Dr Joanna Barstow
@drjovian.bsky.social
850 followers 360 following 1.1K posts
STFC Ernest Rutherford Fellow at the Open University. Astromum x 2. FRAS. Christian, singer, bookworm, musical theatre super fan.
Posts Media Videos Starter Packs
drjovian.bsky.social
I’m definitely with you there! Innovation requires brains that have learned to think creatively. If we outsource our thinking to computers what will that result in long term?
drjovian.bsky.social
Absolutely. Writing good papers also requires creativity IMO. At the end of the day it’s all about storytelling.
drjovian.bsky.social
That was my immediate reaction too Chris. Sure, it’s expected in hydrogen dominated atmospheres for certain temperatures (so seeing it in a brown dwarf is cool but far from shocking). It’s still very much not expected in a CO2 or N2 dominated atmosphere. Caution always good, but context important!
drjovian.bsky.social
It turns out the mob sing: ‘We don’t like what we don’t understand - in fact it scares us .’ Followed shortly after by cries to bring guns/knives and kill the Beast.

I feel like these lyrics are pretty key to the current shitshow we live in. Also, Howard Ashman was a genius.
drjovian.bsky.social
I’m in an amateur production of Beauty and the Beast and in rehearsals last week we got around to learning/setting the Mob Song (the one with repeated calls to ‘Kill the Beast!’) I confess I never paid much attention to the details of the lyrics in the film…
Reposted by Dr Joanna Barstow
pogglerebecca.bsky.social
If you don't know what's going on with anti-trans stuff in the UK, read this.

If you're similarly disgusted with the way anti-trans people have gotten away with demonising and assaulting an innocent minority, send this to your friends, family and MP to demand change.

They won't stop with us.
drjovian.bsky.social
I don’t think there is an official repository yet. It would be excellent if it was part of the NASA Exoplanet archive but I think that would require an awful lot of investment they probably can’t make at the moment.
drjovian.bsky.social
I had lots of fun last week recording a podcast episode for our OpenLearn team, which meant i got to wave my hands around a lot whilst talking about everything exoplanets - and of course, Habitable Worlds Observatory got an honourable mention. youtu.be/KXbo6OAKfoI?...
OpenLearn Podcast #3: Looking for life on exoplanets with Dr Jo Barstow
YouTube video by OpenLearn from The Open University
youtu.be
drjovian.bsky.social
It’s about the difficulties a younger sibling has with everything the family does being about his brother. It might not all be a comfortable watch. But it is very well done.
drjovian.bsky.social
There was a TV drama a few years ago called Coming Down the Mountain that was very good. Not sure if it was ever a book.
drjovian.bsky.social
That's a wrap folks, #HWO25 is done! In 20 years I'll be posting on whatever social media platform then exists about Earthlike planet detections and maybe even signs of life 👀
drjovian.bsky.social
Gupta: warmer planet T-p profiles lie completely in the miscible region. As a planet cools, eventually it will intersect the critical curve, and condensate clouds will emerge. Later there is deep 'rainfall' inside the planet, leading to water deep in the interior. TOI-270d too hot for this! #HWO25
drjovian.bsky.social
Gupta: these simulations can help determine the critical curve defining the regions of pressure-temperature space where water is miscible in all proportions, and regions where hydrogen and water are only partially miscible. Uranus and Neptune have T-p profiles strikingly close to this curve. #HWO25
drjovian.bsky.social
Gupta: insights into atmosphere-interior interactions are critical for interpreting HWO data. Lab experiments at relevant conditions are very hard though! Quantum mechanical methods (ab initio molecular dynamics) can help us understand interactions between hydrogen and water. #HWO25
drjovian.bsky.social
Now our final talk, by Akash Gupta on the story of hydrogen and water - new insights into the interaction of planet atmospheres and interiors. Planet formation entails interaction of hydrogen envelope with interior - are these important? Yes - likely impact structure and thermal evolution #HWO25
drjovian.bsky.social
Gialluca: however, there are big errors on estimated crater size with impactor energy. We need to do much more impact testing to understand this better. We therefore don't want a ~25 planet sample, this might end up being reduced by 50%, so we need contingency/conservative sample sizes #HWO25
drjovian.bsky.social
Gialluca: in general impactors only start affecting yield if the energy is greater than 0.2 J. For a ~26J impactor similar to the JWST C3 impactor, this could result in a ~30% reduction in yield. #HWO25
drjovian.bsky.social
Having a telescope barrel reduces stray light in two ways, it minimises the risk of impacts and minimises incident stray light from background sources. For high energy impactors, the background source improvement isn't that great, but it does protect against impacts happening in the 1st place #HWO25
drjovian.bsky.social
Gialluca: this work provides order of magnitude estimates of stray light from these rare, high energy impact events. Two models exist for predicting crater size for a given impact - give different answers, so we have an optimistic to pessimistic range of possible sizes. #HWO25
drjovian.bsky.social
Now we have Megan Gialluca on assessing the impact of stray light due to micrometeoroid damage. Micrometeoroid damage is unavoidable for space missions. JWST has seen a rate of a couple per month, consistent with pre-launch expectations - excepting the high energy event on the C3 mirror #HWO25
drjovian.bsky.social
Wolff: shorter correlated noise lengthscales produce the widest posteriors, and shortest lengthscales match the width of absorption lines. E.g. oxygen posteriors can be biased here. PSF chromaticity produces correlated noise at these length scales. This will be a limiting noise source for HWO #HWO25
drjovian.bsky.social
Wolff: speckle noise can be modelled using Gaussian processes, simply specified by an amplitude and length scale. Failing to model correlated noise in retrievals biases and artificially narrows posteriors. Most retrieval studies for HWO trade space do not yet account for speckle noise. #HWO25
drjovian.bsky.social
Now we have Nicole Wolff talking about impacts of correlated noise on retrievals of exo-Earth atmospheres. Direct images contain chromatic speckles that move radially outward with wavelength. They are a source of spectrally correlated noise coupling adjacent wavelength bins. #HWO25
drjovian.bsky.social
Stuber: hot exozodi could reduce HWO's performance drastically, but we don't know much detail about it yet. So every estimate of yield is highly uncertain and subject to this! #HWO25