Abstract
This paper examines the use of an elliptically-orbiting tethered-dumbbell (Space Shuttle-satellite) system for satellite transfer to geosynchronous altitude. The two-dimensional rigid body equations of motion are derived using a Lagrangian method. Integration of these equations yields the system states, from tether deployment through payload release. These states are used to predict the ΔV savings (compared to a Hohmann transfer) when the payload is given a “forward swing zero libration” release, that is, the payload is released on a forward swing when the libration angle is instantaneously zero. By varying the pre-deployment true anomaly, the “forward swing zero libration” is caused to occur nearly simultaneously with periapse passage, resulting in maximum Δ V savings. The system deployment velocity and tether length were also varied to observe their effect on Δ V savings.
| Original language | English (US) |
|---|---|
| State | Published - 1986 |
| Event | Astrodynamics Conference, 1986 - Williamsburg, United States Duration: Aug 18 1986 → Aug 20 1986 |
Other
| Other | Astrodynamics Conference, 1986 |
|---|---|
| Country/Territory | United States |
| City | Williamsburg |
| Period | 8/18/86 → 8/20/86 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
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