The Sadr Region (IC 1318 or the Gamma Cygni Nebula)

Posted: Oct 7th, 2021

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NGC

IC

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Technical Info

Telescope/Lens: Объктив Юпитер 37А

Camera: ZWO ASI294MC Pro (Cool)

Mount: HEQ5PRO SynScan GoTo

Guide Scope: SVBONY 60/240

Guide Camera: ZWO ASI462MC+Optolong uv/ir cut

Software: PixInsight

Accessories: ASIAIR

Exposure:

61 x 120" ISO/Gain: 120 - Optolong l-eXtreme 2"

Orange, Bortle 6 zone:

Stanica Dinskaya, Russia

Jul 1st, 2021

2 h 2 m

2269

19

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Resolution: 1280x958 px

Scale: 6691 KB

313

A diffuse emission nebula surrounds Sadr (γ Cygni) at the center of the cross. The Sadr region is one of the surrounding nebulous areas; others include the Butterfly Nebula and the Crescent Nebula. It contains numerous dark nebulae in addition to diffuse emission nebulae.

Sadr itself has an apparent magnitude of approximately 2.2. The nebulous regions around the area are also quite bright.

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