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undergraduate thesis
Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita
2022. urn:nbn:hr:200:881564
Jančić, Tin
Josip Juraj Strossmayer University of Osijek
Faculty of Electrical Engineering, Computer Science and Information Technology Osijek
Department of Software Engineering
Chair of Visual Computing

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Jančić, T. (2022). Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita (Undergraduate thesis). Osijek: Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek. Retrieved from https://urn.nsk.hr/urn:nbn:hr:200:881564

Jančić, Tin. "Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita." Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek, 2022. https://urn.nsk.hr/urn:nbn:hr:200:881564

Jančić, Tin. "Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita." Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek, 2022. https://urn.nsk.hr/urn:nbn:hr:200:881564

Jančić, T. (2022). 'Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita', Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek, accessed 05 April 2025, https://urn.nsk.hr/urn:nbn:hr:200:881564

Jančić T. Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita [Undergraduate thesis]. Osijek: Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek; 2022 [cited 2025 April 05] Available at: https://urn.nsk.hr/urn:nbn:hr:200:881564

T. Jančić, "Analiza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita", Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Faculty of Electrical Engineering, Computer Science and Information Technology Osijek, Osijek, 2022. Available at: https://urn.nsk.hr/urn:nbn:hr:200:881564

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Metadata
TitleAnaliza svjetlosnih krivulja zvijezda za detekciju ekstrasolarnih planeta metodom tranzita
Title (english)Light curve analysis for detection of extrasolar planets using transit method
AuthorTin Jančić
MentorIrena Galić (mentor)
Committee memberIrena Galić (predsjednik povjerenstva)
Committee memberGoran Knežević (član povjerenstva)
Committee memberJosip Job (član povjerenstva)
GranterJosip Juraj Strossmayer University of Osijek
Faculty of Electrical Engineering, Computer Science and Information Technology Osijek
(Department of Software Engineering)
(Chair of Visual Computing)
Osijek
Defense date and country2022-05-18, Croatia
Scientific / art field,
discipline and subdiscipline		TECHNICAL SCIENCES
Computing
Data Processing
Abstract
Metoda tranzita je metoda za otkrivanje ekstrasolarnih planeta. Analiziraju se svjetlosne krivulje zvijezda koje se promatraju duži vremenski period te se traži karakteristični pad u jačini svjetlosti zvijezde koji se događa periodički. Na taj način može se utvrditi gravitacijski utjecaj zvijezde na objekt do te mjere da on kruži oko spomenute zvijezde. Ukoliko je masa objekta dovoljno velika i ukoliko dovoljno dugo kruži oko zvijezde, sustav objekta, tj. planeta i zvijezde postaje stabilan i može se zaključiti da se radi o stalnom planetu tog sustava. U radu je napravljena analiza 5088 zvijezda koje su promatrane 80 dana putem NASA-inog Kepler teleskopa. Podaci su uneseni u tablice koje se referencira u napisanom kodu te se pravi analiza i vizualizacija dobivenih vrijednosti teleskopa. Od 5088 promatranih zvijezda, 38 zvijezda se trenutno smatra kandidatima za zvijezde oko kojih kruži jedan ili više ekstrasolarni planet.
Abstract (english)
The transit method is a method for detecting extrasolar planets. The light curves of stars that are observed over a longer period of time are analyzed and a characteristic drop in the light intensity of the star that occurs periodically is sought. In this way, the gravitational influence of the star on the object can be determined to the extent that it orbits the said star. If the mass of the object is large enough and if it orbits the star long enough, the system of the object, i.e. the planet and the star, becomes stable and it can be concluded that it is a permanent planet of that system. The paper analyzed 5088 stars that were observed for 80 days by NASA's Kepler telescope. The data is entered into tables that are referenced in the written code, and the obtained telescope values ​​are analyzed and visualized. Of the 5088 observed stars, 38 stars are currently considered candidates for stars orbiting one or more extrasolar planets.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:200:881564
Study programmeTitle: Undergraduate University Study Programme in Computer Engineering
Study programme type: university
Study level: undergraduate
Academic / professional title: sveučilišni/a prvostupnik/ prvostupnica (baccalaureus/baccalaurea) inženjer/inženjerka računarstva (sveučilišni/a prvostupnik/ prvostupnica (baccalaureus/baccalaurea) inženjer/inženjerka računarstva)
Type of resourceText
File originBorn digital
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Created on2022-09-06 13:36:18