Gijs D Mulders

@gijsmulders.com

Exoplanet Astronomy Assistant Professor Santiago de Chile http://gijs.cl \m/

ever wonder: 🛸 are aliens real? ☀️ is our solar system unique? 🌍 how can we tell if there’s life on another planet? 📈 should we destroy capitalism? 🧑‍🔬 how could i become an astrobiologist? CLOUDY WITH A CHANCE OF STARSHIPS has the answer! www.barnesandnoble.com/w/cloudy-wit...

Cloudy with a Chance of Starships: How the Drake Equation Reveals the Odds of Life in the Cosmos

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🔭 Applications are now open for the Doctoral and Master Program in Astrophysics at the Institute of Astrophysics UC. 🌌 Research excellence across galaxy evolution, exoplanets, cosmology, stellar populations & more 💰 Full scholarships & stipends for all admitted students 📅 Deadline: July 31, 2026

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🔭 A cautionary tale for undergrads (and above!) using AI for #astro plots: our BSc student wanted to make a "quick" HR diagram showcasing M-dwarfs & thought some chatbot could make one and... well... ...extra credits are now offered to students who can correctly find all errors on cursedHR.png 🫠 🧪

A pathetic attempt by AI sloppery to make a HR diagram, generated by one of our BSc student, and shared here with their permission. Honestly, I can't even begin to explain all the deviations. Imagine a normal HR diagram but one that appears to you in a fever dream. It gets so much worse the longer you look at it. WHY IS THIS ALLOWED TO EXIST AAAAA

New research note accepted to RNAAS! Yes, this is a serious science post today. 🧪 We've created a catalog of Gaia DR3 IDs that correspond to TESS Input Catalog IDs! No more cross-matching on your own or hoping the Gaia DR2/DR3 IDs are the same! arxiv.org/abs/2603.28850 🔭 #exoplanets

Gaia DR3 IDs for TESS Input Catalog Targets

The TESS Input Catalog (TIC) was built on Gaia Data Release 2 (DR2). To date, there has not been an update to the TIC to incorporate Gaia Data Release 3 (DR3) IDs. In this Research Note, we outline ho...

arxiv.org

It's happening!!! Pandora is going to space in just over 16 hours (if all goes well). Pandora is going to help us study exoplanet atmospheres, even when their host stars are misbehaving. I am headed up to Vandenberg to watch the launch shortly, and will make a thread about the mission/launch here!

Pandora spacecraft in front of an exoplanet

I'm very happy I woke up at 4am this morning to catch 3I/ATLAS right before its closest approach to Earth (today!) This interstellar visitor is traveling over 60 km/s ☄️ At 269 million km (1.8 AU), I took a series of 2.5 min exposures with my Seestar 🔭

The application for the ESO Summer Research Programme 2026 has just opened! It‘s a six week programme in Garching close to Munich where pre-Ph.D students can work on a hands-on project. Working at @eso.org is a fabulous experience, so please help me spread the word ✨ 🔗 eso.org/sci/meetings...

ESO - SummerResearch2026

ESO is the European Organisation for Astronomical Research in the Southern Hemisphere. It operates the La Silla Paranal Observatory in Chile and has its headquarters in Garching, near Munich, Germany.

eso.org

Equating giant planet occurrence rate of ~20% to the disk fraction, that means a timescale of ~10 Myr for giant planet formation!

Emily Hunt@emily.space · 8mo ago

New paper led by Fabian Polnitzcky & with @sratzenboeck.bsky.social + @joaoalves.bsky.social: based on the ages of stars with infrared excess in Sco-Cen, it seems planet-forming disks last around twice as long as previous estimates suggest - giving twice as long for planets to form. 🔭☄️ #exoplanets

Their input source selection in the Sco-Cen region, showing stars with (blue) and without (orange) disks.

Question for the #exoplanets crowd: Does any one know where to find an updated version of this plot? I'm looking for the "standard" exoplanet mass vs. semi-major axis plot, but with an overlay of which planets have a spectroscopic measurement of their atmosphere wasp-planets.net/2020/09/29/w...

Which exoplanets do we have atmospheric spectra for?

Here’s an interesting plot created by Zafar Rustamkulov (@exoZafar), a PhD student at Johns Hopkins University. He has added up all the exoplanets for which we have either transmission spectr…

wasp-planets.net

w/ Oli Shorttle, @johannateske.bsky.social & Eliza Kempton we reviewed our current understanding and prospects for peaking on the inside of small #exoplanets in "Constraining exoplanet interiors using observations of their atmospheres": www.science.org/stoken/autho... & arxiv.org/abs/2510.08844 🔭🧪⚒️☄️

Illustration of predicted interior structures of sub-Neptune exoplanets. Observed density and atmospheric constraints are interpreted in three scenarios, each with a gaseous envelope. Water worlds have a small metal core, rocky mantle, high-pressure ice layer, and possible liquid water ocean. Gas dwarfs have a larger metal core and a magma ocean. Global supercritical regimes have no clear boundaries between layers. Image credit: Mark A. Garlick.
Keith Smith@drkeithsmith.bsky.social · 10mo ago

How can we tell what's inside an #exoplanet? @timlichtenberg.bsky.social et al review how a planet's atmosphere interacts with its interior. Atmospheric observations can distinguish between lava worlds, water worlds, temperate surfaces or supercritical interiors. ☄️ www.science.org/doi/10.1126/...

Our paper on the JWST/MIRI observations of the epsilon Eridani system, led by Dr. Schuyler Wolff, were published today! This is the last of the Archetypical Disks in our MIRI Survey, after Fomalhaut and Vega. Just like for those disks, our MIRI images reveal an extended inner asteroid disk!

Four color image of the eps Eri debris disk.