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NGC 6910 Ha, Duane Melvin
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NGC 6910 Ha

Getting plate-solving status, please wait...
NGC 6910 Ha, Duane Melvin
Powered byPixInsight

NGC 6910 Ha

Equipment

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Acquisition details

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Description

150 subs 120 Seconds each exposure    5 Hours integration

QHY 268m camera   Gain 37 Offset 5    APS-C sensor  -15C    
10 darks at 120 Seconds each
Antlia Ha 3nM filter, 2-inch diameter, mounted

Bortle 5  Sky   ambient temp  51 Degrees F     5-21-2023

Esprit 100ED  triplet refractor     100mm x 550mm no reduction
Using the field flattener supplied by Skywatcher

EQ6R PRO Mount with pier extersion

QHY seven-position filter wheel

Guiding by Orion Starshoot Autoguider TM camera with Orion 80mm x 300mm doublet refractor
Direct ST4 to mount using PHD software

Hand focusing using Bahtoniv mask
Synscaninit observation site cell app

Astro Photography Tool  APT    image capture
Deep Sky Stacker
Pixinsight
Adobe Photoshop
Adobe Lightroom

Star Talk

NGC 6910 is an open cluster in the constellation Cygnus. It was discovered by William Herschel on October 17, 1786. The cluster was also observed by John Herschel on September 18, 1828. It is a poor cluster with prominent central concentration and Trumpler class I2p.=10.5px  NGC 6910 is the core cluster of the stellar association Cygnus OB9.  NGC 6910 is located half a degree east-northeast of Gamma Cygni, also known as Sadr. It may be physically related to the nebulaIC 1318 (also known as the Gamma Cygni Nebula) as it lies at a similar distance, behind the galactic Great Rift. Cygnus OB9 is located within the Orion Arm of the Milky Way. Cygnus OB9's dimensions in the sky are 2.5 degrees by 1.5 degrees, which corresponds to its distance of 175×105 light-years across. It includes many OB stars, along with supergiant stars, like the red supergiantRW Cygni.[7] Gamma Cygni is a foreground star, lying at a distance of approximately 1,500 light years.

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NGC 6910 Ha, Duane Melvin