Precise attitude estimation of solar sail spacecraft utilizing coupling between attitude and orbital dynamics

Kenji Kitamura*, Yuichi Tsuda, Sho Taniguchi, Jun'ichiro Kawaguchi

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Orbit determination is the process to estimate the position and velocity from a given set of observations of spacecraft. The common measurements used in orbit determination are range and range rate. For precise orbit determination, the acceleration of spacecraft by solar radiation pressure (SRP) must be taken into account. In order to incorporate the SRP acceleration, the attitude history and the SRP model - surface shape and optical surface feature of spacecraft - need to be known beforehand. Especially, in case of solar sail spacecraft, since their SRP effect is strong, coupling between attitude and orbital dynamics is more remarkable than ordinary ballistic missions. Therefore, by positively utilizing this coupling, it is possible to refine the attitude information based on the residual errors of orbit determination. In this study, we assume that the systematic errors in the orbit determination of the spacecraft are caused solely by the errors in attitude information, and propose an attitude error correction method which utilizes the coupling between attitude and orbital dynamics. In order to examine the validity of the method, the analysis of actual data is conducted. As actual data, flight data of IKAROS - Japanese interplanetary solar sail demonstration spacecraft - are used. The observations used in the orbit determination of IKAORS are range and range rate. In this paper, an estimator is designed whose input is the residuals of the orbit determination result - the difference between actual measurements and modelled observations of range and rage rate - and whose output is the amount of error correction in the attitude history. It is confirmed that orbit and attitude errors are both decreased through this method. This paper explains the theoretical background of this method and shows the result of analysis using the actual data.

Original languageEnglish
Title of host publication62nd International Astronautical Congress 2011, IAC 2011
Pages5021-5028
Number of pages8
Publication statusPublished - 2011
Externally publishedYes
Event62nd International Astronautical Congress 2011, IAC 2011 - Cape Town, South Africa
Duration: 3 Oct 20117 Oct 2011

Publication series

Name62nd International Astronautical Congress 2011, IAC 2011
Volume6

Conference

Conference62nd International Astronautical Congress 2011, IAC 2011
Country/TerritorySouth Africa
CityCape Town
Period3/10/117/10/11

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