Cygnus Loop in HaOIII with RGB Stars

Details
Equipment used
Object Details

The Cygnus loop can be found in the constellation Cygnus and is a supernova remnant. A supernova is a powerful and luminous explosion of a star and occurs at the end of its life cycle. In this case, the source star was approximately 20 times larger than our own sun. This source star exploded between 10'000 and 20'000 years ago. At the time, the explosion was so bright that it could be seen even during the day. The layers of this star can be seen today as nebulae. The entire remnant expanded over the years and now covers an area in the night sky about six times the diameter of the moon.The remnant consists mainly of three distinct regions. The Eastern Veil Nebula at the bottom of the image, the Western Veil Nebula at the top of the image and Pickering's Triangle between these two.

Image on Astrobin: https://www.astrobin.com/q9awbd/
Image on Instagram: https://www.instagram.com/p/C_QUwzSs0Zu/?hl=de&img_index=1

Setup
Widefield Setup

Telescope / Camera Lens
Askar FRA 500 with 0.7x Reducer

Camera
QHY 268M

Mount
Skywatcher HEQ5 Pro

Filter
Astronomik Ha, OIII and RGB

Integration Time
RGB: 33 x 240 s = 2 h 12 min
Ha: 62 x 300 s = 5 h 10 min
OIII: 63 x 300 s = 5 h 15 min


Total: 12 h 37 min

Comments
-

Type of Main Object
Supernova Remnant

Constellation
Cygnus

Observation Site
Goldau, CH
Bortle Class 4

Date
22. - 23. August 2024

annotated
starless

Astrophotography by Sven Arnold

Copyright

Most of my images and documents are in the public domain and can be used freely. Images that cannot be used freely are marked accordingly (copyright). Within the public domain, you also do not have to name me if you publish one of my images or documents, although you can do so if you wish. 

So if you want to use my images and documents, please do so.