Robin Wordsworth
@rdword.bsky.social
320 followers 100 following 31 posts
Physicist/planetary scientist/astrobiologist based at Harvard. Soccer dad in training. Social media native since 2024.
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Reposted by Robin Wordsworth
lkreidberg.bsky.social
Update on the atmosphere vs no atmosphere debate for TRAPPIST-1 b and c -- here's a nice and (IMO) conclusive result from Gillon and Ducrot et al.: no thick atmosphere on either planet. arxiv.org/pdf/2509.02128
arxiv.org
Reposted by Robin Wordsworth
maxplanck.de
The #MaxPlanckPostdocProgram offers a guaranteed contract of at least 3 years, targeted mentoring, and career workshops. The call for applications is open now! 🚀 Take advantage of this opportunity and browse the job vacancies. www.mpg.de/en/max-planc...
Group photo of postdocs conducting research at a Max Planck Institute
Reposted by Robin Wordsworth
rockyworlds.bsky.social
#RockyWorldsDiscussion is back from our summer break! 🔭🧪

Our next speaker is Laura Schaefer from Stanford University, who will tell us about redox gradients in planet formation simulations of terrestrial planets 🌍🌕🪨 Join us on Zoom on Thu 4 Sep @ 16:00 UTC

More: www.rockyworlds.org/event-detail...
An image of the speaker, Laura Schaefer. She is smiling and looking into the camera. She is wearing a purple-grey zip-up jumper and sunglasses on her head. She is against a background of a large rock with some grass visible near the bottom, clearly outdoors. An artistic conception of early Earth showing the planet's surface impacted by asteroids. Earth is shown with partial oceans and the land that is visible is covered in clear craters. Part of the Earth (bottom left) is also shown as covered by lava or a magma ocean.

Image credit: Simone Marchi, NASA. Taken from https://www.scientificamerican.com/article/early-earth-s-atmosphere-was-surprisingly-thin/
rdword.bsky.social
I've stuck a few more here:

people.seas.harvard.edu/~rwordsworth...

The CO rotational band makes a nice bass. Ozone is straight out of 60's Star Trek. And ammonia and water are terrifying.
rdword.bsky.social
yes, collision broadening is included
rdword.bsky.social
Cool, thanks for sharing!
rdword.bsky.social
If you could hear in the infrared, what would CO2 sound like? We calculated this recently for a Gen Ed course, and the result is a little eerie.

Results were generated by mapping IR frequency in inverse cm to sound frequency in Hz.
Reposted by Robin Wordsworth
rdword.bsky.social
Thanks! Our simulations aren't quite in the same regime as Venus, but we separately used the model to recreate Venus's temperature profile and it did pretty well. We found it was right on the edge of convective instability in Venus's lower atmosphere, interestingly.
Reposted by Robin Wordsworth
climatebook.bsky.social
On a related note, we found that convective shutdown by the same mechanism can drastically shorten primordial magma ocean freeze-out times, though with enough irradiation there can be persistent magma oceans despite convective shutdown. arxiv.org/abs/2412.11987
Convective shutdown in the atmospheres of lava worlds
Atmospheric energy transport is central to the cooling of primordial magma oceans. Theoretical studies of atmospheres on lava planets have assumed that convection is the only process involved in setti...
arxiv.org
rdword.bsky.social
I mean yeah pretty worried, of course : ). The problem with the continuum in the visible is that we need really long path lengths and/or sensitive measurements, which means $$$ for experiments. Maybe ab initio can help, although H2O is a tough molecule to simulate.
rdword.bsky.social
New work led by Jess Cmiel finds that planets with steam atmospheres may be cooler — much cooler — at the surface than we previously thought.



iopscience.iop.org/article/10.3...
arxiv.org/abs/2505.00775

This supports and extends conclusions published last year by Selsis et al. in Nature. 🔭 🧪
Characterizing the Radiative–Convective Structure of Dense Rocky Planet Atmospheres - IOPscienceSearch
Characterizing the Radiative–Convective Structure of Dense Rocky Planet Atmospheres, Cmiel, Jessica, Wordsworth, Robin, Seeley, Jacob T.
iopscience.iop.org
rdword.bsky.social
The resurfacing is very episodic but it’d still be pretty bad in a period of peak activity. Then in the good times you’d have slimy microbial mats as far as the eye could see. No skyr or harðfiskur, unfortunately.
rdword.bsky.social
It's a fascinating question. Global temperature matters a lot, but so do other factors like total area and latitude (equatorial LIPs weather fastest due to higher rainfall rates). If e.g. Brazil was turned into a LIP today, that could well trigger a Snowball.
rdword.bsky.social
These ‘large igneous provinces’ have formed a few times in Earth history and are terrifying — imagine a huge chunk of the surface turning into Mordor in a geologic blink of the eye
rdword.bsky.social
What does it take to turn Earth into a Snowball? Formation of a volcanic plateau about the size of India at the equator, according to our new study led by Charlotte Minsky:

agupubs.onlinelibrary.wiley.com/doi/epdf/10....

🔭 🧪
rdword.bsky.social
Interesting paper by Yang et al. on arxiv today arguing clouds might _help_ us observe O2/O3 on exoplanets in some cases:

arxiv.org/pdf/2505.07760
arxiv.org
rdword.bsky.social
Proposed NASA cuts in context, courtesy of the Planetary Society #astronomy #science
rdword.bsky.social
very happy to chat if you're interested in working on this!