
Subjects:	Earth and Planetary Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr
by: Schmidt, Stephen P., et al.
Published: (2026)

Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal that Terrestrial Planets in Mean-motion Resonances are Water Rich
by: Ross, Alejandra, et al.
Published: (2025)

Hot Jupiters are Inflated Primarily by Shallow Heating
by: Schmidt, Stephen P., et al.
Published: (2025)

Formation of Ultra-short-period Planet in Hot Jupiter Systems: Application to WASP-47
by: Wang, Su, et al.
Published: (2025)

The Formation of Ultra-short-period Planets under the Influence of the Nearby Planetary Companions
by: Zhu, Jia Jun, et al.
Published: (2025)

A Revised Density Estimate for the Largest Known Exoplanet, HAT-P-67 b
by: Wang, Gavin, et al.
Published: (2025)

Planet Mass and Metallicity: The Exoplanets and Solar System Connection
by: Swain, Mark R., et al.
Published: (2024)

Mars as an Exoplanet: Lessons from a Planet at the Edge of Habitability
by: Kane, Stephen R., et al.
Published: (2026)

Discovery of Small Ultra-short-period Planets Orbiting KG Dwarfs in Kepler Survey Using GPU Phase Folding and Deep Learning Detection System
by: Wang, Kaitlyn, et al.
Published: (2023)

Investigating Transit Timing Variations in the Ultra-short Period Exoplanet WASP-19b
by: Biswas, Shraddha, et al.
Published: (2025)

Planets Across Space and Time (PAST). VI. Age Dependence of the Occurrence and Architecture of Ultra-Short-Period Planet Systems
by: Tu, Pei-Wei, et al.
Published: (2025)

A candidate giant planet companion to the massive, young white dwarf GALEX J071816.4+373139 informs the occurrence of giant planets orbiting B stars
by: Cheng, Sihao, et al.
Published: (2024)

On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres
by: Feinstein, Adina D., et al.
Published: (2025)

Unexpected Near-Resonant and Metastable States of Young Multi-Planet Systems
by: Hu, Zhecheng, et al.
Published: (2025)

The Prevalence of Resonance Among Young, Close-in Planets
by: Dai, Fei, et al.
Published: (2024)

The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity
by: Rice, David R., et al.
Published: (2024)

Can Neptune's Distant Mean-Motion Resonances Constrain Undiscovered Planets in the Solar System? Lessons from a Case Study of the 9:1
by: Porter, Matthew W., et al.
Published: (2024)

The Intrinsic Multiplicity Distribution of Exoplanets Revealed from the Radial Velocity Method. II. Constraints on Giant Planet Multiplicity from Different Surveys
by: Li, Jiayin, et al.
Published: (2026)

A Resonant Beginning for the Solar System Terrestrial Planets
by: Huang, Shuo, et al.
Published: (2025)

Surprising Spin-orbit Resonances of Rocky Planets
by: Yuan, Henry, et al.
Published: (2024)

Secular Resonances in Planet-Hosting Binary Stars. II. Application to Terrestrial Planet Formation
by: Haghighipour, Nader, et al.
Published: (2025)

Variations in the Radius Distribution of Single- and Compact Multiple-transiting Planets
by: Liberles, Benjamin T., et al.
Published: (2023)

Giant Outer Transiting Exoplanet Mass (GOT `EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away
by: Chachan, Yayaati, et al.
Published: (2024)

Stellar Obliquity of the Ultra-Short-Period Planet System HD 93963
by: Teng, Huan-Yu, et al.
Published: (2025)

On the Ordering of Exoplanet Systems
by: Lozovsky, Michael, et al.
Published: (2025)

Resonant Chains and the Convergent Migration of Planets in Protoplanetary Disks
by: Wong, Ka Ho, et al.
Published: (2024)

Capture and Stability of Resonant Planet Pairs in Turbulent Disk
by: Lin, Linghong, et al.
Published: (2026)

More Likely Than You Think: Inclination-Driving Secular Resonances are Common in Known Exoplanet Systems
by: Faridani, Thea, et al.
Published: (2024)

The Radius, Composition, Albedo, and Absolute Magnitude of Planet Nine Based on Exoplanets with Teq less than 600 K and the Planet Nine Reference Population 3.0
by: Russell, David G., et al.
Published: (2025)

Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Non-zero Initial $Δ$
by: Xu, Yuancheng, et al.
Published: (2025)

An Analytical Model of Wavelength-dependent Opposition Surge in Emittance and Reflectance Spectroscopy of Airless Rocky Exoplanets
by: Gkouvelis, Leonardos
Published: (2025)

Capture into Apsidal Resonance and the Decimation of Planets around In-spiraling Binaries
by: Farhat, Mohammad, et al.
Published: (2025)

Planet-disc interactions around eccentric binaries and misaligned ring formation
by: Martin, Rebecca G., et al.
Published: (2025)

The HD 191939 Exoplanet System is Well-Aligned and Flat
by: Lubin, Jack, et al.
Published: (2024)

Secular Resonances in Planet-Hosting Binary Stars. I. General Theory
by: Haghighipour, Nader, et al.
Published: (2025)

NCCR PlanetS: Observational and computational characterization of exoplanet atmospheres
by: Kitzmann, Daniel, et al.
Published: (2026)

A Climate-Constrained Bayesian Inverse Method for JWST Rocky Exoplanet Eclipse Spectra: A Case Study of LTT 1445A b
by: Wogan, Nicholas, et al.
Published: (2026)

The Epoch of Giant Planet Migration Planet Search Program. III. The Occurrence Rate of Young Giant Planets Inside the Water Ice Line
by: Tran, Quang H., et al.
Published: (2025)

Evidence of 1:1 slope between rocky Super-Earths and their host stars
by: Plotnykov, Mykhaylo, et al.
Published: (2025)

Toward Reliable Interpretations of Small Exoplanet Compositions: Comparisons and Considerations of Equations of State and Materials Used in Common Rocky Planet Models
by: Schulze, Joseph, et al.
Published: (2026)