Keys to Composition: Observational Methods of Determining Near Earth Asteroid Properties Open Access
Marshall, Cheryl Kaye (Spring 2026)
Abstract
Near Earth Objects, or NEOs, provide rare opportunities to study the composition, structure, and dynamical histories of small bodies delivered from the main asteroid belt into near-Earth space. Providing insight into solar system history, migration and collisional processes shape the physical properties of NEOs, such as rotation period, shape, albedo, and spectral type. This thesis examines three NEOs, 2025 FA22, (3361) Orpheus, and 2004 VA, and one main‑belt asteroid, 35 Leukothea, to evaluate observational methods for assessing different properties of NEOs. Fast-moving targets, 2025 FA22 and (3361) Orpheus, prompted the adoption of TRIPPy, Trailed Image Photometry in Python in order to get a light curve to assess spin period and shape. 2004 VA and 35 Leukothea were used for assessing composition through phase‑angle photometry by evaluating the phase-slope coefficient . Each of these contributed to testing and comparing observational techniques in our continual study of the origins of NEOs.
Table of Contents
Table of Contents
Chapter 1. Introduction
I. Importance of Understanding NEOs
II. Observational Techniques
a. Taking Data for Photometry and Calibrations
b. Differential Photometry and Calculating Magnitudes
c. Comparison Stars
d. Result Goals
III. Target Selection
Chapter 2. Light Curves for Fast-Moving NEOs: Pill-Shaped Apertures
I. TRIPPy
II. Changes in Photometric Process for Fast-moving NEOs
III. (3361) Orpheus
IV. 2025 FA22
a. Light Curve Results
b. V–R Analysis
Chapter 3. Albedo and Spectral Type through Phase Angle Photometry
I. Creating Phase Curves
a. Stacking
b. Calculating H Magnitudes
c. Exposure Times and Maximizing SNR
II. 35 Leukothea (A855 HA)
III. 2004 VA
Chapter 4. Conclusions
I. Scientific Conclusions
II. Observational Conclusions
Bibliography
Appendix A
About this Honors Thesis
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