Gijs D Mulders
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gijsmulders.com
Gijs D Mulders
@gijsmulders.com
Exoplanet Astronomy
Assistant Professor
Santiago de Chile
http://gijs.cl
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Solar system-like architectures appear for a small range of initial disk masses around F and G stars, but are not a common feature around K and M stars.

Perhaps we are somewhat special among #exoplanets?

18 /🧵
October 8, 2025 at 9:10 PM
While the mid mass architecture is most efficient at depositing water directly in the habitable zone:

It's pebble snow!

#exoplanets
17/🧵
October 8, 2025 at 9:10 PM
The low-mass architectures are quite efficient at creating water-worlds close to the star.

16 /🧵
October 8, 2025 at 9:10 PM
The architectures are remarkably consistent across stellar mass, with the location and size of planets shifting with snow line and disk mass

15 /🧵
October 8, 2025 at 9:10 PM
The mid mass architectures form a bimodal distribution:

Giant planet cores at the initial snow line location,

and a second peak with smaller, water-rich #exoplanets in the habitable zone!

14/🧵
October 8, 2025 at 9:10 PM
And…

13/🧵
October 8, 2025 at 9:10 PM
Low mass disks from predominantly planetary cores closer in, possible precursors to super-earths or waterworlds.

12/🧵
October 8, 2025 at 9:10 PM
The main results is there are three growth modes:

High mass disks form exclusively giant planet cores outside the snow line

11/🧵
October 8, 2025 at 9:10 PM
And explored a large range of stellar mass and disk mass to identify trends

10/🧵
October 8, 2025 at 9:10 PM
And a snow line that moves in over time

9/🧵
October 8, 2025 at 9:10 PM
Sean added two components:

Pebble filtering from 100s of planetary cores growing simultaneously

8/🧵
October 8, 2025 at 9:10 PM
How would the diverse population of giants planets discovered around other stars, impact the mass and water content of exoplanets in the habitable zone?

4/🧵
October 8, 2025 at 9:10 PM
Jupiter has long been suspected to play as role in shaping the inner solar system and controlling water delivery to earth

3/🧵
October 8, 2025 at 9:10 PM
One of the big mysterious in planet formation is how earth got to its current state:

Not too big or too small, and with the right amount of water to support life.

2/🧵
October 8, 2025 at 9:10 PM
How do giant planets influence the type of #exoplanets that form in the habitable zone?

A thread 1/🧵
October 8, 2025 at 9:10 PM
#achievement for the day

(please don't send me any more email)
August 20, 2025 at 10:04 PM
Probably because Jupiter was relatively massive for a giant planet, and prevented super-Earths from forming
July 1, 2025 at 9:50 PM
So why does the solar system not have these inner super-Earths?
July 1, 2025 at 9:50 PM
So the correlation between super Earths and giant planets depends strongly on the giant planet mass!

#exoplanets ☄️
July 1, 2025 at 9:50 PM
While the super-Earth is two times LESS likely to have a super-Jupiter than than a random star
July 1, 2025 at 9:50 PM
Then we split the sample in half by giant planet mass

Now the super-Earth is FOUR times more likely to have a Saturn-mass planet than a random star
July 1, 2025 at 9:50 PM
Etienne also looked at conditional occurrence rates

A super-Earth is TWICE a likely to have a giant planet than a random star
July 1, 2025 at 9:50 PM
To make sure this wasn’t some sensitivity bias, we calculated giant planet occurrence rates for stars with and without super-Earths.

But the mass difference of a factor 6 remains
July 1, 2025 at 9:50 PM
Where we noticed that cold Jupiters are a lot smaller when they have a super-Earth companion, by about a factor 6 on average
July 1, 2025 at 9:50 PM
He analyzed the radial velocity sample from the California Legacy Survey
July 1, 2025 at 9:50 PM