Averaged solar radiation pressure modeling for high area-to-mass ratio objects in geosynchronous orbits
| Autor: | Roshan Thomas Eapen, Carolin Frueh |
|---|---|
| Rok vydání: | 2018 |
| Předmět: |
020301 aerospace & aeronautics
Atmospheric Science Computer science business.industry Geosynchronous orbit Aerospace Engineering Astronomy and Astrophysics Field of view 02 engineering and technology Mass ratio Abstract space 01 natural sciences Geophysics 0203 mechanical engineering Radiation pressure Space and Planetary Science Position (vector) 0103 physical sciences General Earth and Planetary Sciences Satellite Aerospace engineering business 010303 astronomy & astrophysics Space debris |
| Zdroj: | Advances in Space Research. 62:127-141 |
| ISSN: | 0273-1177 |
| Popis: | Space Situational Awareness, among other efforts, is aimed at providing a comprehensive and accurate knowledge of all Earth-orbiting objects. This is done by maintaining a catalog of space objects’ states (position and velocity). In the absence of observations, the orbits of these objects need to be numerically simulated. In this work, we study the high area-to-mass ratio class of objects which are sensitive to very small changes in perturbations, particularly the attitude dependent solar radiation pressure. This attitude dependency renders the orbit-attitude motion to be coupled. Traditionally, a cannonball model would be used to model these perturbations. While this is acceptable for an attitude stabilized active satellite, for non-functional space debris, the cannonball model does not seem to approximate the true dynamics accurately. Hence, a more precise, albeit computationally expensive propagation model needs to be developed, which warrants a better modeling of the perturbations in the near-Earth space. This work introduces a new model that averages the solar radiation pressure force experienced by multi-layer insulation foil in geosynchronous orbits. While speeding up the computational time by 66%, this model produces errors that are small enough to stay within the field of view of surveying telescopes over the propagation period of four days. The approach is compared with other existing models. |
| Databáze: | OpenAIRE |
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