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
Physicist/planetary scientist/astrobiologist based at Harvard. Soccer dad in training. Social media native since 2024.
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.
yes, collision broadening is included
26.07.2025 22:41 β π 0 π 0 π¬ 0 π 0Cool, thanks for sharing!
26.07.2025 22:40 β π 0 π 0 π¬ 0 π 0π§ͺ I'm a fan of this way of interacting with vibrational spectra. I did this on my blog a while ago: nanoscale.blogspot.com/2015/06/what...
26.07.2025 15:10 β π 3 π 1 π¬ 1 π 0If 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.
Now on @sciam.bsky.social, by @nadiadrake.bsky.social:
The U.S. has axed CMB-S4, its boldest cosmology experiment in generations. Tight budgets and crumbling infrastructure helped doom the project, which was meant to test cosmic inflation. RIP.
www.scientificamerican.com/article/u-s-...
Direct evidence for tectonics (of some kind!) 3.5B years ago. The timeline keeps moving back. Nice find by @alexwilkins.bsky.social at Goldschmidt.
15.07.2025 21:35 β π 30 π 8 π¬ 1 π 0A lab experiment that simulated Mars conditions showed that green algae can grow in plastic containers made from the same algae, setting the stage for a self-sustaining system to build habitats on the planet.
03.07.2025 08:38 β π 11 π 4 π¬ 2 π 2Thanks! 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.
18.06.2025 12:41 β π 1 π 0 π¬ 1 π 0On 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
16.06.2025 15:15 β π 3 π 1 π¬ 0 π 0I 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.
16.06.2025 17:52 β π 1 π 0 π¬ 1 π 0New work led by Jess Cmiel finds that planets with steam atmospheres may be cooler β much cooler β at the surface than we previously thought.
β¨β¨iopscience.iop.org/article/10.3...β¨
arxiv.org/abs/2505.00775
This supports and extends conclusions published last year by Selsis et al. in Nature. π π§ͺ
The abstract submission for Rocky Worlds 4 is now open! groningen2026.rockyworlds.org/registration... πππ§¬π±
02.06.2025 10:59 β π 12 π 7 π¬ 0 π 0The resurfacing is very episodic but itβd still be pretty bad in a period of peak activity. Then in the good times youβd have slimy microbial mats as far as the eye could see. No skyr or harΓ°fiskur, unfortunately.
02.06.2025 23:00 β π 0 π 0 π¬ 1 π 0It'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.
02.06.2025 15:24 β π 2 π 0 π¬ 0 π 0These βlarge igneous provincesβ have formed a few times in Earth history and are terrifying β imagine a huge chunk of the surface turning into Mordor in a geologic blink of the eye
02.06.2025 14:53 β π 4 π 0 π¬ 1 π 0What 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....
π π§ͺ
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
Proposed NASA cuts in context, courtesy of the Planetary Society #astronomy #science
02.05.2025 16:47 β π 101 π 47 π¬ 3 π 3very happy to chat if you're interested in working on this!
22.04.2025 23:43 β π 2 π 0 π¬ 1 π 0yes, we include atmosphere-mantle interaction, although only the magma ocean phase for the moment. things get complicated once the melt solidifies!
22.04.2025 20:59 β π 1 π 0 π¬ 1 π 0This all feels very on topic for Earth Day
22.04.2025 19:45 β π 3 π 1 π¬ 0 π 0Thanks! The point is that if we want to use O2 as a biosignature, we first need to understand how abiotic planets evolve, which means starting with the hot close-in targets.
22.04.2025 16:36 β π 4 π 0 π¬ 1 π 0Sub-Neptunes shrink and oxidize as they cross the radius valley and become rocky planets, in a new paper led by Collin Cherubim
arxiv.org/pdf/2503.05055
#astronomy #science
I'm excited to announce that my first solo-author paper has been accepted at ApJ: arxiv.org/abs/2502.19394. I study the dependence of hot Jupiter circulation on both the temperature and wind initial conditions building upon Liu & Showman (2013), finding that the circulation of typical HJ is robust.
27.02.2025 13:50 β π 30 π 5 π¬ 1 π 0The Planetary Society strongly opposes the sudden, indiscriminate dismissal of more than 1,000 scientists, engineers, and explorers at NASA β the largest involuntary workforce reduction since the end of the Apollo program.
Read more on our stance. β¬οΈ
Our new Nature Geoscience paper led by Danica Adams is now published:
www.nature.com/articles/s41...
Water-rock chemistry released hydrogen and helped make early Mars habitable to microbial life.
We'll be able to test this idea directly once we can study Mars rocks here on Earth.
Our new paper led by Jake Seeley on clouds and convection in H2-dominated atmospheres is out! Technical conclusion: Things get weird when nitrogen is no longer the background gas π§ͺπ
iopscience.iop.org/article/10.3...
arxiv.org/abs/2412.06648