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High fidelity modeling of SRP and its effect on the relative motion of Starshade and WFIRST
Author(s) -
Ariadna Farrés,
Cassandra Webster,
David Folta
Publication year - 2018
Publication title -
nasa sti repository (national aeronautics and space administration)
Language(s) - English
Resource type - Conference proceedings
DOI - 10.2514/6.2018-2227
Subject(s) - computer science , motion (physics) , computer vision
In this paper we perform a detailed analysis of how Solar Radiation Pressure (SRP) affects the relative motion of two spacecrafts, the Wide-Field Infrared Survey Telescope (WFIRST) and Starshade, orbiting in the vicinity of the Sun-Earth L2. While WFIRST orbits about its own Libration Point Orbit (LPO), Starshade will fly a specific trajectory to align with WFIRST and observe a Design Reference Mission of pre-determined target stars. In this analysis, we focus on the transfer orbit for Starshade from one observation to the other. We will describe how SRP affects the dynamics of the Starshade relative to WFIRST and how relevant this effect is in order to get an accurate estimate of the total ∆v.

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