International Journal of Astronomy and Astrophysics
Vol.07 No.03(2017), Article ID:77775,8 pages
10.4236/ijaa.2017.73010
The Solution of Optimal Two-Impulse Transfer between Elliptical Orbits with Plane Change
M. H. A. Youssef
Astronomy Department, Faculty of Science, Cairo University, Cairo, Egypt

Copyright © 2017 by author and Scientific Research Publishing Inc.
This work is licensed under the Creative Commons Attribution International License (CC BY 4.0).
http://creativecommons.org/licenses/by/4.0/



Received: April 10, 2017; Accepted: July 17, 2017; Published: July 20, 2017
ABSTRACT
The optimizing total velocity increment
needed for orbital maneuver between two elliptic orbits with plane change is investigated. Two-impulse orbital transfer is used based on a changing of transfer velocities concept due to the changing in the energy. The transferring has been made between two elliptic orbits having a common centre of attraction with changing in their planes in standard Hohmann transfer with the terminal orbit which is elliptic orbit and not circular. We develop a treatment based on the elements of elliptic orbits
,
and
of the initial orbit, final orbit and transferred orbit respectively. The first impulse
at the perigee induces a rotation of the orbital plane by
which will be minimized. The second impulse
at apogee is induced an angle
to product the final elliptic orbit. The total plane change required
. We calculate the total impulse
and minimize by optimizing angle of plane’s variation
. We obtain a polynomial equation of six degrees on the two transfer angles between neither two elliptic orbits
and
. The solution obtained numerically, using programming code of MATHEMATICA V10, with no condition on the eccentricity or the semi-major axis of the initial, transformed, and the final orbits. We find that there are constrains on the transfer angles
and
. For
it must be between 40˚ and 160˚, and there is no solution if
is less than 40˚ and bigger than 160˚ and
takes the values less than 40˚. The minimum total velocity increments obtained at the value of
less than 25o and 
Keywords:
Orbital Mechanics, Astrodynamics, Optimization, Elliptic Hohmann Transfer
1. Introduction
The problem of the optimal impulsive transfer between two orbits is almost seventy years old, but the question, how many impulses are still open despite of the theories and a lot of numerical works developed in this field. In 1925, Hohmann produced a numerical study showing that the optimum two-impulse transfer path between coplanar circular orbits is a semi-ellipse, tangential at its apsides to both circular orbits, with an impulse occurring at each apse. Hohmann transfer is generalized to the elliptic case (transfer between two coaxial elliptic orbits). A large number of works have been made to optimize non-coplanar transfer between circular or elliptic orbits having collinear major axes [1] [2] [3] [4] . An analytical solution for optimal two-impulse 180˚ transfer between non-coplanar elliptic orbits and the optimal orientation of the transfer plane is presented with numerical solutions under some terminal conditions in [5] . A polynomial equation of six degrees on the generalized Hohmann transfer with plane change using energy concepts is obtained without analytical solution [6] . A fundamental result is presented in Lawden’s work where a primer vector satisfying necessary condition for optimality of the total delta velocity was introduced in coplanar transfer [7] . The necessary condition for optimality is reduced to a polynomial equation of the eighth degrees on the semi-latus rectum and with the fixed transfer angle, for which no solution has been found in two-impulse transfer between two elliptic coplanar orbits [8] . In this work, we give the optimum total velocity increment 











2. Formulation and Optimization
Any analysis of orbital maneuvers, i.e., the transfer of a satellite from one orbit to another by means of a change in velocity, begins with the energy as

where 



where it is evident that
Note that (energy/satellite mass (is dependent only on a, an increases, energy increases. Orbital maneuvers are based on the principle that an orbit is uniquely determined by the position and velocity vector at any point [9] . Conversely, changing the velocity vector at any point instantly transforms the trajectory to a new one corresponding to the new velocity vector. So if we want to move a spacecraft to a higher orbit, we have to increase the semi-major axis (adding energy to the orbit) by increasing velocity. On the other hand, to move the spacecraft to a lower orbit, we decrease the semi-major axis (and the energy) by decreasing the velocity. Any conic orbit can be transformed into another conic orbit by changing the spacecraft velocity vector. Coplanar maneuver only involves the change of the orbit without changing the orbit plane, we have four kind of coplanar maneuvers (i) Tangential orbit Maneuver, (ii) Non-tangential orbit Maneuver, (iii) Hohmann transfer, (iv) Bi-elliptic orbit transfer. The Hohmann’s transfer is the minimum two-impulse transfer between coplanar circular or elliptic, it can be used to transfer a satellite between two nonintersecting orbits, coaxial, aligned. The fundamental of the Hohmann’s transfer is a simple maneuver. This maneuver employs an intermediate elliptic orbit which is tangent to both initial and final orbits at their apsides. A 

























The total velocity increment will obtain from the following relations, as seen in Figure 2.

Figure 1. Geometry of the orbital transfer with plane change.
Figure 2. Geometry of the velocities changing.

where














Thus, the total increment of the velocity is

For simplicity let




Then (9) will be in the form


By partial differentiation of (11) with respect to 

From which we can deduce that

where




After some reduction, we find that
Let
Then

After squaring and some reduction, we may write

Set
Then Equation (16) will be an algebraic equation of degree six in 


3. Solution and Discussion
There is no analytical solution for the Equation (17), but we solved it numerically, using code of MATHEMATICA V10, with no condition on the eccentricity or the semi-major axis of the initial, transformed, and the final orbits. The optimization problem was solved for two angles of rotation of the apsidal lines, using the computed values of the velocities at perigee and apogee, and the transfer angle






4. Conclusion
We give a complete analytical analysis and numerical solution of optimal two-
Table 1. The values of 

Figure 3. The constrain of 

impulse transfer with plane change. Our treatment is based on a changing of transfer velocities concept due to the changing in the energy. We obtained the total velocity increment 













Cite this paper
Youssef, M.H.A. (2017) The Solution of Optimal Two-Impulse Transfer between Elliptical Orbits with Plane Change. International Journal of Astronomy and Astrophysics, 7, 125-132. https://doi.org/10.4236/ijaa.2017.73010
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