Research Partnership Lead at SURF | PhD @ELSI_origins | 🍜 | 🇮🇹 in 🇳🇱| she/her
Europe
Joined February 2019
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We also looked into the longevity of the generated magnetic field and found that both the bulk and mantle iron content strongly influence the lifetime of a magnetic field.
We investigated core structure after accretion and its thermal evolution for rocky planets of different mass and iron content (bulk and mantle iron contents, XFe and # FeM in the figure). We found that rocky planets are likely to feature partially solid cores after accretion.
We calculated the influence of CO2 condensation on the evolution of initially cold and warm rocky planets located in the "habitable zone" of F-K stars.
The symposium was organized in such a way that all sessions took place at sensible times for different time zones, in order for everyone to not have to stay up late and/or wake up early. If you are interested in this format, the schedule is here.
Nice video from the Italian Geological Society to encourage more people to enroll in geology degrees. Geology is more than what you think! 🌍🌋🪐👩🔬🔨 #iogeologo
youtube.com/watch?v=dN11usDF…
We know you might be drowning in other deadlines, but don't forget to send your application to attend @abgradcon 2020 in at @ELSI_origins in Tokyo! Deadline March 15 23:59 JST
Visit abgradcon.org/
TAPS (Tokyo Area Planetary Science) is back at @UTokyo_News_en! Today's keynote speaker is Dave Brain from @CUBoulder
"Do habitable planets require magnetic fields?"#TAPS #TokyoAreaPlanetaryScience @ELSI_origins @prcnaoj_en @JAXA_en
