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Record W2099439413 · doi:10.2514/6.2006-6653

Attitude Dynamics of a Rigid Body around the Lagrangian Points

2006· article· en· W2099439413 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

Bibliographic record

VenueAIAA/AAS Astrodynamics Specialist Conference and Exhibit · 2006
Typearticle
Languageen
FieldEngineering
TopicSpacecraft Dynamics and Control
Canadian institutionsMcGill University
Fundersnot available
KeywordsDynamics (music)LagrangianComputer scienceRigid body dynamicsClassical mechanicsRigid bodyPhysicsTheoretical physicsAcoustics

Abstract

fetched live from OpenAlex

This paper explores the attitude dynamics of a small rigid satellite acted upon by the gravitational field of two massive bodies. Attitude stability of the rigid satellite is studied when it is located near the collinear and triangular Lagrangian point. Lagrangian point satellites are typically placed in periodic orbits around the specified point. It is noted that resonant attitude motion can occur if the natural frequencies associated with the attitude motion and the frequency of the Lyapunov orbit satisfy certain relationship. Attitude motion of the satellite in a halo orbit is also studied. I. Introduction HE basic Circular Restricted Three-Body Problem (CRTBP) deals with the dynamics of a point mass under the gravitational influence of two massive primary bodies, M1 and M2, that are orbiting about each other in circular orbits. Five equilibrium solutions for the CRTBP exist if the problem is set in a rotating frame of reference. These five points are named the Lagrangian points and are labeled from L 1 to L 5. The L 1, L 2, and L 3 are called the collinear points as they lie on the line joining the primary masses. The other two points, L4 and L 5, are called the triangular points as they lie on the vertex of equilateral triangles with M1 and M2 at the other vertices. In this paper the L 1 point is between M1 and M2, and the L 2 point lies beyond M2. An extension of the CRTBP substitutes a rigid body for the point mass and considers its attitude dynamics. In our solar system many interesting objects, both natural and man-made, can be found near the different Lagnangian points. Several spacecraft have orbited around the Sun-Earth L 1 point and they include the ISEEE-3 and the Genesis solar sample collector. In the near future several new space telescopes are likely to orbit the Sun-Earth L 2 point. Further down the road, it is conceivable that a space station could be constructed near the Earth-Moon L 1 in order to facilitate future lunar explorations. Located near the L 4 and L 5 of the Sun-Jupiter system are Trojan asteroids, trapped there by the gravitational forces of the Sun and Jupiter. Some previous works have explored the attitude dynamics of Lagrangian point satellites. Kane and Marsh 1 considered the attitude dynamics of an axial symmetric satellite that is spinning about its axis of symmetry, with the symmetry axis normal to the orbital plane of the primary bodies. Robinson 2,3 first studied the attitude dynamics of a dumb-bell satellite located at a triangular Lagrangian point, and later investigated the attitude stability of a satellite of arbitrary shape located at either a collinear point or a triangular point and determined the regions of stability. Misra and Bellerose 4 studied the librational dynamics of a tethered satellite located at the Earth-Moon Lagrangian points and obtained the libration frequencies. In all of the previous studies the rigid body is assumed to be held at the

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.922
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.005
GPT teacher head0.192
Teacher spread0.188 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it