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This repository contains a python code which calculates level populations and fluorescence efficiencies (g-factors) for atoms (or molecules) in the presence of a radiation field (e.g. the solar spectrum).
This is a modified version of the N-body code mercury, by J. E. Chambers, that includes the Yarkovsky and YORP effects for the dynamics of small solar system objects.
The MATLAB model here presented performs trajectory propagations based on the Constant Density Polyhedron algorithm. With this model, it is possible to compute trajectories in the proximity of astronomical bodies such as asteroids or comets. The algorithm also allows to compute ballistic trajectories.
The goal of this thesis is to calculate the required filter bandwidths of the Comet Camera (CoCa) on the Comet Interceptor mission. Reflectance of the Comet as well as the exposure time need to be taken into account.
This version of the OrbFit package contains a modified orbit9 integrator. The integrator has been modified to integrate the spin axis dynamics of small asteroids, due to the YORP effect. At the same time, the Yarkovsky effect is modified according to the dynamics of the spin axis.