activity
20112023
most citedDensities and Eccentricities of 139 Kepler Planets from Transit Time Variations

247 citations · 1.3k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.EP2023

Masses, Revised Radii, and a Third Planet Candidate in the "Inverted" Planetary System Around TOI-1266

Ryan Cloutier, Michael Greklek-McKeon, Serena Wurmser +40

Is the population of close-in planets orbiting M dwarfs sculpted by thermally driven escape or is it a direct outcome of the planet formation process? A number of recent empirical…

astro-ph.EP2023

Scattered Disk Dynamics: The Mapping Approach

Sam Hadden, Scott Tremaine

We derive, and discuss the properties of, a symplectic map for the dynamics of bodies on nearly parabolic orbits. The orbits are perturbed by a planet on a circular, coplanar orbit…

astro-ph.EP2023★ 1 cited

Mercury's chaotic secular evolution as a subdiffusive process

Dorian S. Abbot, Robert J. Webber, David M. Hernandez +2

Mercury's orbit can destabilize, generally resulting in a collision with either Venus or the Sun. Chaotic evolution can cause g1 to decrease to the approximately constant value of…

astro-ph.EP2023★ 26 cited

Intra-system uniformity: a natural outcome of dynamical sculpting

Caleb Lammers, Sam Hadden, Norman Murray

There is evidence that exoplanet systems display intra-system uniformity in mass, radius, and orbital spacing (like ``peas in a pod'') when compared with the system-to-system varia…

astro-ph.EP2023★ 34 cited

Self-Consistent Spin, Tidal and Dynamical Equations of Motion in the REBOUNDx Framework

Tiger Lu, Hanno Rein, Daniel Tamayo +4

We have introduced self-consistent spin, tidal and dynamical equations of motion into REBOUNDx, a library of additional effects for the popular N-body integrator REBOUND. The equat…

astro-ph.EP2022★ 11 cited

Simple physics and integrators accurately reproduce Mercury instability statistics

Dorian S. Abbot, David M. Hernandez, Sam Hadden +3

The long-term stability of the Solar System is an issue of significant scientific and philosophical interest. The mechanism leading to instability is Mercury's eccentricity being p…

astro-ph.EP2022★ 19 cited

celmech: A Python package for celestial mechanics

Sam Hadden, Daniel Tamayo

We present celmech, an open-source Python package designed to facilitate a wide variety of celestial mechanics calculations. The package allows users to formulate and integrate equ…

astro-ph.EP2022

The Effects of Disk Induced Apsidal Precession on Planets Captured into Mean Motion Resonance

Zachary Murray, Sam Hadden, Matthew J. Holman

The process of migration into resonance capture has been well studied for planetary systems where the gravitational potential is generated exclusively by the star and planets. Howe…

astro-ph.EP2021★ 19 cited

The Criterion for Chaos in Three-Planet Systems

Jeremy Rath, Sam Hadden, Yoram Lithwick

We establish the criterion for chaos in three-planet systems, for systems similar to those discovered by the Kepler spacecraft. Our main results are as follows: (i) The simplest cr…

astro-ph.EP2021★ 25 cited

Rare Event Sampling Improves Mercury Instability Statistics

Dorian S. Abbot, Robert J. Webber, Sam Hadden +2

Due to the chaotic nature of planetary dynamics, there is a non-zero probability that Mercury's orbit will become unstable in the future. Previous efforts have estimated the probab…

astro-ph.EP2021★ 23 cited

How Close are Compact Multi-Planet Systems to the Stability Limit?

