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Date 2010 |
Location Mayhill, NM |
Software ACP, MaxIm DL, TheSky6 |
Mount Software Bisque Paramount ME |
Guide Atik 16IC, Astrodon MMOAG |
|
Optic OGS/RCOS 10" RC |
Camera Atik 11000C |
Filter OSC RGB |
Exposure 1200s x 27 |
Process Astroart 5, Photoshop CS5 |
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Billions and Billions.com/M77
M77 and NGC 1055 in Cetus at lower left (also designated Arp 37) was discovered by Pierre Méchain in 1780. Oriented face-on to us, it is one of the largest galaxies in the Messier catalog with a central core measuring 120,000 light-years across! Estimated to be 50-million ly from us, this barred-Sb-type spiral is a Seyfert galaxy with an extremely active core, emitting both plasma and X-rays. Most interesting is its extended arm system, with prominent dark lanes clearly visible. In the upper right corner is NGC 1055, located thirty arcseconds away. This near edge-on is also an Sb spiral and is gravitationally bound to M77 in a system which includes several other smaller galaxies. The beautiful golden-cored disk was discovered in 1783 by the great William Herschel and has a spectacular dust lane. This data set was the first acquired by my OGS R-C. Click for a larger version or return to the Gallery