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The summer after my freshman year I was awarded a SURF grant to research at CalTech under Marvin L. Goldberger Professor of Planetary Science David J. Stevenson. Our aim was to learn more about Jupiter's interior by refining the range of possible sizes and masses that the planet's core could take on. The motivation for this project was the arrival of NASA's Mission Juno spacecraft at Jupiter that summer, whose Gravity Science Experiment has detected slight disturbances in the spacecraft's orbit about Jupiter in order to accurately measure the planet's moment of inertia. Starting with a simple equation of hydrostatic equilibrium in Jupiter's envelope, the planet's equation of state was perturbed to model changes in the envelope's heavy element makeup, and the resulting effects on the core's theoretical radius and mass were studied.
I wrote a paper summarizing my research called "Uncertainties in the Determination of Jupiter's Core" and presented my findings to a board of CalTech faculty at the end of the fellowship. I was also invited to JPL on July 4th to witness the Jupiter Orbital Insertion (JOI) surrounded by the engineers and scientists that made the mission possible. My paper and presentation are included below.
My first research experience was during the summer of 2014 when I worked on The Haloes and Environments of Nearby Galaxies (HERON) Survey. Led by UCLA research astronomer R. Michael Rich, the survey was the most extensive ever to investigate the outskirts of galaxies near the Milky Way. We learn much about the early history of galaxies from their haloes, where many ancient stars reside, and hope to gain insight into the dark matter intertwined with these galaxies.
Our images were taken with relatively small charge coupled device (CCD) telescopes that allowed for short exposure times, making the survey vastly more economically efficient than similar ventures. My job was to employ PyRAF software to perform image reductions, combining flats, darks, and biases to refine the images and reveal galactic substructures. The image above is a reduction I performed on the intermediate spiral galaxy NGC 4258 (Messier object 106).
The team published its findings in an article in the Monthly Notices of the Royal Astronomical Society. Check it out below!