Celestial hemisphere:  Northern  ·  Constellation: Pegasus (Peg)  ·  Contains:  NGC 7497
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NGC 7497 behind the molecular cloud MBM 54, Alex Woronow
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NGC 7497 behind the molecular cloud MBM 54

Getting plate-solving status, please wait...
NGC 7497 behind the molecular cloud MBM 54, Alex Woronow
Powered byPixInsight

NGC 7497 behind the molecular cloud MBM 54

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NGC 7497 behind the molecular cloud MBM 54OTA:……………….PlaneWave 17” f/6.8Camera:………….FLI ML16803Observatory:…. Deep Sky West, Chile EXPOSURES:                …R….…30 x 300 sec.                                        …G…….20 x 300 …B…....36 x 300                 …L…...116 x 300 Total exposure 16.8 hours Image Width: 39 arc-minutesProcessed by Alex Woronow (2021) using PixInsight, Topaz, 3DLUT, SWT Partially concealed by an anatomizing swarm of a black and dimly lit nebula in our Milky Way lies the distant spiral galaxy NGC 7497. The dust and gas clouds, MBM 54 (part of the Integrated Flux Nebula) in our galaxy, lies maybe 1,000 light-years from us; the galaxy is about 60,000,000 light-years distant. Several other small, distant galaxies hide behind the cloud as well. Much of the molecular cloud MBM 54 receives faint illumination from the general background of stars. Still, a close look at the image shows almost pitch-black and starless regions of nearly unilluminated nebula. Although quite apparently, cloud densities vary significantly in this region, and some gas streamers have been found, there is no evidence for star formation. The streamers have been attributed to shock waves generated, perhaps, when denser regions with the cloud collide (Sakamoto, 1999). Many such streamers appear in this image.

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NGC 7497 behind the molecular cloud MBM 54, Alex Woronow