THE ATMOSPHERES OF EARTHLIKE PLANETS AFTER GIANT IMPACT EVENTS by Lupu, R. E., Zahnle, Kevin, Marley, Mark S., Schaefer, Laura, Fegley, Bruce, Morley, Caroline V., Cahoy, Kerri, Freedman, Richard S., Fortney, Jonathan J.

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False Planets around Giant Stars: A Case Study of Sanders 364 in M67 by Qijia Zhou, David W. Latham, Samuel N. Quinn, Allyson Bieryla, Andrew Vanderburg, Perry Berlind, Michael L. Calkins, Gilbert A. Esquerdo

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Recent advances in giant planetary space environments by Zhonghua Yao, Ruilong Guo, Chongjing Yuan, Dongxiao Pan, Yan Xu

“…The extremely large magnetic moments of giant planets sustain giant planetary magnetospheres, trapping energetic particles with constant electromagnetic perturbations. …”
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Hydrodynamics and Survivability during Post-main-sequence Planetary Engulfment by Ricardo Yarza, Naela B. Razo-López, Ariadna Murguia-Berthier, Rosa Wallace Everson, Andrea Antoni, Morgan MacLeod, Melinda Soares-Furtado, Dongwook Lee, Enrico Ramirez-Ruiz

“…The engulfment of substellar bodies (SBs), such as brown dwarfs and planets, by giant stars is a possible explanation for rapidly rotating giants, lithium-rich giants, and the presence of SBs in close orbits around subdwarfs and white dwarfs. …”
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Tilted Circumbinary Planetary Systems as Efficient Progenitors of Free-floating Planets by Cheng Chen, Rebecca G. Martin, Stephen H. Lubow, C. J. Nixon

“…While most observed free-floating planets are giant planets, we predict that there should be more low-mass free-floating planets that are as of yet unobserved than higher-mass planets.…”
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Earths Are Not Super-Earths, Saturns Are Not Jupiters: Imprints of Pressure-bump Planet Formation on Planetary Architectures by Wenrui Xu, Songhu Wang

“…Our main prediction is that low-mass planets and giant planets can each be divided into two subpopulations with different levels of mass uniformity. …”
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The Sun Remains Relatively Refractory Depleted: Elemental Abundances for 17,412 Gaia RVS Solar Analogs and 50 Planet Hosts by Rayna Rampalli, Melissa K. Ness, Graham H. Edwards, Elisabeth R. Newton, Megan Bedell

“…Furthermore, we find no significant abundance differences between identified close-in giant planet hosts, giant planet hosts, and terrestrial/small planet hosts with the rest of the sample within our precision limits. …”
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EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates of Planets around Late-M Dwarfs within 15 pc by Jeremy Dietrich, Dániel Apai, Martin Schlecker, Kevin K. Hardegree-Ullman, Benjamin V. Rackham, Nicolas Kurtovic, Karan Molaverdikhani, Paul Gabor, Thomas Henning, Wen-Ping Chen, Luigi Mancini, Alex Bixel, Aidan Gibbs, Richard P. Boyle, Samantha Brown-Sevilla, Remo Burn, Timmy N. Delage, Lizxandra Flores-Rivera, Riccardo Franceschi, Gabriele Pichierri, Sofia Savvidou, Jonas Syed, Ivan Bruni, Wing-Huen Ip, Chow-Choong Ngeow, An-Li Tsai, Chia-Lung Lin, Wei-Jie Hou, Hsiang-Yao Hsiao, Chi-Sheng Lin, Hung-Chin Lin, Ritvik Basant, Project EDEN

“…Finally, we explore multiple hypotheses about the occurrence rates of short-period planets (from Earth-sized planets to giant planets) around late-M dwarfs. We show, for example, that giant planets with short periods (<1 day) are uncommon around our target stars. …”
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The formation of super-Earths and mini-Neptunes with giant impacts by Inamdar, Niraj K., Schlichting, Hilke E

“…If the gravitational potential energy resulting from the last mass doubling of the planet by giant impacts is released over the disc dissipation time-scale as core luminosity, then the accreted envelope masses are reduced by about an order of magnitude. …”
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Planet formation and evolution in our Solar System and beyond by Biersteker, John Brooks.

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