SPACEU SYMPOSIUM:
MAXWELL GALLOWAY
ABSTRACT:
We modeled polarized light curves for VHS 1256 b, HIP 99770 b, and AF Leporis b in the NIR over a range of potential cloud formations/sizes/sedimentation parameter values. We discuss the effect of various parameters (e.g. T, g, i) on the potentially observable trends. Our models are part of a larger grid that will be open-access to the community.
INSTITUTE:
UCF | Planetary Sciences
EXPLORE WHAT FLORIDA SPACE INSTITUTE HAS TO OFFER
OPERATIONS
Get involved in our operations and help us continue the good we do for mankind.
RESEARCH
Explore the institute’s world-leading research and our contributions to the continued understanding of space.
EDUCATION
The central hub for students and the local community, working together with the University of Central Florida.