Stars and other bodies follow orbits as they move inside galaxies. In some cases, predicting and modeling these kinds of orbits can be difficult because of the complex distribution of mass in the galaxy. In situations where bodies follow complex orbits that are difficult to model, large amounts of computer calculations may be necessary. This article proposes a new method to help identify orbits that can be difficult to predict by using a new faster method which can help astronomers research this complex topic.
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