New Measurements and Proposed Orbital Parameters for WDS 03575-0110 using Desmos Fitting

Abstract

This paper analyzes the newly observed measurements of the star system WDS 03575-0110, and proposes a set of new orbital parameters for the system. Ten images of WDS 03575-0110 were observed through the Las Cumbres Observatory telescope network, and data were extracted and averaged to measure the separation and position angle of this system as of November 12th, 2024. This resulted in the current separation of 10.902 arcseconds, and the current separation angle of 12.937°. Using parallax data from the GAIA Data Release 3 Mission, the system was deemed to be close enough to be gravitationally bound. Utilizing the newest data point, as well as historical data provided by the U.S. Naval Observatory, new orbital parameters were also found using a Desmos fitting method with an R² of 0.977.