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undergraduate thesis
Keplerovi zakoni
Split: University of Split, University of Split, Faculty of science, 2018. urn:nbn:hr:166:105918
Tošić, Barbara
University of Split
Faculty of Science
Department of Physics

Institutional repository: Repository of Faculty of Science

Cite this document

Tošić, B. (2018). Keplerovi zakoni (Undergraduate thesis). Split: University of Split, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:166:105918

Tošić, Barbara. "Keplerovi zakoni." Undergraduate thesis, University of Split, Faculty of Science, 2018. https://urn.nsk.hr/urn:nbn:hr:166:105918

Tošić, Barbara. "Keplerovi zakoni." Undergraduate thesis, University of Split, Faculty of Science, 2018. https://urn.nsk.hr/urn:nbn:hr:166:105918

Tošić, B. (2018). 'Keplerovi zakoni', Undergraduate thesis, University of Split, Faculty of Science, accessed 29 December 2024, https://urn.nsk.hr/urn:nbn:hr:166:105918

Tošić B. Keplerovi zakoni [Undergraduate thesis]. Split: University of Split, Faculty of Science; 2018 [cited 2024 December 29] Available at: https://urn.nsk.hr/urn:nbn:hr:166:105918

B. Tošić, "Keplerovi zakoni", Undergraduate thesis, University of Split, Faculty of Science, Split, 2018. Available at: https://urn.nsk.hr/urn:nbn:hr:166:105918

Metadata
TitleKeplerovi zakoni
Title (english)Kepler's laws
AuthorBarbara Tošić
MentorMarko Kovač (mentor)
Committee memberMarko Kovač (predsjednik povjerenstva)
Committee memberPetar Stipanović (član povjerenstva)
Committee memberHrvoje Vrcan (član povjerenstva)
GranterUniversity of Split
Faculty of Science
(Department of Physics)
Split
Defense date and country2018-09-27, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract
Preuzimanjem eksperimentalnih podataka Tycha Brahea i svojim umijećem poznavanja Euklidove geometrije, Kepler definira tri briljantna zakona vezana za gibanje nebeskih tijela. U prvom zakonu predstavlja elipse kao prave orbite planeta. Drugi zakon tvrdi da planeti prebrišu jednake površne za jednake vremenske intervale. Treći zakon definira vezu između vremena potrebnog da planet obiđe svoju putanju jednom s velikom poluosi elipse.
Abstract (english)
By taking the experimental information from Tych Brahe and by using his knowledge of Euclid's geometry, Kepler defines three brilliant laws connected to the motion of celestial bodies. In the first law he represents ellipses as the real planet orbits. Second law claims that planets sweep out equal areas in the equal time intervals. Third law defines connection between the time in which a planet passes its trajectory once with the semi-major axis of the ellipse.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:166:105918
Study programmeTitle: Physics
Study programme type: university
Study level: undergraduate
Academic / professional title: sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike (sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike)
Type of resourceText
File originBorn digital
Access conditionsAccess restricted to students and staff of home institution
Terms of useLicence In copyright icon
Created on2018-12-14 16:10:05