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{{wrongtitle|Radio source SHGb02+14a}} | {{wrongtitle|title=Radio source SHGb02+14a}} | ||
'''SHGb02+14a''' is an interesting radio source and candidate in the ] discovered by ] and announced in '']'' on ], ]. This weak source was observed three times at 1420 megahertz. There is no star within 1000 ]s of its direction. | '''SHGb02+14a''' is an interesting radio source and candidate in the ] discovered by ] and announced in '']'' on ], ]. This weak source was observed three times at 1420 megahertz. There is no star within 1000 ]s of its direction. |
Revision as of 13:47, 22 October 2004
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.