Classical methods of orbit determination

dc.contributor.advisor	Figueras Siñol, Francesca
dc.contributor.advisor	Santana-Ros, Toni
dc.contributor.author	Prat Baucells, Roger
dc.date.accessioned	2022-09-07T14:49:33Z
dc.date.available	2022-09-07T14:49:33Z
dc.date.issued	2022-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutors: Francesca Figueras, Toni Santana-Ros	ca
dc.description.abstract	This work’s main goal is to study the classical methods of orbit determination developed by Gauss and Laplace. To do so, simulations of objects orbiting the Earth have been programmed to test these methods and compare the results. They show poor accuracy and don’t allow for predictions in the studied cases, but they improve for large enough orbits where they could be a first approach for more complex orbit determination schemes	ca
dc.format.extent	5 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/188769
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Prat, 2022
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Treballs Finals de Grau (TFG) - Física
dc.subject.classification	Òrbites	cat
dc.subject.classification	Mecànica celeste	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Orbits	eng
dc.subject.other	Celestial mechanics	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Classical methods of orbit determination	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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