Atmospheres of Hot Rocky Planets with Ultra-Short Orbital Period
Investigating atmospheric circulation of hot rocky exoplanets using non-grey GCM simulations with custom correlated-k coefficients.
Hi there! I am a 4th year Ph.D student at Peking University under the supervision of Prof. Daniel Koll. I was an undergraduate student of physics and astronomy at Wuhan University (BSc 2022).
I have been longing for the universe and space since I was a child. This passion led me to choose physics as my major in college, where I was fortunate to join the Qibin (启斌) Astronomy Program and gained some hands-on experience in modeling strong gravitational lensing. Later by chance, I got to know and fell in love with the field of exoplanets, the worlds beyond the Solar System.
Now I work on the atmospheres of exoplanets, mainly the small terrestrial ones. As of September 2025, more than 6,000 exoplanets had been confirmed, yet characterizing their atmospheres remains a challenge in modern astronomy. Nevertheless, atmospheric studies, including the chemistry and dynamics, are of central importance. Atmospheres provide crucial insights into how exoplanets form and evolve over time, which in turn help better understand Solar System planets. Atmospheres of exoplanets are diverse and make some of them potentially habitable for life.
PhD in Atmospheric Sciences
2022-09-01
Peking University
BSc in Physics
2018-09-01
2022-06-30
Wuhan University
My Ph.D project focuses on atmosphere modeling of rocky exoplanets with ultra-short orbital periods, utilizing 3D GCMs (Global Climate Model / General Circulation Model).
Investigating atmospheric circulation of hot rocky exoplanets using non-grey GCM simulations with custom correlated-k coefficients.
We use the ExoCAM GCM to investigate the inner edge of the habitable zone around white dwarfs, finding a novel "bat rotation" regime.