Informationen (Wikipedia): IC 1318, auch als γ-Cygni-Nebel (Gamma-Cygni-Nebel) oder Schmetterlingsnebel bezeichnet, ist ein Emissionsnebel und H-II-Gebiet im Sternbild Schwan. Der Nebel befindet sich zirka 4’900 Lichtjahre von der Erde entfernt und hat eine Ausdehnung von 100 Lichtjahren. Im Zentrum des Nebels liegt der Stern Sadr, mit einer Entfernung von 1’500 Lichtjahren. IC 1318 wird in die drei Teile IC 1318 A, IC 1318 B und IC 1318 C eingeteilt, die sich voneinander unterscheiden. IC 1318 B und IC 1318 C werden von der 20 Lichtjahre breiten Dunkelwolke LDN 889 getrennt.
Aufnahmedaten: September 2-24 2023 und September 2-16 2024
Aufnahmedetails:
Hydrogen-Alpha : 586 x 120 sec + 61 x 300 sec (24.6h)
Color (Foraxx) & Luminance (Ha) combination – Photoshop
Color and Contrast Post-Processing (Photoshop)
Copyright: Basilio Noris
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