prikaz prve stranice dokumenta Planetary orbits in solar and extrasolar systems
  Preuzmi
PDF 244.01 KB
Znanstveni rad - Izvorni znanstveni rad
Planetary orbits in solar and extrasolar systems
Fizika A, 19 (2010), 3; 133-144. urn:nbn:hr:217:879131
Rubčić, Antun; Rubčić, Jasna

Citirajte ovaj rad

Rubčić, A. i Rubčić, J. (2010). Planetary orbits in solar and extrasolar systems. Fizika A, 19. (3), 133-144. Preuzeto s https://urn.nsk.hr/urn:nbn:hr:217:879131

Rubčić, Antun i Jasna Rubčić. "Planetary orbits in solar and extrasolar systems." Fizika A, vol. 19, br. 3, 2010, str. 133-144. https://urn.nsk.hr/urn:nbn:hr:217:879131

Rubčić, Antun i Jasna Rubčić. "Planetary orbits in solar and extrasolar systems." Fizika A 19, br. 3 (2010): 133-144. https://urn.nsk.hr/urn:nbn:hr:217:879131

Rubčić, A. i Rubčić, J. (2010) 'Planetary orbits in solar and extrasolar systems', Fizika A, 19(3), str. 133-144. Preuzeto s: https://urn.nsk.hr/urn:nbn:hr:217:879131 (Datum pristupa: 17.04.2024.)

Rubčić A, Rubčić J. Planetary orbits in solar and extrasolar systems. Fizika A [Internet]. 2010. [pristupljeno 17.04.2024.];19(3):133-144. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:879131

A. Rubčić i J. Rubčić, "Planetary orbits in solar and extrasolar systems", Fizika A, vol. 19, br. 3, str. 133-144, 2010. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:879131. [Citirano: 17.04.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:879131
Prijavite se u repozitorij kako biste mogli spremiti objekt u svoju listu.
Podaci o radu
Naslov (engleski)Planetary orbits in solar and extrasolar systems
AutorAntun Rubčić
AutorJasna Rubčić
MBZ: 2533
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
The analysis of orbital parameters of planets and main planetary satellites of the solar system, published by the present authors, suggests that the Sun's system could be a "prototype" for the distribution of orbits in extrasolar planetary systems. Owing to the recent endeavours in detecting exoplanets, it became possible and suitable to check this assumption. Particularly useful in this work are the multiple extrasolar system with at least four planets. Unfortunately, there are only four stars satisfying this requirement. At the present time eleven stars with three planets have also been observed, which may also be taken into account in reaching reasonable assertions. Quantization of orbits in the solar system by orbital number, the integer n, and quantization of the product nvn (vn is the orbital velocity) by the spacing number, integer k, is also found in extrasolar planets. It is expected that new discoveries will support the present findings.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaFizika A
Brojčani podacivol. 19, br. 3, str. 133-144
p-ISSN1330-0008
URN:NBNurn:nbn:hr:217:879131
Datum objave publikacije2010
URL dokumentahttp://fizika.hfd.hr/fizika_a/av10/a19p133.htm
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Datum i vrijeme pohrane2019-11-01 19:38:18