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Density Matters 2024:
Uncovering the Formation, Interior Structure
and Evolution of Small Exoplanets

Short Info

February 5-9th 2024

Ringberg Castle, Tagungsstätte der Max-Planck-Gesellschaft, Schlossstrasse 20, 83708 Kreuth, Bavaria, Germany. Directions can be found on the Webpage of Schloss Ringberg.

The conference format was that of a workshop with multiple working groups focusing on specific topics. The major topics were:

  1. Formation and Evolution
  2. Internal Structure
  3. Atmospheres
  4. Demographics
There was be ample time for collaborative work.

From the concluding discussion, the participants agreed on the following messages for the broader community.

  1. Sub Neptunes are the most dominant exoplanet population known to date
  2. JWST is capable of detecting the atmospheres of sub Neptunes
  3. There are multiple scenarios capable of explaining the current observations. We need a) more observations and b) testable predictions and contextual factors
  4. There is a need for models coupling the interior and atmosphere while accounting for evolution processes
  5. There is a need for laboratory work and experimental data including
    • Equations of State at high temperatures and pressures
    • Material properties
    • Line lists and continuum emission/absorption
    • Chemical reaction rates
    Theoretical sensitivity studies need to quantifiy the importance of these model ingredients.
  6. Intrinsic distributions of fundamental planetary properties would be very useful for answering important population-level questions.

What is the main direction where research is required to understand the nature of small exoplanets (Earths to sub Neptunes)?

Replies from participants to
Among the participants, we conducted a survey powered by sci-an where we asked about the future directions. The 29 free format replies were automatically categorized into pre-defined categories listed above. Individual quotes selected by me exemplify the replies. In particular, interdisciplinary research, such as the link to geology and atmospheric physics, was stressed.

Individual, anonymous quotes by participants of the Density Matters 2024 workshop.

"Better coupled atmosphere-interior models, which make testable, observable predictions about what molecules to observe in the atmosphere and how to link these to the interior state"

"How can we go from elemental budgets from formation via realistic interiors to final atmospheres?"

"More work in the lab looking at realistic compositions of sub-Neptune atmospheres and their interiors (e.g. silicates, water, and hydrogen at extremely high temperatures and pressures). Many of our models rely on extrapolations that may not be valid."

Schedule

Conference Abstract Booklet

Registered Participants
Name Organization
Renyu Hu NASA Jet Propulsion Laboratory
Tim Lichtenberg University of Groningen
James Rogers UCLA
Anjali Piette Carnegie Earth & Planets Laboratory
Daria Kubyshkina Space Research Institute, Graz, Austria
Raymond T. Pierrehumbert University of Oxford
Peter Gao Carnegie Earth & Planets Laboratory
Lorena Acuña MPI for Astronomy
Enric Palle Instituto de Astrofisica de Canarias
Thomas Henning MPI for Astronomy
Johanna Teske Carnegie Earth and Planets Lab
James Owen Imperial College London
Remo Burn MPI for Astronomy
Allona Vazan The Open University of Israel
Natalie Batalha UC Santa Cruz
Jo Ann Egger Universität Bern
Eve J. Lee McGill University
Léna Parc University of Geneva
Martin Turbet LMD, IPSL, LAB, CNRS
Björn Benneke University of Montreal
Artem Aguichine University of California, Santa Cruz
Gijs D Mulders Universidad Adolfo Ibáñez, Chile
Octavio Miguel Guilera Astrophysical Institute of La Plata
Shang-Min Tsai UC Riverside
Nikku Madhusudhan University of Cambridge
Nicolas Kaufmann University Bern
Alejandro Sánchez López Instituto de Astrofísica de Andalucía
Jesse Weder University of Bern
Ian Crossfield University of Kansas
Lena Noack Freie Universität Berlin, Germany
Chris Ormel Tsinghua University
William Misener University of California, Los Angeles
Martin Schlecker University of Arizona
Andrin Kessler University of Bern
Matthew Conor Nixon University of Maryland
Joseph M. Akana Murphy University of California, Santa Cruz
Brandon Park Coy University of Chicago
Eva-Maria Ahrer MPI for Astronomy
Chanoul Seo SOKENDAI/NAOJ
Hamish Innes Freie Universität Berlin, Germany
Solène Ulmer-Moll University of Bern and Geneva
María Paula Ronco Instituto de Astrofísica de La Plata
Duncan Christie MPI for Astronomy
Julia Venturini University of Geneva
Jaume Orell Miquel Instituto de Astrofisica de Canarias
Matthäus Schulik Imperial College/UCLA
Ryan Cloutier McMaster University
Jegug Ih University of Maryland
Rafael Luque University of Chicago
Ryan Cloutier McMaster University

SOC

Name Organization
Remo Burn MPIA
Rafael Luque University of Chicaco
Natalie Batalha UC Santa Cruz
Hubert Klahr MPIA
Enric Palle Instituto de Astrofisica de Canarias
Allona Vazan The Open University of Israel
Björn Benneke University of Montreal
Julia Venturini University of Geneva

CONTACT

IN CASE OF QUESTIONS

Feel free to write a mail to densitymatters2024@mpia.de
Max Planck Institut für Astronomie, Office 114, Königstuhl 18, 69117 Heidelberg, Germany