You are viewing an obsolete version of the DU website which is no longer
supported by the Administrators.
Visit
The New DU. Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud
[View All]
Fumesucker
(1000+ posts)
Send PM |
Profile |
Ignore
|
Fri May-07-10 04:58 PM
Original message |
| Persistent Evidence of a Jovian Mass Solar Companion in the Oort Cloud |
|
http://www.spaceref.com/news/viewsr.html?pid=33991We present an updated dynamical and statistical analysis of outer Oort cloud cometary evidence suggesting the sun has a wide-binary Jovian mass companion. The results support a conjecture that there exists a companion of mass ~ 1-4 M_Jup orbiting in the innermost region of the outer Oort cloud. Our most restrictive prediction is that the orientation angles of the orbit normal in galactic coordinates are centered on the galactic longitude of the ascending node Omega = 319 degree and the galactic inclination i = 103 degree (or the opposite direction) with an uncertainty in the normal direction subtending ~ 2% of the sky. A Bayesian statistical analysis suggests that the probability of the companion hypothesis is comparable to or greater than the probability of the null hypothesis of a statistical fluke. Such a companion could also have produced the detached Kuiper Belt object Sedna. The putative companion could be easily detected by the recently launched Wide-field Infrared Survey Explorer (WISE).
|
Powered by DCForum+ Version 1.1 Copyright 1997-2002 DCScripts.com
Software has been extensively modified by the DU administrators
Important Notices: By participating on this discussion
board, visitors agree to abide by the rules outlined on our Rules
page. Messages posted on the Democratic Underground Discussion Forums are the
opinions of the individuals who post them, and do not necessarily represent
the opinions of Democratic Underground, LLC.
Printer-friendly format
Email this thread to a friend
Bookmark this thread