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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).
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.
For a solar system object and a period of time, get the object's ephemerides from JPL Horizons, and display them as a (complex) plot showing the visibility and observability of the object.
Este proyecto mediante peticiones realizadas a la API de COPS, y herramientas de Web scraping para los datos del MPC, extráe la información determinante del cometa solocitado, para luego procesar la información y finalmente entregar las curvas seculares de luz.
kepler is a C and Python astronomy library. It implements VSOP87 for the planets, ELP 2000-82B for the Moon, minor body calculations using the MPC database, IAU precession & nutation models, rise/transit/set, Moon phase, eclipse, and equinox/solstice calculations.