Hi all! If you are looking for a conference in exoplanet interiors in 2026, check out "Layers of Understanding: Model Intercomparisons of Exoplanet Interiors": layersofunderstanding2026.github.io
It will take place in MPIA's campus in April 13-17th. The registration deadline is 15 January 2026
05.12.2025 09:37 β π 7 π 6 π¬ 1 π 0
A bright white object glowing with green tones against a dark, starry space backdrop. The text "3I/ATLAS Facts, not fiction" appears on the image.
The interstellar visitor 3I/ATLAS βοΈ cruising through our Solar System is no alien spaceship and won't hit Earth.
Still, the buzz around it is far from unfounded π€©
Discover why with #ChasingStarlight: https://www.youtube.com/watch?v=YtiqLxfSiVI
π π§ͺ
05.12.2025 10:03 β π 35 π 12 π¬ 0 π 2
A schematic for the interior structure of sub-Neptunes. Moving radially outwards from the planetary centre: the βinteriorβ is defined as the region interior to the binodal surface. At the binodal, a phase change occurs as the convective, miscible, hydrogenβsilicate fluid speciates into gas and melt phases. The region above the binodal is defined as the βenvelopeβ. The silicate vapour introduces a mean molecular weight gradient, which can inhibit convection. In this case, heat is transported via conduction and radiative diffusion. Silicate-rich melt droplets rain-out to rejoin the interior. Continuing to move radially outwards, the envelope becomes unstable to convection and the gas become progressively more hydrogen-rich. The very upper region of the envelope is almost pure hydrogen gas, and heat is transported by radiative diffusion. Radiative-convective boundaries (RCBs) are shown as white dashed lines.
Published in #MNRAS: "Redefining interiors and envelopes: hydrogenβsilicate miscibility and its consequences for the structure and evolution of sub-Neptunes", Rogers et al. This is Fig. 2: for the caption & to read the paper please visit academic.oup.com/mnras/articl...
05.12.2025 10:06 β π 5 π 2 π¬ 0 π 1
A note on learning physics βοΈ for starting PhD students:
At the risk of saying something completely useless because everyone has it worked out
There is no magic trick, your classmates *may* be faster than you, but they are still studying as long as they need to and you are quite capable of the same
04.12.2025 21:18 β π 428 π 71 π¬ 7 π 23
This is great news that Roman Space Telescope ππ is functionally completed! Still some testing, and then Roman will move the Kennedy to be mated with the launch vehicle. Roman is a wide-field Hubble - exciting!
04.12.2025 20:21 β π 71 π 14 π¬ 1 π 0
Here's the aftermath of the Zhuque-3 landing impact.
04.12.2025 06:36 β π 30 π 8 π¬ 2 π 1
π’ Don't forget to join us for this talk tomorrow (Thursday)!
14:00 UTC = 15:00 CET = 09:00 EST = 06:00 PST = 23:00 JST
If you haven't signed up to our mailing list to access the Zoom-link, you can also watch it live on our YouTube channel πβοΈπ§ͺ Livestream: www.youtube.com/watch?v=e2jI...
03.12.2025 13:59 β π 1 π 1 π¬ 0 π 0
Our #MarsExpress spots a strange shape on Mars, formed as a space rock collided with the planet's dusty surface.
It's known as a 'butterfly crater' but we see a walnut, an insect, the Eye of Sauron, or perhaps a moth... what do you think?
More info and images π www.esa.int/Science_Expl...
π π§ͺ
03.12.2025 10:38 β π 151 π 28 π¬ 8 π 5
Interested in finding transiting planets at long periods, e.g. with the @platomissioncon.bsky.social?
We just published a Research Note led by Geert Jan Talens, showing that such transits can be much longer or shorter than usually assumed iopscience.iop.org/article/10.3...
03.12.2025 12:21 β π 21 π 9 π¬ 1 π 0
I have eaten
the planets
that were in
the inner solar system
and which
you were probably
saving
for living on
Forgive me
they were delicious
so crunchy
and so warm
02.12.2025 16:42 β π 121 π 44 π¬ 4 π 0
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In ApJ today! Understanding the Origins of Super-puff Planets
iopscience.iop.org/article/10.3...
Main parts:
1) First sub-Neptune thermal evolution models to self-consistently couple to a hydrodynamic mass loss code.
2) The finding of a new XUV-driven mass-loss regime, "TEMP," for all sub-Neptunes
02.12.2025 18:54 β π 13 π 5 π¬ 2 π 0
ALMA has captured extremely detailed radio images of the turbulent atmosphere of a dying star π‘ π
It observed tens of molecular spectral lines, each one revealing a different atmospheric layer.
Read more: www.almaobservatory.org/en/press-rel...
02.12.2025 14:44 β π 48 π 13 π¬ 1 π 4
The Edge of Space-Time: Particles, Poetry and the Cosmic Dream Boogie cover on a neon rainbow background. This cover is black background with a central image that is half Black and white circular pattern and half neon rainbow circle. Beneath the cover it says UK: 7 May 2026.
