Automated Tour Design in the Saturnian System - presented by Yuji Takubo | Assessment of dynamical models for transitioning from the Circular Restricted Three-Body Problem to an ephemeris model with applications - presented by Beom Park

Automated Tour Design in the Saturnian System

Yuji Takubo

Assessment of dynamical models for transitioning from the Circular Restricted Three-Body Problem to an ephemeris model with applications

Beom Park

Beom ParkYuji Takubo
Slide at 34:57
Beom Park
Pulsating-Rotating Frame [1]
[1] Gómez, G., Masdemont, J.J., & Mondelo, J. M. (2002). Solar system models with a selected set of frequencies. Astronomy & Astrophysics, 390(2), 733-749 https://doi.org/10.1051/0004-6361:20020625
Inertial frame
Pulsating-rotating frame
1 [n.d.]
1
References
  • 1.
    G. Gómez et al. (2002) Solar system models with a selected set of frequencies. Astronomy & Astrophysics
Share slide
Summary (AI generated)

We will leverage the second frame, the Pulsating Rotating Frame, to host various dynamical models and create hierarchy within that frame. Initially, we will examine the rotation formula between the capital R vector and the rho vector. The capital R vector represents the inertial frame, the dimensional position vector of the spacecraft, while the rho vector represents the pulsating rotating frame, the non-dimensional spacecraft vector. The Rotation Formula includes three components: translation of the origin, dimensionalization of the length, and rotation represented by the Direction Cosine Matrix.