Astrochemistry Laboratory

Mauricio Ayllon Unzueta

(Postdoctoral Research Associate)

Mauricio Ayllon Unzueta's Contact Card & Information.
Email: mauricio.ayllonunzueta@nasa.gov
Org Code: 691
Address:
NASA/GSFC
Mail Code 691
Greenbelt, MD 20771
Employer: CATHOLIC UNIV OF AMERICA

Brief Bio


I am a nuclear engineer. My areas of expertise are gamma and neutron spectroscopy, Monte Carlo simulations, radiation detection, data acquisition systems, and data analysis. I am part of the science/engineering team of the Dragonfly Gamma ray and Neutron Spectrometer (DraGNS), which will explore the surface of Titan.

Research Interests


Bulk elemental composition measurements with neutrons and gamma rays

Solar System: Astrochemistry

Neutrons and gamma rays offer the possibility to measure elemental concentrations of the near-surface of planetary objects in a non-destructive way.


Inelastic scattering cross section measurements

Solar System: Astrochemistry

Reliable nuclear data is needed to predict the performance of planetary nuclear spectrometers. Inelastic scattering cross sections are particularly problematic in public databases because of discrepancies between measurements and/or lack of data for certain isotopes.


Graphical User Interfaces for data analysis

Solar System: Astrochemistry

Dedicated GUIs for quick analysis of data is important. I am interested in programing GUIs in Python.

Current Projects


Neutron techniques to measure the bulk elemental composition of meteorites

Astrochemistry

Accurate non-destructive techniques to measure the bulk elemental composition of meteorites are needed to aid in the interpretation of data from past and future gamma ray and neutron spectrometers. Current techniques, albeit very accurate and precise, measure the composition of only a small and possibly non-representative sample. A novel instrument known as Associated Particle Imaging (API) has the potential to precisely measure the composition of medium to large meteorite samples.


Compact Neutron Monitor (CNM) lead of DraGNS

Planetary surfaces

The CNM is a key sensor of DraGNS that will allow for accurate bulk elemental composition measurements on the surface of Titan. The CNM is a diamond detector used to measure high energy neutrons, and hence calibrate the neutron source onboard Dragonfly.


Inelastic scattering cross section measurements with API

Novel Data Analysis Development

In collaboration with Lawrence Berkeley National Laboratory, we are developing a novel technique to measure needed nuclear data for gamma ray and neutron spectrometers in a more precise and cost-effective way.