Planetary orbits in single star systems.

Details Planetary orbits in single star systems. Planetary orbits in single star systems.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996fizb....5...85r&link_type=abstract

Fizika B, Vol. 5, No. 2, p. 85 - 92

Computer Science

Planetary Companions: Stars, Planetary Companions: Pulsars

Scientific paper

Recently, it has been shown that the orbital radii of planets and major satellites could be described by the parabolic law rn = const.×n2, 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, the authors 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.

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