scholarly journals A motivating exploration on lunar craters and low-energy dynamics in the Earth–Moon system

2010 ◽  
Vol 107 (1-2) ◽  
pp. 187-207 ◽  
Author(s):  
Elisa Maria Alessi ◽  
Gerard Gómez ◽  
Josep J. Masdemont
2015 ◽  
Vol 25 (05) ◽  
pp. 1550077 ◽  
Author(s):  
F. J. T. Salazar ◽  
E. E. N. Macau ◽  
O. C. Winter

In the frame of the equilateral equilibrium points exploration, numerous future space missions will require maximization of payload mass, simultaneously achieving reasonable transfer times. To fulfill this request, low-energy non-Keplerian orbits could be used to reach L4 and L5 in the Earth–Moon system instead of high energetic transfers. Previous studies have shown that chaos in physical systems like the restricted three-body Earth–Moon-particle problem can be used to direct a chaotic trajectory to a target that has been previously considered. In this work, we propose to transfer a spacecraft from a circular Earth Orbit in the chaotic region to the equilateral equilibrium points L4 and L5 in the Earth–Moon system, exploiting the chaotic region that connects the Earth with the Moon and changing the trajectory of the spacecraft (relative to the Earth) by using a gravity assist maneuver with the Moon. Choosing a sequence of small perturbations, the time of flight is reduced and the spacecraft is guided to a proper trajectory so that it uses the Moon's gravitational force to finally arrive at a desired target. In this study, the desired target will be an orbit about the Lagrangian equilibrium points L4 or L5. This strategy is not only more efficient with respect to thrust requirement, but also its time transfer is comparable to other known transfer techniques based on time optimization.


2011 ◽  
pp. 107-114
Author(s):  
Elisa Maria Alessi ◽  
Gerard Gómez ◽  
Josep J. Masdemont

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


Author(s):  
Yue Wang ◽  
Ruikang Zhang ◽  
Chen Zhang ◽  
Hao Zhang
Keyword(s):  

2001 ◽  
Vol 45 (11) ◽  
pp. 922-928 ◽  
Author(s):  
G. S. Kurbasova ◽  
L. V. Rykhlova

2007 ◽  
Vol 310 (2) ◽  
pp. e454-e456
Author(s):  
V.N. Glazkov ◽  
A.I. Smirnov ◽  
A. Kolezhuk ◽  
H. Tanaka ◽  
A. Oosawa

1967 ◽  
Vol 13 (5) ◽  
pp. 545-546 ◽  
Author(s):  
T. F. Gaskell
Keyword(s):  

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