activity
20242026
most citedComparing the Architectures of Multiplanet Systems from Kepler, K2, and TESS Data

1 citations · 1 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026

Correlations between the Carbon-to-Oxygen Ratio and the Orbital and Physical Properties of Exoplanets

Noah Ferich, Robert Royer, Cody Shakespeare +1

Studies suggest that protoplanetary disks around stars with high carbon-to-oxygen (C/O) ratios can produce terrestrial planets with carbon-dominated compositions instead of silicon…

astro-ph.EP2026

Modeling Carbon-Based Planets with MAGRATHEA

Robert Royer, David R. Rice, Jason H. Steffen

A planet's interior structure not only influences its habitability, but it also provides information about the planet's formation and history. In the quest to characterize the vari…

astro-ph.IM2025

Magrathea v2: A planetary interior modeling platform in C++

David R. Rice, Chenliang Huang, Robert Royer +5

Magrathea is an open-source C++ code for modeling the internal structure of differentiated planets. The initial release, Huang et al. (2022), introduced the base solver, a modular…

astro-ph.EP2025

Effect of Galactic Chemical Evolution on Exoplanet Properties

Jason H. Steffen, Cody Shakespeare, Robert Royer +2

We couple a simplified model for the galactic chemical evolution, with software that models the condensation of dust in protoplanetary disks and software that models the interior s…

astro-ph.EP2025★ 1 cited

Comparing the Architectures of Multiplanet Systems from Kepler, K2, and TESS Data

Robert Royer, Jason H. Steffen

Exoplanet surveys like Kepler, TESS, and K2 have shown that planetary systems are common in our galaxy. These surveys, along with several others, have identified thousands of plane…

astro-ph.EP2025

Uncertainties in the Inference of Internal Structure: The Case of TRAPPIST-1 f

David R. Rice, Chenliang Huang, Jason H. Steffen +1

We use the TRAPPIST-1 system as a model observation of Earth-like planets. The densities of these planets being 1-10% less than the Earth suggest that the outer planets may host si…

astro-ph.EP2024

Enhanced Stability in Planetary Systems with Similar Masses

Dong-Hong Wu, Sheng Jin, Jason H. Steffen

This study employs numerical simulations to explore the relationship between the dynamical instability of planetary systems and the uniformity of planetary masses within the system…

astro-ph.EP2024

The effects of the carbon-to-oxygen ratio on the condensate compositions around Solar-like stars

Cody J. Shakespeare, Min Li, Shichun Huang +2

The initial stellar carbon-to-oxygen (C/O) ratio can have a large impact on the resulting condensed species present in the protoplanetary disk and, hence, the composition of the bo…

astro-ph.EP2024

Composition Tracking for Collisions Between Differentiated Bodies in REBOUND

Noah Ferich, Anna C. Childs, Jason H. Steffen

Previous research suggests that impacts between planetary embryos and planetesimals during the late stages of planet formation can often determine the percentages of core and mantl…