Samuel W. Yee, Daniel Tamayo, Samuel Hadden +1

Transit surveys have revealed a significant population of compact multi-planet systems, containing several sub-Neptune-mass planets on close-in, tightly-packed orbits. These system…

astro-ph.EP2021★ 1 cited

Significant improvement in planetary system simulations from statistical averaging

David M. Hernandez, Eric Agol, Matthew J. Holman +1

Symplectic integrators are widely used for the study of planetary dynamics and other -body problems. In a study of the outer Solar system, we demonstrate that individual symplec…

astro-ph.EP2021★ 3 cited

A Bayesian neural network predicts the dissolution of compact planetary systems

Miles Cranmer, Daniel Tamayo, Hanno Rein +5

Despite over three hundred years of effort, no solutions exist for predicting when a general planetary configuration will become unstable. We introduce a deep learning architecture…

astro-ph.EP2020★ 26 cited

Mildly-Hierarchical triple dynamics and applications to the outer solar system

Hareesh Gautham Bhaskar, Gongjie Li, Sam Hadden +2

Three-body interactions are ubiquitous in astrophysics. For instance, Kozai-Lidov oscillations in hierarchical triple systems have been studied extensively and applied to a wide ra…

astro-ph.EP2020★ 108 cited

Predicting the long-term stability of compact multiplanet systems

Daniel Tamayo, Miles Cranmer, Samuel Hadden +11

We combine analytical understanding of resonant dynamics in two-planet systems with machine learning techniques to train a model capable of robustly classifying stability in compac…

astro-ph.EP2020★ 16 cited

Modeling Radial Velocity Data of Resonant Planets to Infer Migration Histories

Sam Hadden, Matthew J. Payne

A number of giant planet pairs discovered by the radial velocity method with period ratios may reside in mean motion resonances. Convergent orbital migration and reson…

astro-ph.EP2019★ 18 cited

Are long-term -body simulations reliable?

David M. Hernandez, Sam Hadden, Junichiro Makino

-body integrations are used to model a wide range of astrophysical dynamics, but they suffer from errors which make their orbits diverge exponentially in time from the correct o…

astro-ph.EP2019★ 41 cited

An Integrable Model for the Dynamics of Planetary Mean Motion Resonances

Sam Hadden

I consider the dynamics of mean motion resonances between pairs of co-planar planets and derive a new integrable Hamiltonian model for planets' resonant motion. The new model gener…

astro-ph.EP2019★ 135 cited

The L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf

Veselin B. Kostov, Joshua E. Schlieder, Thomas Barclay +112

We report the Transiting Exoplanet Survey Satellite (TESS) discovery of three terrestrial-sized planets transiting L 98-59 (TOI-175, TIC 307210830) -- a bright M dwarf at a distanc…

astro-ph.EP2019★ 42 cited

Near-resonance in a system of sub-Neptunes from TESS

Samuel N. Quinn, Juliette C. Becker, Joseph E. Rodriguez +78

We report the Transiting Exoplanet Survey Satellite () detection of a multi-planet system orbiting the K0 dwarf TOI 125. We find evidence for up to five planets, wit…

astro-ph.EP2018★ 24 cited

Prospects for TTV Detection and Dynamical Constraints with TESS

Sam Hadden, Thomas Barclay, Matthew J. Payne +1

We consider the potential for the Transiting Exoplanet Survey Satellite (TESS) to detect transit timing variations (TTVs) during both its nominal and extended mission phases. Build…

astro-ph.EP2018★ 9 cited

Prospects for Refining Kepler TTV Masses using TESS Observations

Max Goldberg, Sam Hadden, Matthew J. Payne +1

In this paper we investigate systems previously identified to exhibit transit timing variations (TTVs) in Kepler data, with the goal of predicting the expected improvements to the…

astro-ph.EP2018★ 52 cited

A Compact Multi-Planet System With A Significantly Misaligned Ultra Short Period Planet

Joseph E. Rodriguez, Juliette C. Becker, Jason D. Eastman +20

We report the discovery of a compact multi-planet system orbiting the relatively nearby (78pc) and bright () K-star, K2-266 (EPIC248435473). We identify up to six possible p…

astro-ph.EP2018★ 24 cited

The Secular Dynamics of TNOs and Planet Nine Interactions

Gongjie Li, Samuel Hadden, Matthew Payne +1

The existence of Planet Nine has been suggested to explain the pericenter clustering of extreme trans-Neptunian objects (TNOs). However, the underlying dynamics involving Planet Ni…