Gamma Gygni, Sadr
Gamma Cygni (γ Cygni, abbreviated Gamma Cyg, γ Cyg), officially named Sadr /ˈsædər/, is a star in the northern constellation of Cygnus, forming the intersection of an asterism of five stars called the Northern Cross. Based upon parallax measurements obtained during the Hipparcos mission, it is approximately 1,800 light-years (560 parsecs) from the Sun.
SPECIFICATIONS
Telescope
..........................................................................................................................................................................................................................
Telescope
Takahashi FSQ-106ED
Camera
..........................................................................................................................................................................................................................
Location
..........................................................................................................................................................................................................................
Location
Oria, Almería, Spain
Date of observation
..........................................................................................................................................................................................................................
Date of observation
24-28 April, 2 May 2024
Filters
..........................................................................................................................................................................................................................
Processing
..........................................................................................................................................................................................................................
Processing
Pixinsight, Lr
Credits
..........................................................................................................................................................................................................................
