Monitoring the Orbital Period of Algol and Improving the West Point Obervatory.

This project aims to verify the eclipsing period of the binary star system Algol and calculate the mass and radius of its component stars using data gathered from our observations, along with some external sources. In addition to that, we plan to conduct a literature review of historical observations of Algol and upgrade the equipment within the West Point Observatory to allow unmanned overnight imaging. To observe the Algol’s orbital period, we will use the observatory to capture images during predicted eclipses. By comparing the brightness of Algol to neighboring stars, we will produce a light curve to analyze the variation in brightness during the eclipse. The observatory requires additional instrumentation to enable autonomous closure in adverse weather conditions, which will be installed before imaging the 10-hour eclipse. As part of our research, we will also identify and learn to use software for analyzing variable star data, enabling accurate interpretation of the observed light curves. Additionally, we will search for and document any small bodies that may transit or occult Algol, utilizing NASA’s Small-Body Identification Tool.