π π π UK & EUROPE COVER REVEAL π π π
The Edge of Space-Time is coming to European readers via UK publisher @canongate.co.uk on 7 May 2026! With a slightly different subtitle π
Preorders now open! Please support your local indie. It helps authors so much!
buythebook.online/edge-of-spac... #BookSky
02.12.2025 15:21 β π 163 π 49 π¬ 3 π 4
It was great getting to share these exciting results as part of the BOWIE+ seminar series. Ariel has the potential to revolutionise our 3D understanding of exoplanet atmospheres, with a phase curve survey of ~100 targets within its reach. Letβs push to make it happen!
02.12.2025 12:11 β π 5 π 2 π¬ 1 π 0
Plot of companion mass vs [Fe/H] from the linked paper. There's a hole around 2 Jupiter masses and 0.2 dex.
Interesting journal club with the Exoplanets group at @physicsuol.bsky.social, looking at the transition from giant planets to brown dwarfs (arxiv.org/abs/2511.11818). They don't mention it, but is the gap at 2-3 MJ & [Fe/H]~0.2 called anything?
If not, I'm calling it the Leicester doughnut hole π
02.12.2025 13:42 β π 9 π 2 π¬ 0 π 0
Hey space Bluesky, I'm looking for an expert on the Moon's formation to comment on a paper I'm reporting on.
If that's you, or you know someone, do let me know. Would be looking to chat later today. Thanks!
jdaoca[at]gmail[dot]com
02.12.2025 06:39 β π 14 π 15 π¬ 1 π 2
Figure caption: (a) Dorsal skin luminance in eastern tree frog (Hyla orientalis) males inhabiting across a gradient of radiation inside (CEZ) or outside the Chornobyl exclusion zone (outside CEZ). (b) Range of dorsal skin luminance in H. orientalis males (from left to right: Luminance values of 5, 20, 30, 40 and 60).
The frogs in question (just because I bloody love frogs): towards the left are the Chernobyl frogs, clearly darker in colour with increased melanin πΈ
β¬οΈ Taken from Fig 2 of βIonizing radiation and melanism in Chornobyl tree frogsβ by Burraco & Orizaola (2022)
onlinelibrary.wiley.com/doi/full/10....
29.11.2025 09:40 β π 4 π 0 π¬ 1 π 0
The mysterious black fungus from Chernobyl that may eat radiation
Mould found at the site of the Chernobyl nuclear disaster appears to be feeding off the radiation. Could we use it to shield space travellers from cosmic rays?
Some #astrobiology reading for a Saturday morning: I really enjoyed this pop sci BBC article on finding biology like mould and frogs (!) adapting to life in radioactive Chernobyl by increasing melanin, i.e. what shields human skin from UV rays π§ͺπ βLife, uh, finds a wayβ
www.bbc.com/future/artic...
29.11.2025 09:34 β π 51 π 16 π¬ 1 π 3
Thatβs an ongoing research Q, but, maybe. Cooler stars may be too active and hotter stars may not live long enoughβ¦ but perhaps βa bitβ hotter/cooler is OK? Until we find life elsewhere, itβs hard to say with our statistical sample of N=1. See eg sec 1.3.1.2. of www.liebertpub.com/doi/10.1089/...
28.11.2025 15:14 β π 4 π 0 π¬ 0 π 0
An image of the speaker, Annelies Mortier. She is smiling and looking into the camera. She has brown hair down to past her shoulders, and is wearing a red top with a silver necklace. She is against a white wall background.
An artistic illustration of Earth and the Sun (not to scale). In the bottom of the right half the image, the top half of the Earth is visible, showing some cloud coverage over parts of North/Central America. In the top of the left half of the image, the Sun is visible as a flaming ball, with bright edges around it and some granulation + bright spots. In the background, a starry sky.
Image credit: Shutterstock
6,000 #exoplanets have been found to date, but ZERO of them are Earth-like planets around Sun-like stars! Why is that? Do any exist? Or is it just hard? βοΈππ
Join us on Thu 4 Dec @ 14:00 UTC for a #RockyWorldsDiscussion with Annelies Mortier to find out!
More: www.rockyworlds.org/event-detail... βοΈπ§ͺ
28.11.2025 13:36 β π 14 π 2 π¬ 1 π 1
YouTube video by BOWIE+ Seminars
Eclipse Mapping with Ariel: Future Prospects for a Population-Level Mapping Survey
Dan Valentine (@danvalentine.bsky.social) has done some great work looking at using ARIEL to eclipse map exoplanet atmospheres. #exoplanets #astronomy
www.youtube.com/watch?v=lrtL...
