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Optimization of Artificial Neural Networks models applied to the identification of images of asteroids' resonant arguments. (arXiv:2207.14181v3 [astro-ph.EP] UPDATED)
cs.LG updates on arXiv.org arxiv.org
The asteroidal main belt is crossed by a web of mean-motion and secular
resonances, that occur when there is a commensurability between fundamental
frequencies of the asteroids and planets. Traditionally, these objects were
identified by visual inspection of the time evolution of their resonant
argument, which is a combination of orbital elements of the asteroid and the
perturbing planet(s). Since the population of asteroids affected by these
resonances is, in some cases, of the order of several thousand, this has …
artificial artificial neural networks arxiv asteroids astro identification images networks neural networks optimization