Dr. Matthew Richardson
Postdoctoral Research Scientist
Currently resides in Tennessee
Targets of Interest: Main-Belt Asteroids, Mercury, Moon, NEOs, Asteroids
Disciplines/Techniques: Astroparticle Physics, Image Classification, Crater Counting, Machine Learning
Formally trained as a high-energy astrophysicist, my research focused on the source distribution, propagation, and detection of the highest energy charged particles originating from space, commonly referred to as the ultra high energy cosmic rays. My persuit to elucidate the relationship between these highly researched topics in high energy astrophysics has relied on the use of Monte Carlo simulations and analysis of data acquired at the Pierre Auger Observatory. Currently, I use spectral observations in the mid-IR region of asteroids along with thermal modeling and machine learning techniques towards the construction of an asteroid taxonomy.
Active Projects
Continued Studies of the Impact of Solar Wind Ions on the Surface and Exosphere of Mercury
NASA Solar System Workings Program
Institutional PI
Project Team
Understanding Asteroids by the Distribution of their Hydrated Minerals
NASA Solar System Observations Program
Institutional PI
Project Team
External Partners
- The Johns Hopkins University Applied Physics Laboratory
Unraveling the Extent of Basaltic Volcanism in the South Pole-Aitken Basin
NASA Lunar Data Analysis Program
Principal Investigator