28.11.2025 08:54 β π 8 π 2 π¬ 0 π 2
Did you just sayβ¦ bock-*ember*? π₯π
27.11.2025 19:49 β π 13 π 0 π¬ 0 π 0
Reading through ESA's draft #CM25 resolution on the level of resources to be committed between now and 2030 - strong support for the proposal to complete #CosmicVision and get #Voyage2050 (M7, L4) underway. Particularly like that line on international flagship partnerships (HabWorlds? Uranus?).
27.11.2025 19:20 β π 6 π 1 π¬ 1 π 0
π The new @esa.int budget secured today is a big deal imho. +30% compared to the current budget with largest chunk going to space transportation ie π. Science/astro is also getting a big bump, which DG Aschbacher called βthe backbone of the ESA programmeβ. Some funding optimism to close off 2025! π«π₯Ή
27.11.2025 19:06 β π 30 π 7 π¬ 1 π 2
CSIRO Industry PhD Program: Information for industry
Tackle your business challenge. Gain access to top research and development expertise while developing the next generation of researchers.
Putting a general call out to my private sector colleagues - would anyone be interested in supporting an industry PhD?
I would love to bring in students to work on imaging/time series problems, especially in space/remote sensing bridging astronomy and other applications.
27.11.2025 08:45 β π 3 π 2 π¬ 0 π 0
Amazing thread: every time we expand the range of what's possible for terrestrial extremophiles, the likelihood life exists elsewhere in the galaxy goes up for me.
25.11.2025 22:34 β π 117 π 24 π¬ 5 π 0
Storm chaser. Volcano hunter. University Physics, Astronomy, & Earth Science Instructor. MS Physics/BS Astrophysics. Rockhounder & Mineral Collector. Raccoon whisperer. Allow me to share our planet's beauty with you. linktr.ee/spahn711
Assistant Astronomer at @spacetelescope.bsky.social researching exoplanet and brown dwarf atmospheres. Opinions expressed are my own.
https://jlothringer.github.io/
Soon: Ultra metal-poor stars at Uppsala University! Current: Stellar analysis pipelines for PLATO and 4MOST. Former Astrobites author. GM, cellist, fiber crafter. More people should care about CMB spectral distortions.
A feed of photos of the Earth from NASA's DSCOVR EPIC camera. Note that this is not an official NASA account.
For more DSCOVR:EPIC information, see epic.gsfc.nasa.gov
Managed by π΄ @redshift.pics
European Space Agency's Climate Team, often posting about ESA's Climate Change Initiative programme - climate.esa.int
The Director General of the European Space Agency
Building crazy planetary systems on my blog planetplanet.net. Solar System formation. Exoplanets. Free-floating planets and interstellar objects. Astronomy poem book: http://amzn.to/3muytqo He/him.
Starplot is a Python library for creating star charts and maps of the sky!
https://starplot.dev
ββ¨π
Astrophysicien Γ l'Observatoire de la CΓ΄te d'Azur.
Auteur de 'Le tΓ©lescope spatial James Webb' et 'L'odyssΓ©e cosmique, une histoire intime des Γ©toiles'
Theoretical materials scientist, searching for new magnets.
Researcher @ Uppsala University, Department of Physics and Astronomy.
Trans radical feminist.
Born in β94; Street Fighter player since β96; MtG player since β13.
She/her.
Astronomy, Exoplanets, Astrobiology, Cool Worlds Lab, Columbia University. Be kind to one another.
Exo-planet enthusiast. Prof. at Leiden Observatory and SRON. Pet lover <3
News and information for the Science Explorer (SciX) user community. Explore with us at SciXplorer.org
PhD in Astrophysics at Trinity College Dublin studying atmospheres and clouds on brown dwarfs (aka overachieving planets) βοΈπͺ
Previously at: University of Sydney, Lund University
they/them
https://madeline-lam.github.io/
Planetary scientist and science communicator π postdoctoral researcher at West Virginia University πΊπΈ previously at MSSL, University College London π¬π§ she/her
Geologist/planetary scientist at Texas A&M using x-ray vision to study ancient life and surface processes. Commutes to Mars on the Perseverance Rover. He/him
Interstellar Flight Experimental Research Group @mcgill.ca : Researching the technologies that will make our civilization multi-stellar.
https://interstellarflight.space/
My goodness: It's full of planets!
European in Graz.
Often to be found at Space Research Institute at Graz!
(Yes, Graz hosts the Austrian Space Research Institute. It's awesome, check it out!)
(Ja, Graz hat die Weltraumforschung und sie ist toll)
Staff Scientist @ STScI
All posts are my own. (Seriously, who else would want to take credit for this nonsense?)
ORCID: https://orcid.org/0000-0002-2508-9211
ESA/AURA Astronomer at STScI, working on exoplanet atmospheric characterization, MIRI, and time-series observations. Posts are my own and do not necessarily reflect the views of STScI, ESA, or AURA.
Passionate about hiking, camping, and canoeing.
He/him