12 Motion about the libration points

AbstractWe propose to establish an Orbital Stellar Stereoscopic Observatory (OStSO) consisting of two identically equipped spacecrafts (SCs) in the vicinity of two Lagrangian libration points,

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Numerical orbits near the triangular lunar libration points

Icarus ◽

10.1016/0019-1035(75)90030-5 ◽

1975 ◽

Vol 25 (2) ◽

pp. 356-359 ◽

Cited By ~ 2

Author(s):

J.I. Katz

Keyword(s):

Libration Points

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1.3.5 On the Visibility of the Libration Clouds

International Astronomical Union Colloquium ◽

10.1017/s0252921100051599 ◽

1976 ◽

Vol 31 ◽

pp. 124-129

Author(s):

S. Röser

Keyword(s):

Light Intensity ◽

Satellite Observations ◽

Libration Points ◽

Angular Diameter ◽

Schmidt Telescope ◽

Zodiacal Light ◽

Average Brightness ◽

Upper Limit ◽

The Earth

In recent years satellite observations of the region of the Earth-Moon libration points L4 and L5 became available, which showed different results. Roach (1975) has measured perturbations of the Zodiacal Light intensity near the libration points L4 and L5 with a photometer on board the OSO-6 satellite. He interpreted the results as counterglow of a cloud of particles, having an angular diameter of 6 degrees and an average brightness of 20 S10v, whereas observations by Burnett et al. (1974) set an upper limit of 10 S10 blue. Earth bound observations made by Bruman (1969) with the 48-inch Palomar Schmidt telescope gave no indication for discrete objects nor for clouds.

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12 Motion about the libration points

Stationkeeping controllers for Earth–Moon L1 and L2 libration points halo orbits

Explicit solution and resonance dynamics around triangular libration points of the planar elliptic restricted three-body problem

Effect of Perturbations in Coriolis and Centrifugal Forces on Libration Points in the Restricted Six-Body Problem

Effect of three-body interaction on the topology of basins of convergence linked to the libration points in the R3BP

Stability of the libration points of a rotating triaxial ellipsoid

Families of impulsive transfers between libration points in the restricted three-body problem

Global sensitivity to velocity errors at the libration points

Solving Stellar Astronomy Problems in the Orbital Stellar Stereoscopic Observatory Project

Numerical orbits near the triangular lunar libration points

1.3.5 On the Visibility of the Libration Clouds

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