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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

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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 30 December 2024)

Rubčić A, Rubčić J. Planetary orbits in the single star systems. Fizika B [Internet]. 1996 [cited 2024 December 30];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: 30 December 2024]

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