This is an old revision of this page, as edited by ZeroOne (talk | contribs) at 15:45, 26 November 2004 (megahertz). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Revision as of 15:45, 26 November 2004 by ZeroOne (talk | contribs) (megahertz)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff) The correct title of this article is Radio source SHGb02+14a. It appears incorrectly here due to technical restrictions.SHGb02+14a is an interesting radio source and candidate in the Search for Extra-Terrestrial Intelligence discovered by SETI@home and announced in New Scientist on September 1, 2004. This weak source was observed three times at 1420 megahertz. There is no star within 1000 light years of its direction. A more skeptical article concerning the discovery was written by The Planetary Society.