James Webb Space Telescope Fuel Slosh EstimationThe mitigation of fuel slosh in microgravity environments is a pressing matter for the control of both manned and unmanned spacecraft. This paper investigates the attitude perturbations caused by fuel slosh aboard the James Webb Space Telescope (JWST). We develop a dynamical model to parse these perturbations from slew telemetry data. This model uses special Euclidean group SE(3) as well as a novel, N-body variational integrator. The enhanced ability to validate fuel slosh models offers the reduction of settling time after slew operations and, accordingly, the maximization of available science time.
Document ID
20240011800
Acquisition Source
Kennedy Space Center
Document Type
Extended Abstract
Authors
Thi-han W Nge (Florida Atlantic University Boca Raton, United States)
Matthew M Wittal (Kennedy Space Center Merritt Island, Florida, United States)
Carl Hansen (Space Telescope Science Institute Baltimore, United States)
Peter Gauthier (Space Telescope Science Institute Baltimore, United States)
Date Acquired
September 16, 2024
Subject Category
AstrodynamicsAeronautics (General)Fluid Mechanics and ThermodynamicsPropellants and Fuels
Meeting Information
Meeting: 2025 AAS/AIAA Space Flight Mechanics Meeting
Location: Kaua'i, HI
Country: US
Start Date: January 19, 2025
End Date: January 23, 2025
Sponsors: American Institute of Aeronautics and Astronautics, American Astronautical Society