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Talk:Simeis 147

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This is an old revision of this page, as edited by Morbas (talk | contribs) at 08:24, 22 November 2019 (File:Simeis 147.jpg to appear as POTD soon). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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File:Simeis 147.jpg to appear as POTD soon

Hello! This is a note to let the editors of this article know that File:Simeis 147.jpg will be appearing as picture of the day on July 29, 2017. You can view and edit the POTD blurb at Template:POTD/2017-07-29. If this article needs any attention or maintenance, it would be preferable if that could be done before its appearance on the Main Page. — Chris Woodrich (talk) 05:33, 20 July 2017 (UTC)[reply]

Simeis 147
Simeis 147, also known as the Spaghetti Nebula, is a supernova remnant (SNR) in the Milky Way. Straddling the border between the constellations Auriga and Taurus, the nebula was discovered in 1952 at the Crimean Astrophysical Observatory. It is difficult to observe due to its extremely low brightness.Photograph: Rogelio Bernal Andreo

Galactic Coordinates b=-1.71177 L=180.04204 Translation of RA and DEC to less than 1PPM. Morbas (talk) 08:23, 22 November 2019 (UTC)[reply]