Rachel B. Fernandes

I am a Ph.D. candidate at the Lunar and Planetary Laboratory & the Department of Planetary Sciences at The University of Arizona where I work with Dr. Ilaria Pascucci and Dr. Gijs Mulders on the detection, characterization and demographics of exoplanetary systems using data from both ground- and space-based telescopes.

My research background in planet formation spans from my undergraduate work at the University of Cincinnati from where I hold a dual Bachelor of Science degree in Astrophysics and Physics, with a minor in Mathematics. Under the mentorship of Dr. Mike Sitko, I used a Monte Carlo Radiative Transfer (MCRT) code to model the near-IR variability and the outer structures (gaps, rings, spirals arms, etc.) of the dust component of protoplanetary disks around Herbig Ae/Be stars.

I also work with NASA NExSS Earths in Other Solar Systems (EOS) team, a 5 year-long astrobiology research program aimed at understanding how and where habitable, Earth-like planets with biocritical ingredients (volatiles and organics) form.

© 2019 by Rachel Fernandes, created with Wix.com

Background image Credit: Solar Systems nearest Star systems (creationsmart.com)

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