activity
20242026
collaborators

5 papers

astro-ph.EP2026

Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss

Grant C. Weldon, Samuel W. Yee, Bradley M. S. Hansen +17

The production of Neptune-like planets with orbital periods of 3--6 days is challenging for conventional models of high-eccentricity migration. We present the discovery and charact…

astro-ph.EP2026

Saving Doomed Planets: Mass Loss and Angular Momentum Return Boost Hot Jupiter Survival Rates

Grant C. Weldon, Bradley M. S. Hansen, Smadar Naoz

The existence of giant extrasolar planets on short-period orbits ("hot Jupiters") challenges planet formation theories because such planets are difficult to form close to the star.…

astro-ph.EP2025

Dynamical Excitation as a probe of planetary origins

Brad M. S. Hansen, Tze-Yeung Yu, Neel Nagarajan +1

We present a set of numerical simulations of the dynamical evolution of compact planetary systems migrating in a protoplanetary disk whose inner edge is sculpted by the interaction…

astro-ph.EP2025

The cold Jupiter eccentricity distribution is consistent with EKL driven by stellar companions

Grant C. Weldon, Smadar Naoz, Bradley M. S. Hansen

The large eccentricities of cold Jupiters and the existence of hot Jupiters have long challenged theories of planet formation. A proposed solution to both of these puzzles is high-…

astro-ph.SR2024

Once a Triple, Not Always a Triple: The Evolution of Hierarchical Triples that Yield Merged Inner Binaries

Cheyanne Shariat, Smadar Naoz, Kareem El-Badry +4

More than half of all main-sequence (MS) stars have one or more companions, and many of those with initial masses <8 M are born in hierarchical triples. These systems featu…