M16 - Eagle Nebula (HST)
The Eagle Nebula (also known as M 16) is part of a diffuse emission nebula, or H II region, which is catalogued as IC 4703. This region of active current star formation is about 5700 light-years distant. A spire of gas that can be seen coming off the nebula in the northeastern part is approximately 9.5 light-years or about 90 trillion kilometers long.
SPECIFICATIONS
Telescope
..........................................................................................................................................................................................................................
Telescope
Planewave CDK24
Camera
..........................................................................................................................................................................................................................
Location
..........................................................................................................................................................................................................................
Date of observation
..........................................................................................................................................................................................................................
Date of observation
29.10.2020
Filters
..........................................................................................................................................................................................................................
Filters
Astrodon Ha OIII SII
Processing
..........................................................................................................................................................................................................................
Processing
DSS, Siril, Photoshop, Pixinsight
Credits
..........................................................................................................................................................................................................................
