Simulering av Oorts moln och nära planeter

Examensarbete för kandidatexamen

Please use this identifier to cite or link to this item: https://hdl.handle.net/20.500.12380/199644
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dc.contributor.authorStrömbeck, Frida
dc.contributor.authorBore, Alexander
dc.contributor.authorRizk, Charbel
dc.contributor.authorEkdahl, Calle
dc.contributor.departmentChalmers tekniska högskola / Institutionen för teknisk fysiksv
dc.contributor.departmentChalmers University of Technology / Department of Applied Physicsen
dc.date.accessioned2019-07-03T13:24:13Z-
dc.date.available2019-07-03T13:24:13Z-
dc.date.issued2014
dc.identifier.urihttps://hdl.handle.net/20.500.12380/199644-
dc.description.abstractAbstract To examine the influence of different surroundings on cometary orbits we used computer simulations. They showed that there are at least two different sources for the comets that make up the Oort cloud. They also showed that the galactic tide and star passages can send comets of the Oort cloud into the solar system. Comets inside the solar system were also simulated, to determine whether or not Jupiter could catch them, and also to examine which way to preferably avert a comet on a collision course towards Earth.
dc.language.isoeng
dc.setspec.uppsokPhysicsChemistryMaths
dc.subjectEnergi
dc.subjectFysik
dc.subjectAstronomi, astrofysik och kosmologi
dc.subjectEnergy
dc.subjectPhysical Sciences
dc.subjectAstronomy, Astrophysics and Cosmology
dc.titleSimulering av Oorts moln och nära planeter
dc.type.degreeExamensarbete för kandidatexamensv
dc.type.degreeBachelor Thesisen
dc.type.uppsokM2
Collection:Examensarbeten för kandidatexamen // Bachelor Theses



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