prikaz prve stranice dokumenta Planetary orbits in the single star systems
  Download
PDF 170.31 KB
Scientific paper - Original scientific paper
Planetary orbits in the single star systems
Fizika B, 5 (1996), 2; 85-92. urn:nbn:hr:217:025633
Rubčić, Antun; Rubčić, Jasna

Cite this document

Rubčić, A. & Rubčić, J. (1996). Planetary orbits in the single star systems. Fizika B, 5. (2), 85-92. Retrieved from https://urn.nsk.hr/urn:nbn:hr:217:025633

Rubčić, Antun and Jasna Rubčić. "Planetary orbits in the single star systems." Fizika B, vol. 5, no. 2, 1996, pp. 85-92. https://urn.nsk.hr/urn:nbn:hr:217:025633

Rubčić, Antun and Jasna Rubčić. "Planetary orbits in the single star systems." Fizika B 5, no. 2 (1996): 85-92. https://urn.nsk.hr/urn:nbn:hr:217:025633

Rubčić, A. and Rubčić, J. (1996) 'Planetary orbits in the single star systems', Fizika B, 5(2), pp. 85-92. Available at: https://urn.nsk.hr/urn:nbn:hr:217:025633 (Accessed 11 May 2024)

Rubčić A, Rubčić J. Planetary orbits in the single star systems. Fizika B [Internet]. 1996 [cited 2024 May 11];5(2):85-92. Available at: https://urn.nsk.hr/urn:nbn:hr:217:025633

A. Rubčić and J. Rubčić, "Planetary orbits in the single star systems", Fizika B, vol. 5, no. 2, pp. 85-92, 1996. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:025633. [Accessed: 11 May 2024]

Please login to the repository to save this object to your list.
Metadata
Title (english)Planetary orbits in the single star systems
AuthorAntun Rubčić
AuthorJasna Rubčić
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
Recently, we have shown that the orbital radii of planets and major satellites could be described by the parabolic law r_n = const.×n^2, where values of n are consecutive integers. The constant depends on a particular system and includes a dimensionless factor f, which is now correlated with some relevant parameters. Using the parabolic law, we discuss a possible existence of the terrestrial- and/or Jovian-type planets in extra-solar single-star systems, assuming variable stellar mass. An extension to the pulsar PSR B1257+12, the only one with three detected planets, is considered.
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review
Publication versionPublished version
Journal titleFizika B
Numberingvol. 5, no. 2, pp. 85-92
p-ISSN1330-0016
URN:NBNurn:nbn:hr:217:025633
Publication1996
Document URLhttp://fizika.hfd.hr/fizika_b/bv96/b5p085.htm
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Created on2019-10-04 14:19:17