John B. Murray: Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. In: Monthly Notices of the Royal Astronomical Society. 309. Jahrgang, Nr.1, 11. Oktober 1999, S.31–34, doi:10.1046/j.1365-8711.1999.02806.x, bibcode:1999MNRAS.309...31M (oxfordjournals.org [PDF]). – Zitat aus dem Abstract: “Aphelion distances of long-period comets show a slight excess around 30 000 to 50 000 au … This paper examines one of the possible explanations for this non-random clustering.”
John J. Matese, Patrick G. Whitman, Daniel P . Whitmire: Cometary Evidence of a Massive Body in the Outer Oort Clouds. In: Icarus. 141. Jahrgang, Nr.2, 1999, S.354, doi:10.1006/icar.1999.6177, bibcode:1999Icar..141..354M. – Zitat aus dem Abstract: “Approximately 25% of the 82 new class I Oort cloud comets have an anomalous distribution of orbital elements that can best be understood if there exists a bound perturber in the outer Oort cloud.”
John B. Murray: Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. In: Monthly Notices of the Royal Astronomical Society. 309. Jahrgang, Nr.1, 11. Oktober 1999, S.31–34, doi:10.1046/j.1365-8711.1999.02806.x, bibcode:1999MNRAS.309...31M (oxfordjournals.org [PDF]). – Zitat aus dem Abstract: “Aphelion distances of long-period comets show a slight excess around 30 000 to 50 000 au … This paper examines one of the possible explanations for this non-random clustering.”
John J. Matese, Patrick G. Whitman, Daniel P . Whitmire: Cometary Evidence of a Massive Body in the Outer Oort Clouds. In: Icarus. 141. Jahrgang, Nr.2, 1999, S.354, doi:10.1006/icar.1999.6177, bibcode:1999Icar..141..354M. – Zitat aus dem Abstract: “Approximately 25% of the 82 new class I Oort cloud comets have an anomalous distribution of orbital elements that can best be understood if there exists a bound perturber in the outer Oort cloud.”
John B. Murray: Arguments for the Presence of a Distant Large Undiscovered Solar System Planet. In: Monthly Notices of the Royal Astronomical Society. 309. Jahrgang, Nr.1, 11. Oktober 1999, S.31–34, doi:10.1046/j.1365-8711.1999.02806.x, bibcode:1999MNRAS.309...31M (oxfordjournals.org [PDF]). – Zitat aus dem Abstract: “Aphelion distances of long-period comets show a slight excess around 30 000 to 50 000 au … This paper examines one of the possible explanations for this non-random clustering.”