46 citations · 204 across the 25 of their papers we have counts for
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Saturn's Evolutionary History and Seismology: Survival of Deep Stably Stratified Regions in Evolutionary Models of Saturn Consistent with Ring Seismology
Yubo Su, Janosz W. Dewberry, Roberto Tejada Arevalo +2
With recent advances in the modeling of the solar system giant planets, rapid progress has been made in understanding the remaining questions pertaining to their formation and evol…
Isolating the gravitational influence of Uranus's winds requires close passages inward of the rings
Christopher R. Mankovich, Marzia Parisi, Damon F. Landau +1
Close orbits by a Uranus Orbiter and Probe (UOP) could be used to deduce Uranus's multipolar gravity field to higher precision and angular degree than the J2 and J4 currently measu…
Unveiling What Makes Saturn Ring: Quantifying the Amplitudes of Saturn's Planetary Normal-Mode Oscillations and Trends in C-Ring Properties Using Kronoseismology (VII)
Victor M Afigbo, Matthew M Hedman, Phillip Nicholson +4
Certain spiral density waves in Saturn's rings are generated through resonances with planetary normal modes, making them valuable probes of Saturn's internal structure. Previous re…
Setting the Stage for Uranian Seismology from Rings and Radial Velocities
Christopher R. Mankovich, A. James Friedson, Marzia Parisi +6
A Uranus orbiter would be well positioned to detect the planet's free oscillation modes, whose frequencies can resolve questions about Uranus's weakly constrained interior. We calc…
Damping Obliquities of Hot Jupiter Hosts by Resonance Locking
J. J. Zanazzi, Janosz Dewberry, Eugene Chiang
When orbiting hotter stars, hot Jupiters are often highly inclined relative to their host star equator planes. By contrast, hot Jupiters orbiting cooler stars are more aligned. Pri…
Tidal migration of exoplanets around M-dwarfs: frequency-dependent tidal dissipation
Samantha C. Wu, Janosz W. Dewberry, Jim Fuller
The orbital architectures of short-period exoplanet systems are shaped by tidal dissipation in their host stars. For low-mass M-dwarfs whose dynamical tidal response comprises a de…
Saturn's Seismic Rotation Revisited
Christopher R. Mankovich, Janosz W. Dewberry, Jim Fuller
Normal mode seismology is a promising means of measuring rotation in gas giant interiors, and ring seismology presents a singular opportunity to do so at Saturn. We calculate Satur…
Dynamical tides in Jupiter and other rotationally flattened planets and stars with stable stratification
Janosz W. Dewberry
We develop a numerical method for directly computing the dissipative dynamical tidal response of rapidly rotating, oblate stars and gaseous planets with realistic internal structur…
Impacts of zonal winds on planetary oscillations and Saturn ring seismology
Janosz W. Dewberry, Christopher R. Mankovich, Jim Fuller
The excitation of density and bending waves in Saturn's C ring by planetary oscillation modes presents a unique opportunity to learn about gas giant interiors and rotation. However…
Dynamical tidal Love numbers of rapidly rotating planets and stars
Janosz W. Dewberry, Dong Lai
Tidal interactions play an important role in many astrophysical systems, but uncertainties regarding the tides of rapidly rotating, centrifugally distorted stars and gaseous planet…
Constraining Saturn's interior with ring seismology: effects of differential rotation and stable stratification
Janosz W. Dewberry, Christopher R. Mankovich, Jim Fuller +2
Normal mode oscillations in Saturn excite density and bending waves in the C Ring, providing a valuable window into the planet's interior. Saturn's fundamental modes (f modes) exci…