06/02/2026
Wolf-Rayet 134 within the hydrogen emission nebula NGC 6883. A Wolf-Rayet star is an incredibly hot star that is often surrounded by a "bubble" of excited hydrogen (red) or oxygen (blue). In this case the bubble is oxygen, and this image captures just one side of the bubble -- the other side is much dimmer and harder to capture.
WR-134 is in the constellation Cygnus, and is about 6,100 light-years away. The photons emitted by that excited oxygen have been travelling since about the time of the creation of the Earth according to Bishop Usher (who based his chronology on an analysis of the age of patriarchs in the Old Testament all the way back to Adam). Or, since the time of the use of proto-cuneiform writing in ancient Sumer.
56 x 300-sec exposures (plus 30 flats & bias frames, 20 darks)
4 hr 40 min total exposure
Bortle 4 sky
Waxing gibbous Moon, 94% illuminated
ZWO ASI533MC Pro camera (-5°C, gain 101, offset 70)
Optolong L-eNhance filter
Apertura CarbonStar RC6 telescope (1377 mm focal length)
EQ5 Pro mount (guided)
stacked and processed in Siril
Denoised and background extracted in GraXpert
tweaked in Raw Therapee and GIMP