# The Journal of the Astronautical Sciences

The Journal of the Astronautical Sciences > 2017 > 64 > 1 > 97-97

The Journal of the Astronautical Sciences > 2017 > 64 > 1 > 1-17

The Journal of the Astronautical Sciences > 2017 > 64 > 1 > 50-71

*f*(

*x*) =

*x*

^{8}+

*a*

*x*

^{6}+

*b*

*x*

^{3}+

*c*=0 where

*a*,

*c*<0. A possibility of multiple non-spurious roots of this 8th order polynomial equation with

*b*>0 has been extensively treated in the celestial mechanics...

The Journal of the Astronautical Sciences > 2017 > 64 > 1 > 72-96

The Journal of the Astronautical Sciences > 2017 > 64 > 1 > 18-49

*L*

_{4}in the R3BP when the smaller primary is a heterogeneous spheroid with three layers having different densities. We observe that in the nonlinear sense, the triangular libration is stable in the range of linear stability 0<

*μ*<

*μ*

_{c}, a critical value of mass parameter

*μ*, except for three mass ratios μ 1 ′...

The Journal of the Astronautical Sciences > 2017 > 64 > 2 > 118-155

*n*-dimensions in a novel way, through the use of array algebra and Kronecker...

The Journal of the Astronautical Sciences > 2017 > 64 > 2 > 207-230

The Journal of the Astronautical Sciences > 2017 > 64 > 2 > 188-206

The Journal of the Astronautical Sciences > 2017 > 64 > 2 > 99-117

The Journal of the Astronautical Sciences > 2017 > 64 > 2 > 156-187

The Journal of the Astronautical Sciences > 2017 > 64 > 3 > 251-266

The Journal of the Astronautical Sciences > 2017 > 64 > 3 > 267-284

The Journal of the Astronautical Sciences > 2017 > 64 > 3 > 285-309

The Journal of the Astronautical Sciences > 2017 > 64 > 3 > 310-332

The Journal of the Astronautical Sciences > 2017 > 64 > 3 > 231-250

*m*

_{3}is not influencing the motion of the dominating primaries

*m*

_{1}and

*m*

_{2}. We have studied the motion of

*m*

_{4}, moving under the influence of the three primaries

*m*

_{i},

*i*= 1, 2, 3, but the motion of the...

The Journal of the Astronautical Sciences > 2017 > 64 > 4 > 361-378

*method of particular solutions*and

*modified Chebyshev-Picard iteration*. The

*method of particular solutions*differs from the well-known Newton-shooting method in that integration of the state transition matrix (36 additional differential equations) is not required, and instead it makes use of a reference...

The Journal of the Astronautical Sciences > 2017 > 64 > 4 > 333-360

The Journal of the Astronautical Sciences > 2017 > 64 > 4 > 399-413

The Journal of the Astronautical Sciences > 2017 > 64 > 4 > 379-398

*i*.

*e*direct radiations as well as albedo. In this paper this is investigated how albedo perturbed the libration points and...

The Journal of the Astronautical Sciences > 2017 > 64 > 4 > 414-445

*oriented unique repeatable clustered viewpoint feature histogram*(OUR-CVFH), which is most often utilized in personal and industrial robotics to simultaneously recognize and navigate...