M77 is one of the best‑known active galaxies in the Messier catalogue.
It contains a powerful Seyfert II nucleus, driven by a supermassive black hole that emits enormous amounts of energy.
Around the core lie complex gas structures, ionisation regions, and dust lanes that become beautifully visible in deep exposures.
The spiral arms are rich in star formation and show a mix of blue young clusters and red dust zones.
Object Data
Messier:M77
NGC:NGC 1068
Also known as:Cetus A, Arp37
Name:Active (Seyfert) Spiral Galaxy
Type:Seyfert II spiral galaxy (SA(rs)b)
Constellation:Cetus
Size:7.1′ × 6.0′
Distance:47 million ly
Observation Data
Location:Pollux Observatory, Zuidlaren
Date:2024-10-05
Technical Data
Exposure time:L-50 x 180 sec R-30 x 180 sec G-25 x 180 sec B-25 x 180 sec Total: 6.5 h