activity
20242026
collaborators

10 papers

astro-ph.EP2026

On the Secular Evolution of Inclinations Among the Classical Belt TNOs

Dallin Spencer, Darin Ragozzine, Kat Volk +1

Proper orbital elements have been used in diverse ways to study the dynamical architecture of transneptunian objects (TNOs), providing insights into Solar System evolution and migr…

astro-ph.EP2026

Producing planetary debris exterior to white dwarf Roche radii through sublimative rotational fission

Dimitri Veras, Jordan K. Steckloff, Kathryn Volk

The majority of white dwarfs that host periodic transiting planetary debris do so at distances that exceed the rubble-pile Roche limit, in disagreement with canonical formation mod…

astro-ph.EP2026

Small Body Dynamics with SBDynT: Proper Elements and Chaos Analysis

Dallin Spencer, Kat Volk, Darin Ragozzine +1

The Small Body Dynamics Tool (SBDynT) is software written for the community of Solar System small body researchers to perform dynamical classification, characterization, and invest…

astro-ph.EP2025

LiDO: Discovery of a 10:1 Resonator with a Novel Libration State

Rosemary E. Pike, Ruth Murray-Clay, Kathryn Volk +9

The Large inclination Distant Objects LiDO survey has discovered the first securely classified object in the 10:1 mean motion resonance of Neptune. This object, 2020 VN40, is short…

astro-ph.EP2025

Predictions of the LSST Solar System Yield: Discovery Rates and Characterizations of Centaurs

Joseph Murtagh, Megan E. Schwamb, Stephanie R. Merritt +16

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will start by the end of 2025 and operate for ten years, offering billions of observations of the southern nigh…

astro-ph.EP2024

Forcing Planets to Evolve: Interactions Between Uranus and Neptune at Late Stages of Dynamical Evolution

Arcelia Hermosillo Ruiz, Ruth Murray-Clay, Kathryn Volk +1

In early Solar System numerical simulations, where chaos is a primary driver, it is difficult to explore parameter space in a systematic way. In such simulations, stable configurat…

astro-ph.EP2024

Machine Learning Assisted Dynamical Classification of Trans-Neptunian Objects

Kathryn Volk, Renu Malhotra

Trans-Neptunian objects (TNOs) are small, icy bodies in the outer solar system. They are observed to have a complex orbital distribution that was shaped by the early dynamical hist…

astro-ph.EP2024

Jupiter Co-Orbital Comet P/2023 V6 (PANSTARRS): Orbital History and Modern Activity State

Theodore Kareta, John W. Noonan, Kathryn Volk +2

The discovery of the transient Jupiter co-orbital comet P/2019 LD2 (ATLAS) drew significant interest. Not only will LD2 transition between being a Centaur and a Jupiter Family Come…

astro-ph.EP2024

Differences between Stable and Unstable Architectures of Compact Planetary Systems

Kathryn Volk, Renu Malhotra

We present a stability analysis of a large set of simulated planetary systems of three or more planets based on architectures of multiplanet systems discovered by \textit{Kepler} a…

astro-ph.EP2024

Uranus's influence on Neptune's exterior mean motion resonances

Severance Graham, Kathryn Volk

Neptune's external mean motion resonances play an important role in sculpting the observed population of transneptunian objects (TNOs). The population of scattering TNOs are known…