Yet another "discovery" dealing with something we studied years ago.
A Japanese team had concluded, over a decade ago (following a statistical study of whatever few Oort cloud and Kuiper belt objects knows at the time) that there should be one or two more planets (real ones, not snowballs the size of Pluto) left to be discovered.
The article you cite is based on a paper published in 1999, a few years after the Japanese results.
It simply say that the present distribution of lop-sided orbits COULD be explained by the presence of a large planet (this is not difficult to believe, especially in light of the earlier Japanese results); the part that might be pushing it ever so slightly is the "could be larger than Jupiter" and the sprinkling of "may" throughout the article.
The authors were still pushing the idea of a brown dwarf. This has pretty well been dropped, as a brown dwarf at such a short distance from us would have been detected with the latest infra-red telescopes (we can detect brown dwarfs that small at hundreds of light-years).
Also, our modern understanding of brown dwarf would not have accepted their "putative" object with a mass of only 50% bigger than Jupiter as a brown dwarf. Given the super-Jupiters found around other stars, this object -- if it exists at all -- would just be a fat-jupiter.
Icarus is a professional astronomy journal. It is reliable and the papers are peer-reviewed. Therefore the information is reliable and the data would have been checked to make sure that others also see the same kinds of distributions of orbits (for example). It does represent the information as it was known at the time. Careful reading of the paper itself would probably reveal that the article by the Mail online contains a few... how could we say politely... enhancements.
The world of astronomy has abandoned the idea of a brown dwarf that close to us. The idea that there could still be one or two large planets out there is still valid.
The posting linking this to 2012 is, of course, ludicrous. However, the charlatan behind the Big 2012 Hoax have always liked the "Brown Dwarf" scenario.
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(From a search using Scholar.Google.com)
Icarus, Volume 141, Issue 2, October 1999, Pages 354-366
Cometary Evidence of a Massive Body in the Outer Oort Clouds
J. J. Matese1, P. G. Whitman and D. P. Whitmire
Department of Physics, University of Louisiana at Lafayette, Lafayette, Louisiana, 70504-4210, f1
Received 9 September 1998;
revised 11 March 1999.
Available online 2 April 2002.
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. Statistically significant correlated anomalies include aphelia directions, energies, perihelion distances, and signatures of the angular momentum change due to the Galaxy. The perturber, acting in concert with the galactic tide, causes these comets to enter the loss cylinder—an interval of Oort cloud comet perihelion distances in the planetary region which is emptied by interactions with Saturn and Jupiter. More concisely, the impulse serves to smear the loss cylinder boundary inward along the track of the perturber. Thus it is easier for the galactic tide to make these comets observable. A smaller number of comets are directly injected by the impulsive mechanism. We estimate that the perturber–comet interactions take place at a mean distance of ≈25,000 AU. The putative brown dwarf would have a mass of 3 / 2 MJupiter and an orbit whose normal direction is within 5° of the galactic midplane. This object would not have been detected in the IRAS database, but will be detectable in the next generation of planet/brown dwarf searches, including SIRTF. It is also possible that its radio emissions would make it distinguishable in sensitive radio telescopes such as the VLA.
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bound perturber = object in orbit around our Sun, massive enough to cause perturbations in the Oort cloud.
They did take into account the tidal perturbations due to the Galaxy
loss cylinder = a zone of lesser density, in the Oort cloud, where objects are moved away because of periodic interference by Jupiter and Saturn (there are equivalent "gaps" in the main asteroid belt).
VLA = Very Large Array, a set of many radio-telescopes linked together to enhance their performance.