Currently trying to understand planet formation as a professor of astronomy @UWMadison; previously a #51PegasibFellow @Caltech; PhD from @michiganastro

Joined April 2019
In Nick Marston's first first-author paper (accepted now to ApJ, and available here: arxiv.org/abs/2606.11330) he asks the question: do *all* super-puff exoplanets defy the expectations of core accretion? He modeled the interior structures of 34 cold super-puffs...
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...and found that most can be explained within standard core accretion pathways. But 6 planets remain difficult to reconcile even after accounting for system age and internal heat from either impact or radiogenic sources.
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Nick will presenting his work at DDA (dda.aas.org/node/184) in a couple of weeks - if you are attending, make sure to stop by his poster and learn more about these super-puffs that require novel explanations, including one REALLY weird super-puff!
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New first-author paper from Adam Distler, now accepted to ApJ, evaluates whether the inner edges of peas-in-a-pod (PIAP) multiplanet systems are affected by secular resonance crossings driven by the rotational evolution of the host star....
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He finds that PIAP geometries are not susceptible to such secular resonances, and thus will not experience the same redistribution of angular momentum deficit that can drive the emergence of mutual inclination in systems with larger (/non-equal) period ratios....
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New ApJ paper: Can inner planets survive when a giant becomes a hot/warm Jupiter via high-eccentricity tidal migration? Usually no. Survival requires the giant’s periastron to stay >14 mutual Hill radii away. Observed systems with hot Jupiters + inner planets are inconsistent...
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AbSciCon will be in Madison, WI in May 2026! Please consider submitting an abstract to session 39, Dynamical Environments of Habitable Worlds, led by Joseph Livesey. Hope to see you all there!
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Mean motion resonances (familiar from planetary systems) also govern how stellar-mass BHs migrate and merge in AGN disks. Marguerite Epstein-Martin (applying to postdocs THIS FALL) has a new paper “Mean Motion Resonances in AGN Disks” (arxiv.org/abs/2510.12895v1).
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Marguerite's previous work spans time-evolution of AGN disks to secular resonances in young protoplanetary disks. In this new paper, she computes where in AGN disks stellar-mass BH binaries may survive, and when they will be stochastically forced out of resonance.
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Some hot Jupiters might not have traveled far. New simulations by UW-Madison recent undergrad alum Devansh Mathur show that if enough solid material is funneled inward, both a hot Jupiter and its inner companions could form in situ. Accepted to PASP: arxiv.org/abs/2510.13527v1
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At the University of Wisconsin–Madison, we are excited to host 51 Pegasi b Fellows in the Department of Astronomy! Applications are due October 3, 2025. This was the fellowship that I had as a postdoc, and I’d be happy to chat if you think you might be interested in applying!
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Two weeks until abstracts (and requests for travel support) are due for this fall's GLEAM! gleam.astro.wisc.edu/overvie… I hope to see you here!
We’re so happy to host GLEAM 2025 at UW–Madison this Fall, Nov 6–7! gleam.astro.wisc.edu/ Join us for two days of exoplanets & community with a view of the shores of Lake Mendota. No registration fee. Travel support available. Abstracts & Travel Support Requests due Sept 5th.
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We’re so happy to host GLEAM 2025 at UW–Madison this Fall, Nov 6–7! gleam.astro.wisc.edu/ Join us for two days of exoplanets & community with a view of the shores of Lake Mendota. No registration fee. Travel support available. Abstracts & Travel Support Requests due Sept 5th.
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