Elsevier

Acta Astronautica

Volume 185, August 2021, Pages 148-160
Acta Astronautica

Tethered aerobraking design for repeatable maneuvers

https://doi.org/10.1016/j.actaastro.2021.04.027Get rights and content

Highlights

  • Analytic solutions for tether dynamics in an elliptical orbit.

  • Efficient, robust computational algorithm for targeting tether libration angle and angular rate via tether length control.

  • Demonstrates that repeated aerobraking maneuvers are possible with practical power requirements.

Abstract

An aerobraking maneuver performed with a tethered system has the benefit of increasing the drag for a given center of mass orbit by dropping the lower subsatellite into the denser atmosphere. While this concept has received significant attention in the literature, the exact means of controlling the attitude prior to the aerobraking fly-through has not been adequately treated. In particular, a scheme for repeated passes in elliptical orbits has not been developed, which would be required, for example, in a debris elimination system. This work uses tether reeling during the exoatmospheric flight in order to control the tether libration to target a desired state prior to the aerobraking trajectory. The design of the control law requires numerical solution of nonlinear equations, but newly developed analytics provide an estimate that reduces computational time and increases the robustness of the algorithm. The results show that the nearly periodic state that is required for successive passes can be achieved for practical tether lengths and power requirements.

Introduction

Momentum exchange tethers have been deeply studied as they are an efficient tool to introduce changes in the orbit of a satellite. For instance, for a system formed by two masses connected by a long cable, cutting the tether when the satellite is vertically orientated boosts the upper end-body into a higher elliptical orbit and the lower body into a lower energy one [1]. Recently, the idea has been applied to space debris [2,3]. A piece of debris is captured, reeled out along a long tether, and then released making use of the gravity gradient to deorbit the debris. This exchange of momentum between the debris and debris elimination satellite unfortunately places the latter into a higher orbit. After relatively few debris objects are deorbited, the debris elimination satellite is boosted above the LEO belt. The methodology developed in this paper can be implemented to counteract the increase in orbital energy caused by deorbiting a piece of debris, allowing for repeated deorbit of arbitrarily many debris objects without the use of propellant.

The salient interaction between tethered satellites and dense atmospheres has been extensively studied. Lorenzini et al. [4] studied the feasibility of a tethered system in a circular orbit around Mars (e=0), which investigated a sustained penetration of a probe into the Martian atmosphere. For hyperbolic orbits (e>1), Puig-Suari et al. [[5], [6], [7]] envisioned the satellite as a means to decelerate spacecraft and achieve an aerocapture. A practical analytical tool was provided to determine the initial conditions required for the transfer maneuver. However, the intermediate case of a system orbiting in an eccentric orbit (0<e<1) has not been adequately developed. In particular, a design for sustained, repeated aerobraking maneuvers (necessary for the debris removal concept described above) has not been accomplished.

Attitude control of the tether libration has also received much attention, in particular during the deployment and retrieval phase. Controlling the libration in elliptical orbits or to a non-vertical reference (both of which are required for this concept) have been topics of considerably less study. One exception is the work by Arnold in which he computes the nonzero equilibrium tether angle for a nearly circular orbit during deployment and retrieval [8]. He observes changes in the orbital elements due to the gravity gradient forces which can be seen in the results of this work. Martinez-Sanchez considers elliptical orbits, but has a nominal control law that is referenced to a vertical orientation [9]. Several papers treat the general case of large librational excursions in an elliptical orbit, but all of these develop a stabilizing control with a periodic reference motion [[10], [11], [12], [13]]. None of the work in the literature deals with targeting a specific non-equilibrium state at a given time in an elliptical orbit as is required for the aerobraking portion of this concept.

