Tim Lichtenberg

@timlichtenberg.bsky.social

Assistant Professor of Planetary Physics at Kapteyn Astronomical Institute, University of Groningen 🇪🇺 he/him | formingworlds.space | born at 351 ppm

I really enjoyed this collaboration: it goes to show that especially in the sciences, where data remains costly, Bayesian approaches like BO, BAL, and BED can make a difference. Also, I guess this is officially my first astrophysics paper, very exciting! 🔭🪐🌌

Forming Worlds Lab@formingworlds.space · last wk.

Harrison worked closely with our group all through his PhD, and still does. His new paper asks what you can learn about an exoplanet by fitting its whole life instead of a snapshot of today. 🔭 https://arxiv.org/abs/2607.25845 #Exoplanets #PlanetaryScience

New paper on arXiv today! On the efficacy of using novel Bayesian machine learning to dispatch 'expensive' forward models of planetary evolution. This connects with #PLATO ageing and can help solve degeneracies in current static-retrieval approaches which treat #exoplanets as snapshots.

Constraining the lives and times of exoplanets through evolutionary Bayesian retrievals

Static retrieval frameworks are leading tools for interpreting exoplanet observations, yet time-independent modelling leaves them prone to degeneracy and unable to resolve exoplanets' histories. The c...

arxiv.org

Harrison worked closely with our group all through his PhD, and still does. His new paper asks what you can learn about an exoplanet by fitting its whole life instead of a snapshot of today. 🔭 https://arxiv.org/abs/2607.25845 #Exoplanets #PlanetaryScience

Harrison Nicholls@nichollsh.bsky.social · last wk.

New paper on arXiv today! On the efficacy of using novel Bayesian machine learning to dispatch 'expensive' forward models of planetary evolution. This connects with #PLATO ageing and can help solve degeneracies in current static-retrieval approaches which treat #exoplanets as snapshots.

New paper with @formingworlds.space colleagues. With planetary evolution models, we demonstrate that the combined physics of redox-sensitive degassing and escape can generate transient episodes of atmospheric re-inflation on super-Earths. "Reflation" is an observational marker of reducing interiors.

Forming Worlds Lab@formingworlds.space · 3w ago

New paper led by Lorenzo Cesario, his second first-author paper from his MSc 🌍 Some close-in super-Earths puff their atmospheres back up late in life instead of only shrinking. We call it reflation. Read the paper: https://arxiv.org/abs/2607.13793 #Exoplanets #PlanetaryScience

Schematic comparing oxidised (blue, top) and reduced (red, bottom) super-Earth atmospheres evolving over time. Three planets shrink from left to right under XUV irradiation arrows driving escape to space. Reduced atmospheres are rich in CO and hydrogen with water; oxidised atmospheres in CO2, CO and water, with SO2 appearing later. The reduced planet swells before shrinking, illustrating the reflation mechanism.

🔭 The amazing Claire Marie Guimond @xoplanets.bsky.social is so good at explaining all things (exo)geoscience! 🌋🌍 I learned so much in this A+ interview about… night-side volcanism?! Where energy dissipates through tidally-locked #exoplanets from molten dayside ➡️ volcanoes form on the other side! 🤯

SETI Institute@setiinstitute.bsky.social · 3mo ago

ICYMI, this week's SETI Live focused on a rocky, tidally locked world with possible lava oceans. Designated K2-141 b, researchers used models to determine how heat moves through the planet’s interior. Watch the full interview: youtube.com/live/nYX2sNg... 🧪 🔭 👩‍🔬

My 25th (!) newsletter post shares my main takeaway from the #RockyWorlds4 conference: Hot rocks are what's cool in rocky exoplanet research right now. Lava planets, especially look like they're about to teach us a *ton* about how rocky planets work. So come on in, the lava's fine! 🧪🔭

Hot rocks are what's cool in rocky exoplanet research

Habitable zone? Pfft. For exciting planetary science discoveries, keep your eye on lava worlds and hot rocks.

reviewertoo.com

Another cool result shared at #RockyWorlds4: Nearly all sub-Neptunes, if they are gas dwarfs (as opposed to water worlds), should have magma oceans beneath their hydrogen atmospheres. That includes the notorious K2-18b — if it is indeed a gas dwarf and not an ocean planet. Preprint:

Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets

Sub-Neptunes are the most common type of detected exoplanet, yet their observed masses and radii are degenerate with several interior structures. One possibility is that sub-Neptunes have silicate/iro...

arxiv.org