Abstract
The Sun-Earth libration points, L1 and L2, are located 1.5 million kilometers from the Earth towards and away from the Sun. Halo orbits about these points have significant advantages for space observatories in terms of viewing geometry, thermal and radiation environment, and delta-V expediture.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Similar content being viewed by others
References
Eismont, N., Sinitsyn, V., Farquhar, R. W., and Dunham, D. W.: 1990, Internat. Astronautical Fed. Paper, 90-302
Farquhar, R.: 1969, J. of Astronautics and Aeronautics 7, 52
Farquhar, R. W.: 1990, Internat. Astronautical Fed. Paper, 90-308
Farquhar, R., Muhonen, D., Newman, C, and Heuberger, H.: 1980, J. of Guidance and Control 3, 549
Farquhar, R., Muhonen, D., and Richardson, D.: 1977, J. of Spacecraft and Rockets 14, 170
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1990 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Farquhar, R.W., Dunham, D.W. (1990). Use of Libration-Point Orbits for Space Observatories. In: Kondo, Y. (eds) Observatories in Earth Orbit and Beyond. Astrophysics and Space Science Library, vol 166. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3454-5_52
Download citation
DOI: https://doi.org/10.1007/978-94-011-3454-5_52
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-5528-4
Online ISBN: 978-94-011-3454-5
eBook Packages: Springer Book Archive