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The Owl Nebula (also known Messier 97) is a planetary nebula located approximately 2,030 light years away in the constellation Ursa Major. When William Parsons observed the nebula in 1848, his hand-drawn illustration resembled an owl’s head. It has been known as the Owl Nebula ever since. The nebula is approximately 8,000 years old. It is approximately circular in cross-section with a little visible internal structure. The nebula is arranged in three concentric shells, with the outermost shell being about 20–30% larger than the inner shell. The owl-like appearance of the nebula is the result of an inner shell that is not circularly symmetric, but instead forms a barrel-like structure aligned at an angle of 45° to the line of sight.

Messier 108, nicknamed the Surfboard Galaxy, is a barred spiral galaxy located in the constellation Ursa Major. The galaxy lies at an approximate distance of 45.9 million light years from Earth. The galaxy is inclined 75 degrees to our line of sight. Even though it appears almost edge-on, M108 is a popular target among amateur astronomers and astrophotographers because details of its structure can be seen even in amateur telescopes.

m97+M108 seen using Celestron RASA 8 and ZWO ASI183MC