Metallicity Dependence of Giant Planets around M Dwarfs by Tianjun Gan, Christopher A. Theissen, Sharon X. Wang, Adam J. Burgasser, Shude Mao

Subjects: “…Extrasolar gaseous giant planets…”
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Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet's Cores by Zifan Lin, Saverio Cambioni, Sara Seager

“…We conclude that most high-density exoplanets are unlikely to be remnant giant planet cores.…”
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JWST/NIRCam 4–5 μm Imaging of the Giant Planet AF Lep b by Kyle Franson, William O. Balmer, Brendan P. Bowler, Laurent Pueyo, Yifan Zhou, Emily Rickman, Zhoujian Zhang, Sagnick Mukherjee, Tim D. Pearce, Daniella C. Bardalez Gagliuffi, Lauren I. Biddle, Timothy D. Brandt, Rachel Bowens-Rubin, Justin R. Crepp, James W. Davidson Jr., Jacqueline Faherty, Christian Ginski, Elliott P. Horch, Marvin Morgan, Caroline V. Morley, Marshall D. Perrin, Aniket Sanghi, Maïssa Salama, Christopher A. Theissen, Quang H. Tran, Trevor N. Wolf

Subjects: “…Extrasolar gaseous giant planets…”
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Jupiter Evolutionary Models Incorporating Stably Stratified Regions by Roberto Tejada Arevalo, Ankan Sur, Yubo Su, Adam Burrows

Subjects: “…Solar system gas giant planets…”
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The Heating Efficiency of Hot Jupiters from a Data-driven Perspective by Sheng Jin, Dong-Hong Wu, Yi-Xuan Cao, Zi-Yi Guo

Subjects: “…Extrasolar gaseous giant planets…”
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Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-hydrodynamic Code by Riley Rosener, Michael Zhang, Jacob L. Bean

Subjects: “…Extrasolar gaseous giant planets…”
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Effects of Thermodynamics on the Concurrent Accretion and Migration of Gas Giants in Protoplanetary Disks by Hening Wu, Ya-Ping Li

“…Accretion and migration usually proceed concurrently for giant planet formation in the natal protoplanetary disks. …”
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On the Formation of Planets in the Milky Way’s Thick Disk by Tim Hallatt, Eve J. Lee

“…Our calculations imply that the deficit in planet occurrence around thick-disk stars should be even more pronounced for giant planets, particularly those at wide orbital separations, predicting a higher rocky-to-giant planet ratio in the Galactic thick disk versus thin disk.…”
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Direct imaging of exoplanets: Legacy and prospects by Chauvin, Gael

“…From the astrophysical point of view, it is indeed crucial to understand the mechanisms of formation and evolution of giant planets, including planet and disk interactions, which will completely sculpt the planetary architectures and thus dominate the formation of terrestrial planets, especially in regions around the host star capable of supporting life. …”
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Planetary formation and early phases by Crida, Aurélien

“…Finally, gas accretion proceeds on ten Earth mass solid cores.Once the gas disk is dissipated, giant planets may form satellites from massive rings, the terrestrial planets assemble from smaller embryos, and global dynamical instabilities give the planetary systems their final architecture.…”
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Multi-wavelength global maps of Jupiter and Saturn using Cassini imaging system data by Xinyue Wang, Liming Li, Xun Jiang, Robert A. West

“…., clouds, storms, vortices, eddies, waves, and turbulence), thereby enhancing our understanding of atmospheric dynamics on the giant planets.…”
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The Doubly Librating Plutinos by Renu Malhotra, Takashi Ito

“…These results may offer new constraints for theoretical models of the dynamical history of the Plutinos and of the orbital migration history of the giant planets.…”
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Formation of Super-Earths and Mini-Neptunes from Rings of Planetesimals by Sho Shibata, Andre Izidoro

“…The solar system's planetary architecture has been proposed to be consistent with the terrestrial and giant planets forming from material rings at ∼1 au and ∼5 au, respectively. …”
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The Hottest Neptunes Orbit Metal-rich Stars by Shreyas Vissapragada, Aida Behmard

“…While some studies suggest that Neptune desert planets form and evolve similarly to longer-period Neptunes, others argue that they are products of rare collisions between smaller planets, or that they are the exposed interiors of giant planets (i.e., “hot Jupiters gone wrong”). These origin stories make different predictions for the metallicities of Neptune desert host stars. …”
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Orbit of a Possible Planet X by Amir Siraj, Christopher F. Chyba, Scott Tremaine

“…Since a natural explanation for clustering in ϖ is an unseen planet, we run 300 N -body simulations with the giant planets, a disk of test particles representing Kuiper Belt objects, and an additional planet with varied initial conditions for its mass, semimajor axis, eccentricity, and inclination. …”
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