Data for "Investigating temporary capture in the Sun-Jupiter three-body system via Lagrangian coherent structures"

The supplementary online materials for the paper "Investigating temporary capture in the Sun-Jupiter three-body system via Lagrangian coherent structures" consist of two parts.

Part 1: Coordinates of the LCS Surfaces in Figure 8

This part contains the coordinates of the local maxima of FTLE (Finite-Time Lyapunov Exponent) values that compose the Lagrangian Coherent Structures (LCS) surface presented in Figure 8 of the paper. These coordinates are crucial for understanding the formation and characteristics of the LCS in the three-body system.

Part 2: Orbital States of Asteroid 2002 GV28 Based on the High-Fidelity Ephemeris Model from Section 2.2 of the Paper

This part includes the orbital states of asteroid 2002 GV28, propagated using a high-fidelity ephemeris model as described in Section 2.2 of the paper. The data provides information on the asteroid's state in two different coordinate systems:

Heliocentric J2000.0 Ecliptic Coordinate System:

This dataset includes the position and velocity of the asteroid relative to the Sun at various time steps.

The columns typically include: Time (Julian Date), X (km), Y (km), Z (km), Vx (km/s), Vy (km/s), Vz (km/s).

Sun-Jupiter Rotating Coordinate System:

This dataset provides the position and velocity of the asteroid relative to the Sun-Jupiter rotating frame.

The columns typically include: Time (Julian Date), X (normlized), Y (normlized), Z (normlized), Vx (normlized), Vy (normlized), Vz (normlized).

Each entry in these datasets corresponds to specific time steps during the propagation, providing a comprehensive view of the asteroid's trajectory in both coordinate systems.