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undergraduate thesis
24 460 svjetlosnih godina od Zemlje
2024. urn:nbn:hr:166:057719
Kusanović, Dora
University of Split
Faculty of Science

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Kusanović, D. (2024). 24 460 svjetlosnih godina od Zemlje (Undergraduate thesis). Split: University of Split, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:166:057719

Kusanović, Dora. "24 460 svjetlosnih godina od Zemlje." Undergraduate thesis, University of Split, Faculty of Science, 2024. https://urn.nsk.hr/urn:nbn:hr:166:057719

Kusanović, Dora. "24 460 svjetlosnih godina od Zemlje." Undergraduate thesis, University of Split, Faculty of Science, 2024. https://urn.nsk.hr/urn:nbn:hr:166:057719

Kusanović, D. (2024). '24 460 svjetlosnih godina od Zemlje', Undergraduate thesis, University of Split, Faculty of Science, accessed 23 January 2025, https://urn.nsk.hr/urn:nbn:hr:166:057719

Kusanović D. 24 460 svjetlosnih godina od Zemlje [Undergraduate thesis]. Split: University of Split, Faculty of Science; 2024 [cited 2025 January 23] Available at: https://urn.nsk.hr/urn:nbn:hr:166:057719

D. Kusanović, "24 460 svjetlosnih godina od Zemlje", Undergraduate thesis, University of Split, Faculty of Science, Split, 2024. Available at: https://urn.nsk.hr/urn:nbn:hr:166:057719

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Metadata
Title24 460 svjetlosnih godina od Zemlje
Title (english)24 460 light-years from Earth
AuthorDora Kusanović
MentorMarko Kovač (mentor)
MentorTamara Rom (pomoć pri izradi, neposredni voditelj)
Committee memberMarko Kovač (predsjednik povjerenstva)
Committee memberMarin Vojković (član povjerenstva)
Committee memberTamara Rom (član povjerenstva)
GranterUniversity of Split
Faculty of Science
Split
Defense date and country2024-09-26, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract
Zvjezdani su skupovi nakupine velikog broja zvijezda. Kuglasti su skupovi pravilnog oblika zbog djelovanja gravitacijske sile te se takvi skupovi najčešće nalaze u galaktičkom halou. Zvijezde koje pripadaju istom skupu nastaju u isto vrijeme i imaju neke zajedničke značajke što omogućava identifikaciju članova skupa, a time i određivanje starosti te udaljenosti od Zemlje. Korištenjem teleskopa Celestron Nexstar Evolution 8 i monokoromatske kamere ZWO ASI294MM Pro fotografira se kuglasti skup Messier 5 (M5, NGC 5904), jedan od najstarijih skupova u Mliječnoj stazi. Za određivanje članova skupa M5 koriste se podaci o paralaksi, magnitudi i gibanju skupa sa satelita Gaia te se podaci grafički prikazuju u programu TOPCAT.
Abstract (english)
Stellar clusters are large groups of stars. Globular clusters have a regular shape due to the gravitational force and such clusters are usually found in galactic halos. The stars that belong to the same cluster are formed at the same time and have some features in common which makes it possible to identify the members of the cluster, and thus to determine their age and distance from Earth. The globular cluster Messier 5 (M5, NGC 5904), one of the oldest clusters in the Milky Way, is photographed using the Celestron Nexstar Evolution 8 telescope and monochromatic camera ZWO ASI294MM Pro. The data on parallax, magnitude and motion on the celestial sphere are obtained from the Gaia satellite to determine the members of the cluster M5, and the data graphically viewed in TOPCAT software.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:166:057719
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 conditionsOpen access
Terms of useLicence In copyright icon
Created on2024-10-29 12:11:28