In this paper, a system formed by an orbiter and a probe connected by a long and thin tether that rotates around its center of mass in the plane of the orbit, is proposed as a means to efficiently reduce the orbital energy of a spacecraft in an eccentric orbit around the Earth (see Fig. 1). During the closest approach to the planet, the probe deeps down into the atmosphere to slow down the satellite. The work integrates previously developed theory for the aerobraking maneuvers with a new tether control law via tether reeling for targeting the desired initial tether libration state (angle and angular rate) for the aerobraking maneuver. This control scheme maintains the reusable nature of the system, allowing for an arbitrary number of atmospheric fly-throughs to decrease energy as additional debris is removed.

Section snippets

Mission concept

The mission design for a repeatable aerobraking maneuver is accomplished by separating the problem into endoatmospheric and exoatmospheric trajectories (Fig. 1). During the exoatmospheric flight, the tether length is actuated to achieve the proper boundary conditions for the endoatmospheric flight which then achieves the desired decrease in orbital energy.

Puig-Suari and Longuski [7] develop the endoatmospheric aerobraking maneuver for a vertical orientation of the tether at periapsis to

System model

The system is treated as the ensemble of an orbiter and a probe connected by a long and thin tether. Since the two spacecraft are small compared with the dimensions of the entire system, they are treated as particles, affected by gravitational and drag forces [5]. The tether has small diameter, therefore the mass and area are neglected and it will not experience any force other than tension. The tether is assumed to be rigid, which was demonstrated to be valid for well designed aerobraking

General maneuver design for multiple passes

The loss of energy that occurs over the entire mission of multiple orbits is specified as a decrease of the semi-major axis, Δatotal. Although the impact with the atmosphere occurs during a finite time, the endoatmospheric flight can be modeled as a decrease in velocity, Δv, occurring impulsively at periapsis.

The endoatmospheric maneuver is designed based upon the Vertical Dumbbell maneuver by Puig-Suari et al. [7]. This maneuver achieves a vertical orientation at periapsis (α=0 and α˙=0rad/s

Exoatmospheric solution

Solving the piecewise-defined control law [Eq. (27)] that matches the BC's [Eq. (28a), (28b), (28c), (28d), (28e), (28f), (28g)] is not trivial. Equations (28a), (28b) are satisfied by setting the initial conditions of the exoatmospheric flight to be the ones given by the TA algorithm.

The remaining BC's are satisfied using the control law, which is composed by five parameters: c3, c4, c7, c8 and ts. Two of these parameters are solved by inspection of Eqs. (28c), (28g), yielding:c3=l2andc7=l2ec8

Case study

A case study is shown to demonstrate the theoretical feasibility of the mission for a case that is consistent with a maneuver that requires a LEO satellite to decrease its altitude by several kilometers (e.g., debris elimination). The characteristics of the system are described in Table 2 and its initial orbit has the following orbital elements:e0=0.4,a0=10901.7km

The semi-major axis corresponds to a periapsis altitude (hper) of 170 km above sea level. Assuming a constant semi-major axis loss

Analysis of the exoatmospheric analytic solutions

The efficacy of the analytic solutions is investigated by considering different schemes to achieve the Full Numerical solution. Three strategies are used to calculate the exoatmospheric control law. The first is the scheme described in the “Use of Analytic Theories” section, which uses the two analytic solutions as an input for the FN, with the perturbation theory solution obtained under a continuation scheme. The second is the use of the sinusoidal solution as the guess for the FN. The third

Design tools

Based on the same spacecraft characterized in Table 2, two studies are conducted to provide insight into the nature of different maneuvers with varying orbital conditions. The goal is to come up with useful design tools that help achieve a desired maneuver.

Conclusions

A semi-major axis reduction of several kilometers using multiple aerobraking passes has been demonstrated to be feasible for a tethered system in an elliptic orbit around the Earth. Much larger decreases in energy are possible which have been verified by numerical simulation. By extension, the concept allows for an arbitrary number of repeated passes facilitating sustained operations for missions such as debris elimination.

Analytic solutions to the control law provide a good initial guess for

Declaration of competing interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

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