Heart, Soul and Double Cluster (Lorenzo Palloni)

Celestial hemisphere: Northern · Constellation: Cassiopeia (Cas) · Contains: IC 1795 · IC 1805 · IC 1831 · IC 1848 · NGC 1027 · NGC 869 · NGC 884 · NGC 896 · NGC 957 · The star 11Per · The star 7Per · The star 8Per · The star 9Per · The star ηPer · chi Persei Cluster · h Persei Cluster

Heart, Soul and Double Cluster

After a long time, I could use again my Star Adventurer, finally far from the LP of my city.
My expectations for the night were so high! I prepared every detail carefully in the days before.
So I reached the place, about 900 meters, likely B5 (a paradise compared to my B9 class).
I went there with very clear in mind what I wanted: Heart, Soul and Double Cluster. Yes, for this 1 year-waited trip the name was perfect: Heart & Soul.
Finally I could frame something to North, invisible from by backyard.
I enjoyed a lot to prepare the gear in the peaceful nature. The night was pleasant, perfect climate, not like the hot cities.

Not everything was golden like the beautiful sunset: I wasted the first hour with some issues.
The platesolve did not work (solved later, at the end of the night...), so I had to manually frame this image; probably simple for an expert itinerant AP but not for me, as from my backyard I use only platesolve. It was great when I could frame it exactly like I had in mind, without so many troubles (in the single frames the nebulae are totally invisible. This was, by the way, totally disappointing and I was also worried for the future image - indeed...).

Very quick postprocessing, I wanted something simple like simple was the gear used:
Canon 6D (no mod), Canon 70-200 @200mm f/5.6. No filters.

It was a great night. I will do better image next time.
Thanks for watching.

Original
B
Final
C

Imagers of Italy
The OSC Club (One Shot Camera)
Camera Lens Astrophotography

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Status	Basic success
Started	...
Astrometry.net job	4827091
PixInsight job	n/a
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Heart, Soul and Double Cluster

Heart, Soul and Double Cluster

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Heart, Soul and Double Cluster

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