Pair-correlation analysis of HD 10180 reveals a possible planetary orbit at about 0.92 AU
arXiv:1009.5507
Abstract
The pair-correlations between the positions of the six known planets in the exoplanetary system HD 10180 are studied. There are six non-trivial and almost equally spaced peaks. This demonstrates longer-ranged positional order between the orbits and suggests a seventh orbit at 0.92 AU that is consistent with these correlations.
arXiv comment5 pages, 4 figures
References in corpus (4)
- Discovery of a Cool Planet of 5.5 Earth Masses Through Gravitational Microlensing
- The HARPS search for southern extra-solar planets XVIII. An Earth-mass planet in the GJ 581 planetary system
- The HARPS search for southern extra-solar planets. XXVII. Up to seven planets orbiting HD 10180: probing the architecture of low-mass planetary systems
- The Exo-planetary System of 55 Cancri and the Titius-Bode Law